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LIBRARY 
UNIVERSITY  OF  CALIFORNIA. 

Deceived          /fa/ OSS  ,  i8g</ 

f  * 

tAcce&sion  No.  *7  ft 


£0    . 


OF 

TTNIVERSI' 


ABEL'S  THEOEEM  AND  THE  ALLIED  THEOKY 


INCLUDING  THE 


THEOKY  OF  THE  THETA  FUNCTIONS 


:   C.  J.  CLAY   AND  SONS, 
CAMBRIDGE   UNIVERSITY  PRESS   WAREHOUSE, 
AVE   MARIA  LANE. 

OSIaggoto :  263,  ARGYLE  STREET. 


P.  A.  BROCKHAUS. 
Hork:    THE  MACMILLAN  COMPANY. 


ABEL'S      THEOREM 


AND    THE 


ALLIED    THEOEY 


INCLUDING   THE   THEORY    OF   THE 


THETA   FUNCTIONS 


OF  THE 

UNIVERSITY 


BY 


H.    F.    BAKER,    M.A. 

FELLOW    AND    LECTURER    OF    ST    JOHN'S    COLLEGE, 
UNIVERSITY   LECTURER   IN   MATHEMATICS. 


CAMBRIDGE: 
AT  THE   UNIVERSITY   PRESS. 

1897 

[All  Rights  reserved] 


PRINTED    BY    J.    AND    C.    F.    CLAY, 
AT   THE    UNIVERSITY    PRESS. 

To      4 


^w- 


PREFACE. 


IT  may  perhaps  be  fairly  stated  that  no  better  guide  can  be  found  to  the 
analytical  developments  of  Pure  Mathematics  during  the  last  seventy  years 
than  a  study  of  the  problems  presented  by  the  subject  whereof  this  volume 
treats.  This  book  is  published  in  the  hope  that  it  may  be  found  worthy  to 
form  the  basis  for  such  study.  It  is  also  hoped  that  the  book  may  be 
serviceable  to  those  who  use  it  for  a  first  introduction  to  the  subject. 
And  an  endeavour  has  been  made  to  point  out  what ^are  conceived  to  be  the 
most  artistic  ways  of  formally  developing  the  theory  regarded  as  complete. 

The  matter  is  arranged  primarily  with  a  view  to  obtaining  perfectly 
general,  and  not  merely  illustrative,  theorems,  in  an  order  in  which  they  can 
be  immediately  utilised  for  the  subsequent  theory;  particular  results,  however 
interesting,  or  important  in  special  applications,  which  are  not  an  integral 
portion  of  the  continuous  argument  of  the  book,  are  introduced  only  so  far 
as  they  appeared  necessary  to  explain  the  general  results,  mainly  in  the 
examples,  or  are  postponed,  or  are  excluded  altogether.  The  sequence  and 
scope  of  ideas  to  which  this  has  led  will  be  clear  from  an  examination  of  the 
table  of  Contents.  fc- 

The  methods  of  Riemann,  as  far  as  they  are  explained  in  books  on  the 
general  theory  of  functions,  are  provisionally  regarded  as  fundamental ;  but 
precise  references  .are  given  for  all  results  assumed,  and  great  pains  have 
been  taken,  in  the  theory  of  algebraic  functions  and  their  integrals,  and  in 
the  analytic  theory  of  theta  functions,  to  provide  for  alternative  developments 
of  the  theory.  If  it  is  desired  to  dispense  with  Riemann's  existence  theorems, 
the  theory  of  algebraic  functions  may  be  founded  either  on  the  arithmetical 
ideas  introduced  by  Kronecker  and  by  Dedekind  and  Weber ;  or  on  the 
quasi-geometrical  ideas  associated  with  the  theory  of  adjoint  polynomials ; 
while  in  any  case  it  does  not  appear  to  be  convenient  to  avoid  reference  to 
either  class  of  ideas.  It  is  believed  that,  save  for  some  points  in  the 
periodicity  of  Abelian  integrals,  all  that  is  necessary  to  the  former  ele 
mentary  development  will  be  found  in  Chapters  IV.  and  VII.,  in  connection 
with  which  the  reader  may  consult  the  recent  -paper  of  Hensel,  Acta 
Mathematica,  xvm.  (1894),  and  also  the  papers  of  Kronecker  and  of 
B.  •  b 


V]  PREFACE. 

Dedekind  and  Weber,  Grelle's  Journal,  xci.,  xcn.  (1882).  And  it  is  hoped 
that  what  is  necessary  for  the  development  of  the  theory  from  the  elemen 
tary  geometrical  point  of  view  will  be  understood  from  Chapter  VI.,  in 
connection  with  which  the  reader  may  consult  the  Abel'sche  Functionen  of 
Clebsch  and  Gordan  (Leipzig,  1866)  and  the  paper  of  Noether,  Mathematische 
Annalen,  vii.  (1873).  In  the  theory  of  Riemann's  theta  functions,  the 
formulae  which  are  given  relatively  to  the  £  and  g>-  functions,  and  the 
general  formulae  given  near  the  end  of  Chapter  XIV.,  will  provide  sufficient 
indications  of  how  the  theta  functions  can  be  algebraically  denned ;  the 
reader  may  consult  Noether,  Mathematische  Annalen,  xxxvn.  (1890),  and 
Klein  and  Burkhardt,  ibid.  xxxn. — xxxvi.  In  Chapters  XV.,  XVII.,  and 
XIX.,  and  in  Chapters  XVIII.  and  XX.,  are  given  the  beginnings  of  that 
analytical  theory  of  theta.  functions  from  which, -in  conjunction  with  the 
general  theory  of  functions  of  several  independent  variables,  so  much  is  to 
be  hoped ;  the  latter  theory  is  however  excluded  from  this  volume. 

To  the  reader  who  does  not  desire  to  follow  the  development  of  this 
volume  consecutively  through,  the  following  course  may  perhaps  be  sug 
gested;  Chapters  I.,  II.,  III.  (in  part),  IV.,  VI.  (to  §  98),  VIII.,  IX.,  X., 
XL  (in  part),  XVIII.  (in  part),  XII. ,  XV.  (in. part);  it  is  also  possible  to 
begin  with  the  analytical  theory  of  theta  functions,  reading  in  order  Chapters 
XV.,  XVI.,  XVII.,  XIX.,  XX. 

The  footnotes  throughout  the  volume  are  intended  to  contain  the 
mention  of  all  authorities  used  in  its  preparation  ;  occasionally  the  hazardous 
plan  of  adding  to  the  lists  of  references  during  the  passage  of  the  sheets 
through  the  press,  has  been  adopted  ;  for  references  omitted,  and  for  refer 
ences  improperly  placed,  only  mistake  can  be  pleaded.  Complete  lists  of 
papers  are  given  in  the  valuable  report  of  Brill  and  Noether, "  Die  Entwicklung 
der  Theorie  der  algebraischen  Functionen  in  alterer  und  neuerer  Zeit," 
Jahresbericht  der  Deutschen  Mathematiker-Vereinigung,  Dritter  Band,  1892 — 3 
(Berlin.  Reimer,  1894);  this  report  unfortunately  appeared  only  after  the 
first  seventeen  chapters  of  this  volume,  with  the  exception  of  Chapter  XL, 
and  parts  of  VIL,  were  in  manuscript ;  its  plan  is  somewhat  different  from 
that  of  this  volume,  and  it  will  be  of  advantage  to  the  reader  to  consult 
it.  Other  books  which  have  appeared  during  the  progress  of  this  volume,  too 
late  to  effect  large  modifications,  have  not  been  consulted.  The  examples 
throughout  the  volume  are  intended  to  serve  several  different  purposes ;  to 
provide  practice  in  the  ideas  involved  in  the  general  theory ;  to  suggest  the 
steps  of  alternative  developments  without  interrupting  the  line  of  reasoning 
in  the  text;  and  to  place  important  consequences  which  are  not  utilised,  if 
at  all,  till  much  subsequently,  in  their  proper  connection. 

For  my  first  interest  in  the  subject  of  this  volume,  I  desire  to  acknowledge 
my  obligations  to  the  generous  help  given  to  me  during  Gottingen  vacations, 


PREFACE.  Vll 

on  two  occasions,  by  Professor  Felix  Klein.  In  the  preparation  of  the  book 
I  have  been  largely  indebted  to  his  printed  publications ;  the  reader  is 
recommended  to  consult  also  his  lithographed  lectures,  especially  the  one 
dealing  with  Riemann  surfaces.  In  the  final  revision  of  the  sheets  in 
their  passage  through  the  press,  I  have  received  help  from  several  friends. 
Mr  A.  E.  H.  Love,  Fellow  and  Lecturer  of  St  John's  College,  has  read 
the  proofs  of  the  volume ;  in  the  removal  of  obscurities  of  expression 
and  in  the  correction  of  press,  his  untiring  assistance  has  been  of  great 
value  to  me.  Mr  J.  Harkness,  Professor  of  Mathematics  at  Bryn  Mawr 
College,  Pennsylvania,  has  read  the  proofs  from  Chapter  XV.  onwards;  many 
faults,  undetected  by  Mr  Love  or  myself,  have  yielded  to  his  perusal ;  and 
I  have  been  greatly  helped  by  his  sympathy  in  the  subject-matter  of  the 
volume.  To  both  these  friends  I  am  under  obligations  not  easy  to  discharge. 
My  gratitude  is  also  due  to  Professor  Forsyth  for  the  generous  interest  he 
has  taken  in  the  book  from  its  commencement.  While,  it  should  be  added, 
the  task  carried  through  by  the  Staff  of  the  University  Press  deserves  more 
than  the  usual  word  of  acknowledgment. 

This  book  has  a  somewhat  ambitious  aim  ;  and  it  has  been  written  under 
the  constant  pressure  of  other  work.  It  cannot  but  be  that  .many  defects 
will  be  found  in  it.  But  the  author  hopes  it  will  be  sufficient  to  shew  that 
the  subject  offers  for  exploration  a  country  of  which  the  vastness  is  equalled 
by  the  fascination. 


ST  JOHN'S  COLLEGE,  CAMBRIDGE. 
April  26,  1897. 


CONTENTS. 
CHAPTER  I. 

THE   SUBJECT  OF   INVESTIGATION. 
§§  PAGES 

1           Fundamental  algebraic  irrationality 1 

2,    3         The  places  and  infinitesimal  on  a  Riemann  surface      .         .         .  1,    2 

4,    5         The  theory  unaltered  by  rational  transformation          .                 .'  3 — 6 
6           The  invariance  of  the  deficiency  in  rational  transformation ;  if  a 
rational   function   exists  of  order  1,  the   surface   is   of  zero 

deficiency  ...........  7,    8 

7,    8         The  greatest  number  of  irremoveable  parameters  is  3p  -  3  .         .  9,    10 

9,    10       The  geometrical  statement  of  the  theory 11,    12 

11  Generality  of  Riemann's  methods 12,    13 

CHAPTER   II. 

THE   FUNDAMENTAL   FUNCTIONS   ON   A   RlEMANN   SURFACE. 

12  Riemann's  existence  theorem  provisionally  regarded  as  fundamental  14 

13  Notation  for  normal  elementary  integral  of  second  kind           .         .  15 

14  Notation  for  normal  elementary  integral  of  third  kind    ...  15 

15  Choice  of  normal  integrals  of  the  first  kind 16 

16  Meaning  of  the  word  period.     General  remarks    .         .         .       ^.  16,    17 

17  Examples  of  the  integrals,  and  of  the  places  of  the  surface        .  18 — 20 

18  Periods  of  the  normal  elementary  integrals  of  the  second  kind         .  21 

19  The  integral  of  the  second  kind  arises  by  differentiation  from  the 

integral  of  the  third  kind 22,    23 

20  Expression  of  a  rational  function  by  integrals  of  the  second  kind    .  24 

21  Special  rational  functions,  which  are  invariant  in  rational  trans 

formation  .  25,    26 

22  Riemann  normal  integrals  depend  on  mode  of  dissection  of  the 

surface 26 

CHAPTER   III. 

THE    INFINITIES   OF   RATIONAL   FUNCTIONS. 

23  The  interdependence  of  the  poles  of  a  rational  function      .         .  27 
24,    25       Condition  that  specified  places  be  the  poles  of  a  rational  function  .         28 — 30 

26  General  form  of  Weierstrass's  gap  theorem 31,    32 

27  Provisional  statement  of  the  Riemann-Roch  theorem    ...         33,    34 


K  CONTENTS. 

§§  PAGES 

28,    29  Cases  when  the  poles  coalesce ;   the  p  critical  integers         .         .  34,    35 

30  Simple  anticipatory  geometrical  illustration  ......  36,    37 

31 — 33  The  (p-l)p(p  +  l)  places  which  are  the  poles  of  rational  functions • 

of  order  less  than  p  +  l 38 — 40 

34 — 36  There  are  at  least  2jo  +  2  such  places  which  are  distinct     .         .  41 — 44 

37  Statement  of  the  Riemann-Roch  theorem,  with  examples    .         .  44 — 46 


CHAPTER   IV. 
SPECIFICATION  OF  A  GENERAL  FORM  OF  RIEMANN'S  INTEGRALS. 

38  Explanations  in  regard  to  Integral  Rational  Functions        .         .  47,    48 

39  Definition   of  dimension  ;   fundamental   set   of  functions  for  the 

expression  of  rational  functions 48 — 52 

40  Illustrative  example  for  a  surface  of  four  sheets  .         .         .         .  53,    54 

41  The  sum  of  the  dimensions  of  the  fundamental  set  of  functions 

is  p  +  n-l 54,    55 

42  Fundamental  set  for  the  expression  of  integral  functions         .         .  55,    56 

43  Principal  properties  of  the  fundamental  set  of  integral  functions     .  57 — 60 

44  Definition  of  derived  set  of  special  functions  00,  0j,  ...,  4>n_l        .  61 — 64 

45  Algebraical  form  of  elementary  integral  of  the  third  kind,  whose 

infinities  are  ordinary  places  ;   and  of  integrals  of  the   first 

kind            .         .         .                  . 65 — 68 

46  Algebraical  form  of  elementary,  integral  of  the  third  kind  in  general  68 — 70 

47  Algebraical  form  of  integral   of  the   second  kind,  independently 

deduced 71—73 

48  The  discriminant  of  the  fundamental  set  of  integral  functions         .  74 

49  Deduction  of  the  expression  of  a  certain  fundamental   rational 

function  in  the  general  case 75 — 77 

50  The  algebraical  results   of  this   chapter  are  sufficient  to  replace 

Riemann's  existence  theorem *     .  78,    79 


CHAPTER  V. 

CERTAIN  FORMS  OF  THE  FUNDAMENTAL  EQUATION  OF  THE  RIEMANN  SURFACE. 

51  Contents  of  the  chapter 80 

52  When  p>l,   existence   of  rational   function   of  the  second  order 

involves  a  (1,  1)  correspondence 81 

53—55       Existence  of  rational  function  of  the  second   order  involves  the 

hyperelliptic  equation 81 — 84 

56,    57       Fundamental  integral  functions  and  integrals  of  the  first  kind         .  85 — 86 

58  Examples 87 

59  Number  of  irremoveable  parameters  in  the  hyperelliptic  equation  ; 

transformation  to  the  canonical  form 88 — 89 

60—63       Weierstrass's  canonical  equation  for  any  deficiency          .         .         .  90—92 


CONTENTS. 


XI 


§§ 

64—66 
67,    68 

69—71 
72—79 


Actual  formation  of  the  equation  .         .         . 

Illustrations  of  the  theory  of  integral  functions  for  Weierstrass's 

canonical  equation 

The  method  can  be  considerably  generalised    .         .     •    .         .      •  . 
Hensel's  determination  of  the  fundamental  integral  functions 


PAGES 

93—98 

99—101 
102—104 
105—112 


CHAPTER   VI. 

GEOMETRICAL  INVESTIGATIONS. 

80          Comparison  of  the  theory  of  rational  functions  with  the  theory 

of  intersections  of  curves          .         .         .         .         ...         .  113 

81 — 83       Introductory  indications  of  elementary  form  of  theory     .         .         .  113—116 

84  The  method  to  be  followed  in  this  chapter 117 

85  Treatment  of  infinity.     Homogeneous  variables  might  be  used    .  118,-   119 

86  Grade  of  an  integral  polynomial ;    number  of  terms  ;   generalised 

zeros          .  120,    121 

87  Adjoint  polynomials  ;  definition  of  the  index  of  a  singular  place     .  122 

88  Pliicker's  equations ;  connection  with  theory  of  discriminant       •    .  123,    124 
89,    90       Expression  of  rational  functions  by  adjoint  polynomials  .         .         .  125,    126 

91  Expression  of  integral  of  the  first  kind          .         .         .         .         .  127 

92  Number  of  terms   in   an   adjoint  polynomial  ;    determination   of 

elementary  integral  of  the  third  kind      .         .         ...        .  128 — 132 

93  Linear  systems  of  adjoint  polynomials  ;  reciprocal  theorem     .         .  133,    134 
94,    95       Definitions  of  set,  lot,  sequent,  equivalent  sets,  coresidual  sets         .  135 
96,    97       Theorem  of  coresidual  sets ;  algebraic  basis  of  the  theorem     .         .  136 

98          A  rational  function  of  order  less  than  p  + 1  is  expressible  by  <£- 

polynomials ,  137 

99,    100     Criticism  of  the  theory;    Cayley's  theorem  .         .'      '  .'"',    ,         .  138—141 

101 — 104     Rational  transformation  by  means  of  (^-polynomials    .         .         .  142—146 

105 — 108     Application  of  special  sets 147 — 151 

109         The  hyperelliptic  surface ;   transformation  to  canonical  form       .  152 

1.10 — 114     Whole  rational  theory  can  be  represented  by  means  of  the  invari 
ant  ratios  of  (^-polynomials  ;  number  of  relations  connecting 

these 153—159 

115 — 119     Elementary  considerations  in  regard  to  curves  in  space       .         .  160 — 167 


CHAPTER  VII. 


COORDINATION  OF  SIMPLE   ELEMENTS.     TRANSCENDENTAL   UNIFORM 

FUNCTIONS. 

Scope  of  the  chapter 168 

Notation  for  integrals  of  the  first  kind          .         .         .         .         .  169 

The  function  ^  (x,  a;  z,  cl5  ...,  cp)  expressed  by  Riemann  integrals  170,    171 

Derivation  of  a  certain  prime  function 172 

Applications  of  this  function  to  rational  functions  and  integrals  173 


Xll  CONTENTS. 

§§  PAGES 

126—128    The  function   ^(x,a-,   z,  c) ;    its  utility    for   the   expression    of 

rational  functions 174 — 176 

129         The  derived  prime  function    E(x,z);   used  to  express  rational 

functions 177 

130,    131     Algebraic    expression    of    the    functions    ^  (x,  a ;   z,  clt  ...,cp), 

ty{x,  a;  z,c) 177,    178 

132          Examples  of  these  functions;   they  determine  algebraic  expres 
sions  for  the  elementary  integrals 179 — 182 

133,  134  Derivation  of  a  canonical  integral  of  the  third  kind;  for  which 
interchange  of  argument  and  parameter  holds;  its  algebraic 
expression  ;  its  relation  with  Riemann's  elementary  normal 
integral 182—185 

135  Algebraic   theorem   equivalent  to  interchange   of  argument  and 

parameter 185 

136  Elementary  canonical  integral  of  the  second  kind         .         .         .       186,    187 

137  Applications.     Canonical  integral  of  the  third  kind  deduced  from 

the  function  ^(.v,a;  z,c^  ...,cp).     Modification  for  the  func 
tion  ty(x,  a;  z,  c) 188—192 

138  Associated  integrals  of  first  and  second  kind.     Further  canonical 

integrals.     The  algebraic  theory  of  the  hyperelliptic  integrals 

in  one  formula.         .         . 193,    194 

139,    140     Deduction  of  Weierstrass's  and  Riemann's  relations  for  periods 

of  integrals  of  the  first  and  second  kind        ....  195 — 197 

141  Either  form  is  equivalent  to  the  other 198 

142  Alternative  proofs  of  Weierstrass's  and  Riemann's  period  relations  199,    200 

143  '  Expression   of  uniform   transcendental  function  by  the  function 

ty(x,  a;  z,  c) '   .         .         .         .  201 

144,    145     Mittag-Lefner's  theorem  .         .         .         ...         .         .  202 204 

146  Expression    of  uniform   transcendental   function  in  prime  factors          205 

147  General  form  of  interchange  of  argument  and  parameter,  after 

Abel 206 


CHAPTER  VIII. 

ABEL'S  THEOREM.    ABEL'S  DIFFERENTIAL  EQUATIONS. 

148—150     Approximative  description  of  Abel's  theorem 207—210 

151  Enunciation  of  the  theorem 210 

152  The  general  theorem  reduced  to  two  simpler  theorems        .         .  211,    212 
153,    154     Proof  and  analytical  statement  of  the  theorem     ....  212 214 

155  Remark;  statement  in  terms  of  polynomials         .         .         .         .  215 

156  The   disappearance   of  the    logarithm   on   the   right  side  of  the 

equation .         .  216 

157  Applications  of  the  theorem.     Abel's  own  proof  ....  217 222 

158,    159     The  number  of  algebraically  independent  equations  given  by  the 

theorem.     Inverse  of  Abel's  theorem 222 224 

160,    161     Integration  of  Abel's  differential  equations  " 225 231 

162          Abel's  theorem  proved  quite  similarly  for  curves  in  space  .         .  231 — 234 


CONTENTS.  Xlll 

CHAPTER  IX. 

JACOBI'S    INVERSION    PROBLEM. 

§§  PAGES 

163  Statement  of  the  problem 235 

164  Uniqueness  of  any  solution 236 

165  The  necessity  of  using  congruences  and  not  equations         .         .  237 
166,    167     Avoidance  of  functions  with  infinitesimal  periods         .         .         .  238,    239 

168,    169     Proof  of  the  existence  of  a  solution 239—241 

170 — 172     Formation    of    functions    with    which    to   express    the    solution; 

connection  with  theta  functions       .  242—245 


CHAPTER   X. 

RIEMANN'S  THETA  FUNCTIONS.     GENERAL  THEORY. 

173  Sketch  of  the  history  of  the  introduction  of  theta  functions        .  246 

174  Convergence.     Notation.     Introduction  of  matrices       .         .         .  247,    248 
175,    176     Periodicity  of  the  theta  functions.     Odd  and  even  functions       .  249 — 251 

177  Number  of  zeros  is  p '.  252 

178  Position  of  the  zeros  in  the  simple  case        .        .        .        i  'orf3  253,    254 

179  The  places  TOI}  ...,  mp 255 

180  Position  of  the  zeros  in  general 256,    257 

181  Identical  vanishing  of  the  theta  functions     .....  258,    259 
182,    183    Fundamental  properties.     Geometrical  interpretation  of  the  places 

m1,...,mp •      .         .         .         .  259—267 

184 — 186     Geometrical   developments;    special   inversion   problem;    contact 

curves •    .,        tj 268 — 273 

187  Solution   of    Jacobi's   inversion   problem   by  quotients    of    theta 

functions 274,    275 

188  Theory  of  the  identical  vanishing  of  the  theta  function.     Ex 

pression  of  (^-polynomials  by  theta  functions         .         .         .  276 — 282 

189—191     General  form  of  theta  function.   Fundamental  formulae.    Periodicity  283 — 286 

192  Introduction  of  the  f  functions.  Generalisation  of  an  elliptic  formula  287 

193  Difference  of  two  f  functions  expressed  by  algebraic  integrals  and 

rational  functions       .......  288 

194 — 196     Development.    Expression  of  single  f  function  by  algebraic  integrals  289 — 292 

197,    198     Introduction  of  the  $  functions.    Expression  by  rational  functions  292-295 


CHAPTER   XI. 

THE   HYPERELLIPTIC    CASE    OF   RlEMANN'S   THETA    FUNCTIONS. 

199  Hyperelliptic  case  illustrates  the  general  theory  ....  296 

200  The  places  »i1>t..,  mp.     The  rule  for  half  periods          .         .         .       297,    298 
201,    202     Fundamental  set  of  characteristics  defined  by  branch  places       .       299—301 


XIV 


CONTENTS. 


§§  PAGES 

203          Notation.     General  theorems  to  be  illustrated       ....  302 

204,    205     Tables  in  illustration  of  the  general  theory 303—309 

206 — 213     Algebraic  expression  of  quotients  of  hyperelliptic  theta  functions. 

Solution  of  hyperelliptic  inversion  problem     .         .         .         .  309 — 317 
214,    215     Single  £  function  expressed  by  algebraical  integrals  and  rational 

functions 318 — 323 

216  Rational  expression  of  $>  function.     Relation  to  quotients  of  theta 

functions.     Solution  of  inversion  problem  by  g>  function  .         .  323 — 327 

217  Rational  expression  of  $>  function 327 — 330 

218 — 220     Algebraic  deduction    of    addition    equation    for   theta    functions 

when  p  =  2;    generalisation  of  the  equation  tr  (u+v)  a-  (u-v) 

=  cr2w.  o-V(^v-jptt) 330—337 

221  Examples  for  the  case  p  =  2.     Qopel's  biquadratic  relation  .         .  337 — 342 

CHAPTER   XII. 

A   PARTICULAR   FORM   OF   FUNDAMENTAL   SURFACE. 

222  Chapter  introduced  as  a  change  of  independent  variable,  and  as 

introducing  a  particular  prime  function          ....  343 

223—225     Definition  of  a  group  of  substitutions ;   fundamental  properties  .  343—348 

226,    227     Convergence  of  a  series ;   functions  associated  with  the  group     .  349 — 352 
228 — 232     The  fundamental   functions.     Comparison  with  foregoing  theory 

of  this  volume 353 — 359 

233 — 235     Definition  and  periodicity  of  the  Schottky  prime  function  .         .  359 — 364 

236,    237     Its  connection  with  the  theta  functions 364 — 366 

238  A  further  function  connected  therewith 367 — 372 

239  The  hyperelliptic  case     .        .        .        .        ..       .        «.       .        .  372,    373 

CHAPTER   XIII. 
RADICAL  FUNCTIONS. 

240  Introductory    . .  374 

241,    242     Expression  of  any  radical  function  by  Riemann's   integrals,  and 

by  theta  functions 375,    376 

243          Radical  functions  are  a  generalisation  of  rational  functions         .  377 

244,    245     Characteristics  of  radical  functions         .         .         .         .         .         .  378 — 381 

246 — 249     Bitangents  of  a  plane  quartic  curve 381 — 390 

250,    251     Solution  of  the  inversion  problem  by  radical  functions        .         .  390 — 392 


CHAPTER   XIV. 

FACTORIAL  FUNCTIONS. 

252  Statement  of  results  obtained.     Notations 393,    394 

253  Necessary  dissection  of  the  Riemann  surface        ....  395 

254  Definition   of    a    factorial   function    (including   radical  function). 

Primary  and  associated  systems  of  factorial  functions  .         .       396,    397 


CONTENTS. 


XV 


§§  PAGES 

255  Factorial  integrals  of  the  primary  and  associated  systems  .         .  397,    398 

256  Factorial  integrals  which  are  everywhere  finite,  save  at  the  fixed 

infinities.     Introduction  of  the  numbers  or,  <r  + 1     .         .         .  399 

257  When  <r  +  l>0,  there  are  o-  +  l  everywhere  finite  factorial  functions 

of  the  associated  system    ........  400 

258  Alternative  investigation  of  everywhere  finite  factorial  functions 

of  the  associated  system.     Theory  divisible  according  to  the 

values  of  o-  +  l  and  o-'  +  l 401,    402 

259  Expression  of  these  functions  by  everywhere  finite  integrals        .  403 

260  General  consideration  of  the  periods  of  the  factorial  integrals     .  404 
261,    262     Riemanri-Roch  theorem  for  factorial  functions.     When  or' +  1=0, 

least  number  of  arbitrary  poles  for  fimction  of  the  primary 

system  is  or'  +  l 405,    406 

263         Construction   of  factorial   function   of  the  primary  system   with 

or'  +  l  arbitrary  poles       .         .         .         .         .         .         .         .  406,    407 

264,    265     Construction   of  a  factorial   integral   having  only   poles.      Least 
number  of  such  poles,  for  an  integral  of  the  primary  system, 

is  o-  +  2 407,    410 

266  This  factorial  integral  can  be  simplified,  in  analogy  with  Riemann's 

elementary  integral  of  the  second  kind 411 

267  Expression  of  the  factorial  function  with  or'  +  l  poles  in  terms  of 

the  factorial  integral  with  o-  +  2  poles.     The  factorial  function 

in  analogy  with  the  function  i\r  (x,  a;  z,  clt  ...,  cp).         .         .  411 — 413 

268  The  theory  tested  by  examination  of  a  very  particular  case        .  413 — 419 

269  The  radical  functions  as  a  particular  case  of  factorial  functions  419,    420 

270  Factorial   functions  whose  factors  are  any  constants,  having  no 

essential  singularities        ........  421 

271,    272     Investigation  of  a  general  formula  connecting  factorial  functions 

and  theta  functions 422 — 426 

273  Introduction  of  the  Schottky-Klein  prime  form,  in  a  certain  shape  427 — 430 

274  Expression  of  a  theta  function  in  terms  of  radical  functions,  as  ' 

a  particular  case  of  §  272        .         .         .         .       '-.        .    "  .  430 

275,    276     The  formula  of  §  272  for  the  case  of  rational  functions      .         .  431—433 

277  The  formula  of  §  272  applied  to  define  algebraically  the  hyper- 

elliptic  theta  function,  and  its  theta  characteristic        .         .  433 — 437 

278  Expression  of  any  factorial   function  by  simple  theta  functions  ; 

examples 437,    433 

279  Connection  of  theory  of  factorial  functions  with  theory  of  auto- 

morphic  forms  .  439 442 


CHAPTER    XV. 

RELATIONS  CONNECTING  PRODUCTS  OF  THETA  FUNCTIONS — INTRODUCTORY. 


280 
281 


443 


Plan  of  this  and  the  two  following  chapters          .... 

A  single-valued  integral  analytical  function  of  p  variables,  which 
is  periodic  in  each  variable  alone,  can  be  represented  by  a 
series  of  exponentials  ....  443 445 


XVI  CONTENTS. 

§§  PAGES 

282,    283     Proof  that  the  22p  theta  functions  with   half-integer  character 
istics  are  linearly  independent         ......  446 — 447 

284,    285     Definition  of  general  theta  function  of  order  r ;  its  linear  expres 
sion   by  r1'   theta  functions.     Any  p-f2   theta  functions   of 
same  order,  periods,  and  characteristic  connected  by  a  homo 
geneous  polynomial  relation     .......  447 — 455 

286         Addition   theorem   for  hyperelliptic   theta   functions,  or   for  the 

general  case  when  p<4   ........  456 — 461 

286,    288     Number  of  linearly  independent  theta  functions  of  order  r  which 

are  all  of  the  same  parity        .......  461 — 464 

289          Examples.     The  Gopel  biquadratic  relation 465 — 470 


CHAPTER    XVI. 

A   DIRECT   METHOD   OF  OBTAINING   THE   EQUATIONS  CONNECTING  THETA 

PRODUCTS. 

290  Contents  of  this  chapter 471 

291  An  addition  theorem  obtained  by  multiplying  two  theta  functions .  471 — 474 

292  An  addition  theorem  obtained  by  multiplying  four  theta  functions  474 — 477 

293  The  general   formula   obtained    by   multiplying    any   number   of 

theta  functions          .         .  .         .         .         .  477 485 


CHAPTER    XVII. 
THETA  RELATIONS  ASSOCIATED  WITH  CERTAIN  GROUPS  OF  CHARACTERISTICS. 

294  Abbreviations.     Definition  of  syzygetic  and  azygetic.     References 

to  literature  (see  also  p.  296) 486,    487 

295  A  preliminary  lemma .  488 

296  Determination  of  a  Gopel  group  of  characteristics        .         .         .  489,    490 

297  Determination  of  a  Gopel  system  of  characteristics      .         .         .  490,    491 
298,    299     Determination  and  number  of  Gopel  systems  of  the  same  parity  492 — 494 
300 — 303     Determination  of  a  fundamental  set  of  Gopel  systems          .         .  494 — 501 
304,    305     Statement  of  results  obtained,  with  the  simpler  applications       .  502 — 504 
306 — 308     Number  of  linearly  independent  theta  functions   of  the  second 

order  of  a  particular  kind.  Explicit  mention  of  an  import 
ant  identity 505 — 510 

309 — 311  The  most  important  formulae  of  the  chapter.  A  general  addi 
tion  theorem.  The  g>  function  expressed  by  quotients  of 

theta  functions 510 — 516 

312 — 317  Other  applications  of  the  principles  of  the  chapter.  The  expres 
sion  of  a  function  3  (nv)  as  an  integral  polynomial  of  order 

«2  in  2"  functions  $(v) 517—527 


CONTENTS. 


XV11 


CHAPTER    XVIII. 
TRANSFORMATION  OF  PERIODS,  ESPECIALLY  LINEAR  TRANSFORMATION. 

§§  PAGES 

318         Bearings  of  the  theory  of  transformation 528,    529 

319 — 323     The  general  theory  of  the  modification  of  the  period  loops  on  a 

Riemann  surface 529 — 534 

324  Analytical  theory  of  transformation  of  periods  and  characteristic 

of  a  theta  function 534 — 538 

325  Convergence  of  the  transformed  function       .         .         .         .         .  538 

326  Specialisation  of  the  formulae,  for  linear  transformation      .         .  539,    540 

327  Transformation  of  theta  characteristics  ;  of  even  characteristics  ; 

of  syzygetic  characteristics        .         .         .         .         .         .         .541,    542 

328  Period  characteristics  and  theta  characteristics     .         .         .  •       .  543 

329  Determination  of  a  linear  transformation  to  transform  any  even 

characteristic  into  the  zero  characteristic        ....  544,    545 

330,    331     Linear  transformation  of  two  azygetic  systems  of  theta  charac 
teristics  into  one  another         .        .        .        .        .        .         .    .  546 — 550 

332         Composition  of  two  transformations  of  different  orders ;  supple 
mentary  transformations 551,    552 

333,  334  Formation  of  p  +  2  elementary  linear  transformations  by  the 
composition  of  which  every  linear  transformation  can  be 
formed ;  determination  of  the  constant  factors  for  each  of 

these ,.:;./.,.       Lrj         .  553—557 

335  The  constant  factor  for  any  linear  transformation        .         .         .  558,    559 

336  Any  linear  transformation   may  be  associated  with   a  change  of 

the  period  loops  of  a  Riemann  surface 560,    561 

337,    338     Linear  transformation  of  the  places  mlt  ...,  mp  .•*    •     .         .         .  562 

339  Linear  transformation  of  the  characteristics  of  a  radical  function  563,    564 

340  Determination  of  the  places  Wj,  ...,  mp  upon  a  Riemann  surface 

whose  mode  of  dissection  is  assigned      .       ..».'..•.       ..  565 — 567 

341  Linear  transformation  of  quotients  of  hyperelliptic  theta  functions  568 

342  A  convenient  form  of  the  period  loops  in  a  special  hyperelliptic 

case.     Weierstrass's  number  notation  for  half-integer  charac 
teristics       .            .            .            ..:;.:,;;    .;.        •    .     •..:.            .            .            .  569,     570 


CHAPTER    XIX. 


ON    SYSTEMS   OF   PERIODS   AND    ON    GENERAL    JACOBIAN    FUNCTIONS. 


343 

344—350 


571 


571—579 


Scope  of  this  chapter       ......... 

Columns  of  periods.     Exclusion  of  infinitesimal  periods.     Expres 
sion  of  all  period  columns  by  a  finite  number  of  columns, 

with  integer  coefficients 

351 — 356     Definition   of  general   Jacobian    function,    and   comparison   with 

theta  function 579 588 

357—362  Expression  of  Jacobian  function  by  means  of  theta  functions. 
Any  p  +  2  Jacobian  functions  of  same  periods  and  parameter 
connected  by  a  homogeneous  polynomial  relation  .  .  588 — 598 


XV111  CONTENTS. 


CHAPTER    XX. 
TRANSFORMATION  OF  THETA  FUNCTIONS. 

§§  PAGES 

363          Sketch  of  the  results  obtained.     References  to  the  literature       .  599,    600 

364,    365     Elementary  theory  of  transformation  of  second  order  .         .         .  600 — 606 
366,    367     Investigation  of  a  general  formula  preliminary  to  transformation 

of  odd  order 607—610 

368,    369     The  general  theorem  for  transformation  of  odd  order  .         .         .  611 — 616 

370  The  general  treatment  of  transformation  of  the  second  order      .  617—619 

371  The  two  steps  in  the  determination  of  the  constant  coefficients  619 

372  The  first  step  in  the  determination  of  the  constant  coefficients  619 — 622 

373  Remarks  and  examples  in  regard  to  the  second  step  .         .         .  622 — 624 

374  Transformation  of  periods  when  the  coefficients  are  not  integral  624 — 628 

375  Reference  to  the  algebraical  applications  of  the  theory         .         .  628 


CHAPTER   XXI. 

COMPLEX  MULTIPLICATION  OF  THETA  FUNCTIONS.     CORRESPONDENCE 
OF  POINTS  ON  A  RlEMANN  SURFACE. 

376         Scope  of  the  chapter .        .        .  629 

377,    378     Necessary    conditions   for    a    complex    multiplication,    or    special 

transformation,  of  theta  functions   ......  629 — 632 

379 — 382     Proof,  in  one  case,  that  these  conditions  are  sufficient         .         .  632 — 636 

383  Example  of  the  elliptic  case 636—639 

384  Meaning  of  an  (r,  s)  correspondence  on  a  Riemann  surface         .  639,    640 

385  Equations  necessary  for  the  existence  of  such  a  correspondence  640 — 642 

386  Algebraic  determination  of  a  correspondence  existing  on  a  per 

fectly  general  Riemann  surface        .         ...         .         . .       .  642 — 645 

387  The  coincidences.     Examples  of  the  inflections  and  bitangents  of 

a  plane  curve   645 — 648 

388  Conditions  for  a  (1,  s)  correspondence  on  a  special  Riemann  surface  648,    649 

389  When  p>l  a  (1,  1)  correspondence  is  necessarily  periodic  .         .  649,    650 

390  And  involves  a  special  form  of  fundamental  equation         .         .  651 
391—393     When  p>l  there  cannot  be  an  infinite  number  of  (1,  1)  corre 
spondences         652 — 654 

394          Example  of  the  case  p  =  l 654—656 


CHAPTER   XXII. 
DEGENERATE  ABELIAN  INTEGRALS. 

395  Example  of  the  property  to  be  considered    .        .  .        .  657 

396  Weierstrass's  theorem.     The  property  involves  a  transformation 

leading  to  a  theta  function  which  breaks  into  factors  .         .       657,    658 


CONTENTS. 


XIX 


397  Weierstrass's  and   Picard's    theorem.     The    property   involves    a 

linear  transformation  leading  to  T^'2  =  l/r. 

398  Existence  of  one  degenerate  integral  involves  another  (p  =  2) 
399,    400    Connection  with  theory  of  special  transformation,  when  p  —  Z     . 
401 — 403     Determination    of    necessary    form    of    fundamental    equation. 

Eeferences 


PAGES 

658,    659 

659 
660,    661 

661—663 


404 


APPENDIX   I. 

ON   ALGEBRAIC   CURVES   IN    SPACE. 

Formal  proof  that  an  algebraic  curve  in  space  is  an  interpreta 
tion  of  the  relations  connecting  three  rational  functions  on 
a  Riemann  surface  (cf.  §  162) 664, 


665 


APPENDIX  II. 

ON   MATRICES. 

405 — 410     Introductory  explanations        .         .         .         ;        .,        .        ,  ...  666 669 

411 — 415     Decomposition  of  an  Abelian  matrix  into  simpler  ones        .  '  .  669 674 

416          A  particular  result ...            674 

417,    418     Lemmas ,        .  .           675 

419,   420     Proof  of  results  assumed  in  §§  396,  397       ....  .'.  675,    676 


INDEX  OF  AUTHORS  QUOTED   . 
TABLE  OF  SOME  FUNCTIONAL  SYMBOLS 
SUBJECT  INDEX 


677,    678 

679 
680—684 


ADDENDA.     CORRIGENDA. 

PAGE  LINE 

6,  2,  for  bb^da,  read  (tb*~lda. 

8,  22,  for  deficiency  1,  read  deficiency  0. 

11,  12,  for  2n-2+p,  read  2n-2  +  2p. 

16,  §  16,     4,  for  called,  read  applied  to. 

dx  .  dx 

18,  25,    for  —  ,  read  —  . 

x  y 

37,  31,    for  in,  read  is. 

38,  3,    for  surfaces,  read  surface. 
43,             20,    for  w,  read  w. 

56,  22,  for  (x-af~\  read  (x  -a)P-A+1. 

61,  24,  add  or  g{  (x,  y). 

66,  22,  for  r'-l,  read  Tj'-l. 

70,  14,  for  rr+l,  read  rr+l. 

73,  28,  for  x'^'^''2  sl5  2,  read  x~2r'~2  slt  j. 

81.  The  argument  of  §  52  supposes  p>l. 

104,  §  72.  See  also  Hensel,  Crelle,  cxv.  (1895). 

114,  3  from  the  bottom,  add  here. 

137.  To  the  references,  add,  Macaulay,  Proc.  Lon.  Math.  Soc.,  xxvi.  p.  495. 

157.  See  also  Kraus,  Math.  Annal.  xvi.  (1879). 

166.  See  also  Zeuthen,  Ann.  d.  Mat.  2a  Ser.,  t.  in.   (1869). 

189,  21,  for  xii,  read  xi. 

196,  23,  for  \h,  read  \h. 
24,  for  \h,  read  \h. 

197,  24,  for  A,  read  B. 

198,  5,    for  ^(w')"1^,  read  y(u')~lu. 

18,    for  fourth  minus  sign,  read  sign  of  equality. 

206,  4,    supply  dz,  after  third  integral  sign:   the  summation  is  from  k  =  2,  fc'=0. 

5,     supply  dz,  after  first  integral  sign. 
8,    for  $(X)l<t>(X),  read  0'(*)/0(X). 
247,  11.     Positive  means  >0.     The  discriminant  must  not  vanish. 

6      from  bottom.     Cf.  p.  531,  notef. 
282,  11,    for  ft,  read  O. 

284,  18,     the  equation  is  httP  =  iriP  +  bP'. 

316,  3      from  the  bottom,  for  u,  read  UQ. 

320,  heading,  destroy  full  stop. 

327,  23,    for  Pi(xp),  read  /J.J(XP). 

340.  Further    references    are   given    in    the    report    of    Brill    and    Noether    (see 

Preface),  p.  473. 
342.  For  various  notations  for  characteristics  see  the  references  in  the  report  of 

Brill  and  Noether,  p.  519. 
379,  16,    for  T(II,  ritp,  read  v^-",  vpx'a. 

420,  18,     read  ...characteristic,  other  than  the  zero  characteristic,  as  the  sum  of  two 

different  odd  half-integer  characteristics  in 

441,  15,    for  one,  read  in  turn  every  combination. 

533,  13.     The  relation  had  been  given  by  Frobenius. 

557,  15,    for  .w2,  read  w-?. 

575,  20,    for  from,  read  for. 

587,  8  and  11 ;    the  quantity  is  AeA. 

In  this  volume  no  account  is  given  of  the  differential  equations  satisfied  by  the  theta 
functions,  or  of  their  expansion  in  integral  powers  of  the  arguments.  The  following  refer 
ences  may  be  useful :  Wiltheiss,  Crelle,  xcix.,  Math.  Annal.  xxix.,  xxxi.,  xxxin.,  Gotting. 
Nachr.,  1889,  p.  381;  Pascal,  Gotting.  Xachr.,  1889,  pp.  416,  547,  Ann.  di  Mat.,  Ser.  2%  t. 
xvii.;  Burkhardt  (and  Klein),  Math.  Annal.  xxxn.  The  case  p  —  2  is  considered  in  Krause, 
Transf.  Hyperellip.  Functionen.- 

The  following  books  of  recent  appearance,  not  referred  to  in  the  text,  may  be  named  here. 
(1)  The  completion  of  Picard,  Traite  d'Analyse,  (2)  Jordan,  Cours  d'Analyse,  t.  n.  (1894), 
(3)  Appell  and  Goursat,  Theorie  des  Fonctions  algebriques  et  de  leurs  integrates  (1895),  (4) 
Stahl,  Theorie  der  AbeVschen  Functionen  (1896). 


CHAPTER  I. 


ADDITIONAL  CORRECTIONS  FOR  BAKER'S  ABELIAN  FUNCTIONS. 

PAGE  LINE 

138,  14,  from  the  bottom,  for  greater,  read  less. 

219,  12,  13,  from  the  bottom,  for  r,  read  R. 

315,  6,  from  the  bottom,  for  f,  read  f. 

316,  5,  from  the  bottom,  for  u,  read  u0. 

317,  4,  from  the  bottom,  for  a,  vanishes,  &j ,  read,  respectively,  bl ,  is  infinite,  a. 
333,  3,  for  the  first  + ,  read  -  . 

333,  3,  7,  8,     from  the  bottom,  for  A,  read  V. 

334,  6,  7,     from  the  bottom,  for  pt,  pj,  read  p$,  pf'2. 

335,  12,     from  the  bottom,  for  A,  read  \ . 

340,  6,     from   the    bottom,  for   Gopel,   read    Kummer.      Supply   also    the    reference, 

Weber,  Crelle  LXXXIV.  (1878),  p.  341. 

359,  1,     after  periods,  add  and  let  ^  (u)  =  @  (u)  +  @(u  +  u'). 

5,    for  $>,  read  ^ ;  for  iir,  read  Ziir. 

9,    for  P  +  iQ,  read  (P  +  iQ)  [(£>'  (u)  +  $'  (v)],  where  u,  v  are  the  arguments  occurring 
in  the  denominator ;   and  similarly  for  P-iQ ;   and  add  to   the  function 

the  term  4P    f  (u)  -  — ,  f  (w')l,  where  f(w)  is  Weierstrass's  function. 

367,  5,     from  the  bottom,  for  m,  read  p. 

444,  16,    for  x,  read  u. 

445,  14,    for  n,  read  p. 

457,  14,     from  the  bottom,  supply  the  reference,  §  181. 

615,  5,    for  xviii.,  read  xvn. 

665,  6,     from   the  bottom,  add,  which   may  be   taken   to   be   linear  polynomials  in 

x  only. 

sheet.  Or  the  sheets  may  wind  into  one  another :  in  which  case  we  shall 
regard  this  winding  point  (or  branch  point)  as  constituting  one  place :  this 
place  belongs  then  indifferently  to  either  sheet ;  the  sheets  here  merge  into 
one  another.  In  the  first  case,  if  a  be  the  value  of  x  for  which  the  sheets 
just  touch,  supposed  for  convenience  of  statement  to  be  finite,  and  x  a  value 

*  For  references  see  Chap.  II.  §  12,  note. 

t  Such  a  point  is  called  by  Riemann  "ein  sich  aufhebender  Verzweigungspunkt  " :    Gesam- 
melte  Werke  (1876),  p.  105. 

B.  1 


ADDENDA.     CORRIGENDA. 


PAGE  LINE 

^ 


6,  2,  for  db^da,  read  db^~da. 

8,  22,  for  deficiency  1,  read  deficiency  0. 

11,  12,  for  2n-2+p,  read  2n-2  +  2p. 

16,  §  16,     4,  for  called,  read  applied  to. 

dx  ,  da; 

18,  25,    for  —  ,  read  —  . 

x  y 

37,  31,    for  in,  read  is. 

38,  3,    for  surfaces,  read  surface. 
43,             20,    for  w,  read  w. 

56,  22,    for  (x-af~\  read  (x-a)<>-*+1. 

fil  24.     add  or  n,  (x.   u\. 


587,  8  and  11 ;   the  quantity  is  AeA. 


In  this  volume  no  account  is  given  of  the  differential  equations  satisfied  by  the  theta 
functions,  or  of  their  expansion  in  integral  powers  of  the  arguments.  The  following  refer 
ences  may  be  useful :  Wiltheiss,  Crelle,  xcix.,  Hath.  Annal.  xxix.,  xxxi.,  xxxm.,  Gotting. 
Nachr.,  1889,  p.  381;  Pascal,  Gotting.  Nachr.,  1889,  pp.  416,  547,  Ann.  di  Mat.,  Ser.  2%  t. 
xvii.;  Burkhardt  (and  Klein),  Math.  Annal.  xxxn.  The  case  p  =  2  is  considered  in  Krause, 
Transf.  Hyperellip.  Functionen.- 

The  following  books  of  recent  appearance,  not  referred  to  in  the  text,  may  be  named  here. 
(1)  The  completion  of  Picard,  Traite  d'Anatyse,  (2)  Jordan,  Cours  d'Analyse,  t.  11.  (1894), 
(3)  Appell  and  Goursat,  Theorie  des  Fonctions  algebriques  et  de  leurs  integrates  (1895),  (4) 
Stahl,  Theorie  der  AbeVschen  Functionen  (1896). 


CHAPTER  I. 

THE  SUBJECT  OF  INVESTIGATION. 

1.  THIS  book  is  concerned  with  a  particular  development  of  the  theory 
of  the  algebraic  irrationality  arising  when  a  quantity  y  is  defined  in  terms 
of  a  quantity  x  by  means  of  an  equation  of  the  form 

a0yn  +  atf1'1  +...+  an^y  +  an  =  0, 

wherein  a0,  al}  ...,an  are  rational  integral  polynomials  in  x.  The  equation  is 
supposed  to  be  irreducible ;  that  is,  the  left-hand  side  cannot  be  written  as 
the  product  of  other  expressions  of  the  same  rational  form. 

2.  Of  the  various  means  by  which  this  dependence  may  be  represented, 
that  invented  by  Riemann,  the  so-called  Riemann  surface,  is  throughout 
regarded  as  fundamental.     Of  this  it  is  not  necessary  to  give  an  account 
here*.     But  the  sense  in  which  we  speak  of  a  place  of  a  Riemann  surface 
must  be  explained.     To  a  value  of  the  independent  variable  x  there  will  in 
general  correspond  n  distinct  values  of  the  dependent  variable  y — represented 
by  as  many  places,  lying  in  distinct  sheets  of  the  surface.     For  some  values 
of  x  two  of  these  n  values  of  y  may  happen  to  be  equal :  in  that  case  the 
corresponding  sheets  of  the  surface  may  behave  in  one  of  two  ways.     Either 
they  may  just  touch  at  one  point  without  having  any  further  connexion  in 
the  immediate  neighbourhood  of  the  point t :  in  which  case  we  shall  regard 
the  point  where  the  sheets  touch  as  constituting  two  places,  one  in  each 
sheet.     Or  the  sheets  may  wind  into  one  another :   in  which  case  we  shall 
regard  this  winding  point  (or  branch  point)  as  constituting  one  place :  this 
place  belongs  then  indifferently  to  either  sheet ;  the  sheets  here  merge  into 
one  another.     In  the  first  case,  if  a  be  the  value  of  x  for  which  the  sheets 
just  touch,  supposed  for  convenience  of  statement  to  be  finite,  and  x  a  value 

*  For  references  see  Chap.  II.  §  12,  note. 

t  Such  a  point  is  called  by  Riemann  "ein  sich  aufhebender  Verzweigungspunkt  " :    Gesam- 
melte  Werke  (1876),  p.  105. 

B.  1 


2  THE   PLACES   OF   A  RIEMANN   SURFACE.  [2 

very  near  to  a,  and  if  b  be  the  value  of  y  at  each  of  the  two  places,  also 
supposed  finite,  and  ylt  yz  be  values  of  y  very  near  to  b,  represented  by 
points  in  the  two  sheets  very  near  to  the  point  of  contact  of  the  two 
sheets,  each  of  3/1  —  6,  yz  —  b  can  be  expressed  as  a  power-series  in  x  —  a 
with  integral  exponents.  In  the  second  case  with  a  similar  notation  each 
of  2/1  —  6,  y2  —  6  can  be  expressed  as  a  power-series  in  (x  —  a)*  with  integral 
exponents.  In  the  first  case  a  small  closed  curve  can  be  drawn  on  either 
of  the  two  sheets  considered,  to  enclose  the  point  at  which  the  sheets  touch : 

and  the  value  of  the  integral  •= — .  Id  log  (x  -  a)  taken  round  this  closed  curve 

will  be  1 ;  hence,  adopting  a  definition  given  by  Riemann*,  we  shall  say  that 
x  —  a  is  an  infinitesimal  of  the  first  order  at  each  of  the  places.  In  the 
second  case  the  attempt  to  enclose  the  place  by  a  curve  leads  to  a  curve 
lying  partly  in  one  sheet  and  partly  in  the  other;  in  fact,  in  order  that 
the  curve  may  be  closed  it  must  pass  twice  round  the  branch  place.  In  this 

case  the  integral  ^ — .  Id  log  [(x  —  a)*]  taken  round  the  closed  curve  will  be  1 : 

and  we  speak  of  (x  —  a}*-  as  an  infinitesimal  of  the  first  order  at  the  place. 
In  either  case,  if  t  denote  the  infinitesimal,  x  and  y  are  uniform  functions 
of  t  in  the  immediate  neighbourhood  of  the  place ;  conversely,  to  each  point 
on  the  surface  in  the  immediate  neighbourhood  of  the  place  there  corre 
sponds  uniformly  a  certain  value  of  if.  The  quantity  t  effects  therefore  a 
conformal  representation  of  this  neighbourhood  upon  a  small  simple  area  in 
the  plane  of  t,  surrounding  t  —  0. 

3.  This  description  of  a  simple  case  will  make  the  general  case  clear. 
In  general  for  any  finite  value  of  x,  x  =  a,  there  may  be  several,  say  k,  branch 
points J;  the  number  of  sheets  that  wind  at  these  branch  points  may  be 
denoted  by  w1+l,w.2+l,  . ..,  wk+  1  respectively,  where 

(w1  +  1)  +  (w,  +  l)  +  ...+(wk+l)  =  n, 

so  that  the  case  of  no  branch  point  is  characterised  by  a  zero  value  of  the 
corresponding  w.  For  instance  in  the  first  case  above,  notwithstanding  that 
two  of  the  n  values  of  y  are  the  same,  each  of  w1}  w.2,  ...,Wk  is  zero  and  k  is 
equal  to  n  :  and  in  the  second  case  above,  the  values  are  k  =  n  —  1,  wr  =  1,  w.2  =  0, 
w3  =  0,  . . . ,  wk  =  0.  In  the  general  case  each  of  these  k  branch  points  is  called  a 

place,  and  at  these  respective  places  the  quantities  (x  -  a)w>+l,  ...,  (x—  a)wt+l 

*  Gesammelte  Werke  (1876),  p.  96. 

+  The  limitation  to  the  immediate  neighbourhood  involves  that  t  is  not  necessarily  a  rational 
function  of  x,  y. 

It  may  be  remarked  that  a  rational  function  of  x  and  y  can  be  found  whose  behaviour  in 
the  neighbourhood  of  the  place  is  the  same  as  that  of  t.  See  for  example  Hamburger, 
Zeitschrift  f.  Math,  und  Phys.  Bd.  16,  1871 ;  Stolz,  Math.  Ann.  8,  1874 ;  Harkness  and  Morley, 
Theory  of  Functions,  p.  141. 

t  Cf.  Forsyth,  Theory  of  Functions,  p.  171.     Prym,  Crelle,  Bd.  70. 


4]  TRANSFORMATION  OF  THE  EQUATION.  3 

are  infinitesimals  of  the  first  order.     For  the  infinite  value  of  x  we  shall 
similarly  have  n  or  a  less  number  of  places  and  as  many  infinitesimals,  say 


-_ 

+1,  ...,  (-r'+1,  where  (Wl  +  l)+  ...  +(w,.  +  I)  =  n.     And  as  in  the  par- 

xj  \x/ 

ticular  cases  discussed  above,  the  infinitesimal  t  thus  defined  for  every  place 
of  the  surface  has  the  two  characteristics  that  for  the  immediate  neighbour 
hood  of  the  place  x  and  y  are  uniquely  expressible  thereby  (in  series  of 
integral  powers),  and  conversely  t  is  a  uniform  function  of  position  on  the 
surface  in  this  neighbourhood.  Both  these  are  expressed  by  saying  that 
t  effects  a  reversible  conformal  representation  of  this  neighbourhood  upon  a 
simple  area  enclosing  t  =  0.  It  is  obvious  of  course  that  quantities  other 
than  t  have  the  same  property. 

A  place  of  the  Riemann  surface  will  generally  be  denoted  by  a  single 
letter.  And  in  fact  a  place  (x,  y}  will  generally  be  called  the  place  x. 
When  we  have  occasion  to  speak  of  the  (n  or  less)  places  where  the  inde 
pendent  variable  x  has  the  same  value,  a  different  notation  will  be  used. 

4.  We  have  said  that  the  subject  of  enquiry  in  this  book  is  a  certain 
algebraic  irrationality.  We  may  expect  therefore  that  the  theory  is  practi 
cally  unaltered  by  a  rational  transformation  of  the  variables  x,  y  which  is  of 
a  reversible  character.  Without  entering  here  into  the  theory  of  such  trans 
formations,  which  comes  more  properly  later,  in  connexion  with  the  theory 
of  correspondence,  it  is  necessary  to  give  sufficient  explanations  to  make  it 
clear  that  the  functions  to  be  considered  belong  to  a  whole  class  of  Riemann 
surfaces  and  are  not  the  exclusive  outcome  of  that  one  which  we  adopt  initially. 

Let  £  be  any  one  of  those  uniform  functions  of  position  on  the  funda 
mental  (undissected)  Riemann  surface  whose  infinities  are  all  of  finite  order. 
Such  functions  can  be  expressed  rationally  by  x  and  y*.  For  that  reason  we 
shall  speak  of  them  shortly  as  the  rational  functions  of  the  surface.  The 
order  of  infinity  of  such  a  function  at  any  place  of  the  surface  where  the 
function  becomes  infinite  is  the  same  as  that  of  a  certain  integral  power  of 

the  inverse  -  of  the  infinitesimal  at  that  place.     The  sum  of  these  orders  of 

6 

infinity  for  all  the  infinities  of  the  function  is  called  the  order  of  the  function. 
The  number  of  places  at  which  the  function  f  assumes  any  other  value  a  is 
the  same  as  this  order  :  it  being  understood  that  a  place  at  which  £  —  a  is 
zero  in  a  finite  ratio  to  the  rth  order  of  t  is  counted  as  r  places  at  which  £  is 
equal  to  off.  Let  v  be  the  order  of  £.  Let  T?  be  another  rational  function  of 

*  Forsyth,  Theory  of  Functions,  p.  370. 

t  For  the  integral   —  /dlog(£-a),  taken  round  an  infinity  of  log(£-a),  is  equal  to  the 

order  of  zero  of  £  -  a  at  the  place,  or  to  the  negative  of  the  order  of  infinity  of  £,  as  the  case  may 
be.  And  the  sum  of  the  integrals  for  all  such  places  is  equal  to  the  value  round  the  boundary  of 
the  surface—  which  is  zero.  Cf.  Forsyth,  Theonj  of  Functions,  p.  372. 

1—2 


4  CONDITION   OF   REVERSIBILITY.  [4 

order  p.  Take  a  plane  whose  real  points  represent  all  the  possible  values  of 
|f  in  the  ordinary  way.  To  any  value  of  |f,  say  |f  =  a,  will  correspond  v 
positions  Xlt  ...,  Xvon  the  original  Riemann  surface,  those  namely  where  £ 
is  equal  to  a  :  it  is  quite  possible  that  they  lie  at  less  than  v  places  of  the 
surface.  The  values  of  77  at  X1}  ...,  Xv  may  or  may  not  be  different.  Let 
H  denote  any  definite  rational  symmetrical  function  of  these  v  values  of  77. 
Then  to  each  position  of  a  in  the  |f  plane  will  correspond  a  perfectly  unique 
value  of  H,  namely,  H  is  a  one-valued  function  of  £.  Moreover,  since  77  and 
|f  are  rational  functions  on  the  original  surface,  the  character  of  H  for  values 
of  |f  in  the  immediate  neighbourhood  of  a  value  a,  for  which  H  is  infinite,  is 
clearly  the  same  as  that  of  a  finite  power  of  ff  —  a.  Hence  H  is  a  rational 
function  of  |f.  Hence,  if  Hr  denote  the  sum  of  the  products  of  the  values  of 
i]  at  Xlt  ...,  Xv,  r  together,  77  satisfies  an  equation 

r)"-r)"^H1  +  r)^H2-...+(-YHv  =  0> 
whose  coefficients  are  rational  functions  of  |f. 

It  is  conceivable  that  the  left  side  of  this  equation  can  be  written  as  the 
product  of  several  factors  each  rational  in  |f  and  77.  If  possible  let  this  be 
done.  Construct  over  the  |f  plane  the  Riemann  surfaces  corresponding  to 
these  irreducible  factors,  77  being  the  dependent  variable  and  the  various 
surfaces  lying  above  one  another  in  some  order.  It  is  a  known  fact,  already 
used  in  defining  the  order  of  a  rational  function  on  a  Riemann  surface,  that 
the  values  of  77  represented  by  any  one  of  these  superimposed  surfaces  in 
clude  all  possible  values  —  each  value  in  fact  occurring  the  same  number  of 
times  on  each  surface.  To  any  place  of  the  original  surface,  where  |f,  77  have 
definite  values,  and  to  the  neighbourhood  of  this  place,  will  correspond  there 
fore  a  definite  place  (|f,  77)  (and  its  neighbourhood)  on  each  of  these  super 
imposed  surfaces.  Let  77!,  ...,tjr  be  the  values  of  77  belonging,  on  one  of 
these  surfaces,  to  a  value  of  £  :  and  T?/,  ...,  r}s'  the  values  belonging  to  the 
same  value  of  |f  on  another  of  these  surfaces.  Since  for  each  of  these  surfaces 
there  are  only  a  finite  number  of  values  of  £  at  which  the  values  of  77  are 
not  all  different,  we  may  suppose  that  all  these  r  values  on  the  one 
surface  are  different  from  one  another,  and  likewise  the  s  values  on  the  other 
surface.  Since  each  of  the  pairs  of  values  (|f,  77^,  .  .  .  ,  (|f,  r)r)  must  arise  on 
both  these  surfaces,  it  follows  that  the  values  77!,  ...,tjr  are  included  among 
77/,  ...,  77/.  Similarly  the  values  T7/,  ...,  i?/  are  included  among  77^  ...,77,.. 
Hence  these  two  sets  are  the  same  and  r  =  s.  Since  this  is  true  for  an 
infinite  number  of  values  of  |f,  it  follows  that  these  two  surfaces  are  merely 
repetitions  of  one  another.  The  same  is  true  for  every  such  two  surfaces. 
Hence  r  is  a  divisor  of  v  and  the  equation 


when  reducible,  is  the  v/rih  power  of  a  rational  equation  of  order  r  in  77.     It 
will  be  sufficient  to  confine  our  attention  to  one  of  the  factors  and  the  (£,  77) 


5]  CORRESPONDENCE  OF  TWO  SURFACES.  5 

surface  represented  thereby.  Let  now  Xlt  .  .  .  ,  Xv  be  the  places  on  the  original 
surface  where  £  has  a  certain  value.  Then  the  values  of  77  at  Xlt  .  .  ,  Xv  will 
consist  of  v/r  repetitions  of  r  values,  these  r  values  being  different  from  one 
another  except  for  a  finite  number  of  values  of  £  Thus  to  any  place  (f,  77)  on 
one  of  the  v/r  derived  surfaces  will  correspond  v/r  places  on  the  original 
surface,  those  namely  where  the  pair  (£,  77)  take  the  supposed  values.  Denote 
these  by  PlfPa,  —  Let  Y  be  any  rational  symmetrical  function  of  the  v/r 
pairs  of  values  (a}1}  y^),  (#2,  2/2)»  •••>  which  the  fundamental  variables  a,  y  of  the 
original  surface  assume  at  P1;  P2)  —  Then  to  any  pair  of  values  (£,  77)  will 
correspond  only  one  value  of  Y  —  namely,  Y  is  a  one-valued  function  on  the 
(£,  77)  surface.  It  has  clearly  also  only  finite  orders  of  infinity.  Hence  Y  is 
a  rational  function  of  £,  77.  In  particular  #u  #2,  ...  are  the  roots  of  an 
equation  whose  coefficients  are  rational  in  £,  77  —  as  also  are  yi}  yz,  ____ 

There  exists  therefore  a  correspondence  between  the  (£,  77)  and  (x,  y) 

surfaces  —  of  the  kind  which  we  call  a  (1,  -  j  correspondence:  to  every  place 
of  the  (x,  y)  surface  corresponds  one  place  of  the  (£,  77)  surface;  to  every 
place  of  this  surface  correspond  -  places  of  the  (x,  y)  surface. 

The  case  which  most  commonly  arises  is  that  in  which  the  rational 
irreducible  equation  satisfied  by  77  is  of  the  vih  degree  in  77:  then  only  one 
place  of  the  original  surface  is  associated  with  any  place  of  the  new  surface. 
In  that  case,  as  will  appear,  the  new  surface  is  as  general  as  the  original 
surface.  Many  advantages  may  be  expected  to  accrue  from  the  utilization  of 
that  fact.  We  may  compare  the  case  of  the  reduction  of  the  general  equation 
of  a  conic  to  an  equation  referred  to  the  principal  axes  of  the  conic. 

5.     The  following  method*  is  theoretically  effective  for  the  expression  of  x,  y  in  terms 
of  &  r,. 

Let  the  rational  expression  of  £,  rj  in  terms  of  x,  y  be  given  by 

<£  (x,  y)  -  &  (x,  y  )  =  0,    ^  (x,  y}  -  rfX  (x,  y}  =  0, 

and  let  the  rational  result  of  eliminating  #,  y  between  these  equations  and  the  initial 
equation  connecting  x,  y  be  denoted  by  F(£,  rj)  =  0,  each  of  $,  ...,  ^,  ^denoting  integral 
polynomials.  Let  two  terms  of  the  expression  (f>(z,  y)  —  ty(&,  y)  =  0  be  axry*—t-bxr'y*'. 
This  expression  and  therefore  all  others  involved  will  be  unaltered  if  «,  6  be  replaced  by 
such  quantities  a  +  h,  b  +  k,  that  hxry*=z£kxr'y*'.  In  a  formal  sense  this  changes  F(£,  rj) 
into 


where  X  ^  1,  and  F  is  such  that  all  differential  coefficients  of  it  in  regard  to  a  and  b  of  order 
less  than  X  are  identically  zero. 

Hence  the  term  within  the  square  brackets  in  this  expression  must  be  zero.     If  it  is 
possible,  choose  now  r  =  rf  +  \  and  s  =  s',  so  that  k= 


*  Salmon's  Higher  Algebra  (1885),  p.  97,  §  103. 


ALGEBRAICAL   FORMULATION.  [5 

Then  we  obtain  the  equation 


This  is  an  equation  of  the  form  above  referred  to,  by  which  x  is  determinate  from  £  and 
T].     And  y  is  similarly  determinate. 

It  will  be  noticed  that  the  rational  expression  of  xt  y  by  £,  rj,  when  it  is  possible 
from  the  equations 


will  not  be  possible,  in  general,  from  the  first  two  equations  :  it  is  only  the  places  x,  y 
satisfying  the  equation  f(x,  y)  =  Q  which  are  rationally  obtainable  from  the  places  £,  17 
satisfying  the  equation  F(£,  r))  =  0.  There  do  exist  transformations,  rationally  reversible, 
subject  to  no  such  restriction.  They  are  those  known  as  Cremona-transformations*. 
They  can  be  compounded  by  reapplication  of  the  transformation  x  :  y  :  I  =  rj  :  {•  :  £»/. 

We  may  give  an  example  of  both  of  these  transformations  — 
For  the  surface 


the  function  £=y2/(^2  +  .£  +  l)  is  of  order  2,  being  infinite  at  the  places  where  x2+z+l  =  0, 
in  each  case  like  (x-a)~°,  and  the  function  r}=x/y  is  of  order  4,  being  infinite  at  the 
places  x*+x+I=0,  in  each  case  like  (^-a)"t,  a  being  the  value  of  x  at  the  place. 
From  the  given  equation  we  immediately  find,  as  the  relation  connecting  £  and  17, 


and  infer,  since  the  equation  formed  as  in  the  general  statement  above  should  be  of 
order  2  in  rj,  that  this  general  equation  will  be 


Thence  in  accordance  with  that  general  statement  we  infer  that  to  each  place  (£,  >;)  on 
the  new  surface  should  correspond  two  places  of  the  original  surface  :  and  in  fact  these  are 
obviously  given  by  the  equations 

r}^=^/ 
If  however  we  take 

£=y2/(#2 

where  «  is  an  imaginary  cube  root  of  unity,  so  that  17  is  a  function  of  order  3,  these 
equations  are  reversible  independently  of  the  original  equation,  giving  in  fact 

x  =  („£  _  wy  )/(£  -  ^},    y  =  (m-    2 
and  we  obtain  the  surface 


having  a  (1,  1)  correspondence  with  the  original  one. 

It  ought  however  to  be  remarked  that  it  is  generally  possible  to  obtain  reversible 
transformations  which  are  not  Cremona-transformations. 

6.  When  a  surface  (x,  y)  is  (1,1)  related  to  a  (£,  77)  surface,  the  defi 
ciencies  of  the  surfaces,  as  denned  by  Riemann  by  means  of  the  connectivity, 
must  clearly  be  the  same. 

*  See  Salmon,  Higher  Plane  Curves  (1879),  §  362,  p.  322. 


6]  RELATION   OF   DEF1CIENCES.  7 

It  is  instructive  to  verify  this  from  another  point  of  view*. — Consider  at 

how  many  places  on  the  original  surface  the  function  -~  is  zero.    It  is  infinite 

CLOG 

at  the  places  where  %  is  infinite:  suppose  for  simplicity  that  these  are 
separated  places  on  the  original  surface  or  in  other  words  are  infinities  of 
the  first  order,  and  are  not  at  the  branch  points  of  the  original  surface.  At 

d£  1 

a  pole  of  £,   ,-  is  infinite  twice.     It  is  infinite  like  —  at  a  branch  place  (a) 

CLOG  v 

where  x  —  a  =  tw+l:  namely  it  is  infinite  ^w  =  2n  +  '2p  -  2  times  t  at  the  branch 
places  of  the  original  surface.  It  is  zero  2n  times  at  the  infinite  places  of  the 
original  surface.  There  remain  therefore  2v  +  2n  +  2p  —  2  —  2n  =  2v  +  2p  —  2 

places  where  ~  is  zero.     If  a  branch  place  of  the  original  surface  be  a  pole 

1         -7fc  1 

of  £,  and  £  be  there  infinite  like  -,  -~  is  infinite  like  - — —  ,  namely  2+w 

t    ax  t2 .  tw 

times :    the  total  number  of  infinities  of  -^  will  therefore  be  the  same  as 

dx 

7«- 

before.     Now  at  a  finite  place  of  the  original  surface  where  -r  =  0,  there  are 

ax 

two  consecutive  places  for  which  £  has  the  same  value.     Since  -  =  1  they  can 

only  arise  from  consecutive  places  of  the  new  surface  for  which  £  has  the 
same  value.  The  only  consecutive  places  of  a  surface  for  which  this  is  the 
case  are  the  branch  places.  Hence  f  there  are  2v+2p  —  2  branch  places  of 
the  new  surface.  This  shews  that  the  new  surface  is  of  deficiency  p. 

When  v/r  is  not  equal  to  1,  the  case  is  different.  The  consecutive  places 
of  the  old  surface,  for  which  £  has  the  same  value,  may  either  be  those  arising 
from  consecutive  places  of  the  new  surface — or  may  be  what  we  may  call 
accidental  coincidences  among  the  v/r  places  which  correspond  to  one  place 
of  the  new  surface.  Conversely,  to  a  branch  place  of  the  new  surface, 
characterised  by  the  same  value  for  £  for  consecutive  placesj,  will  correspond 
vjr  places  on  the  old  surface  where  £  has  the  same  value  for  consecutive 
places.  In  fact  to  two  very  near  places  of  the  new  surface  will  correspond 
v/r  pairs  each  of  very  near  places  on  the  old  surface.  If  then  C  denote  the 
number  of  places  on  the  old  surface  at  which  two  of  the  v/r  places  corre 
sponding  to  a  place  on  the  new  surface  happen  to  coincide,  and  w'  the  number 
of  branch  points  of  the  new  surface,  we  have  the  equation 


'- 
r 


*  Compare  the  interesting  geometrical  account,  Salmon,  Higher  Plane  Curves  (1879),  p.  326, 
§  364,  and  the  references  there  given. 

t  Forsyth,  Tlieory  of  Functions,  p.  348. 

:£  Namely,  near  such  a  branch  place  f  =  a,  £  -  a  is  zero  of  higher  order  than  the  first. 


8  PARAMETERS   NOT   REMOVED  [6 

and  if  p   be  the  deficiency  of  the  new  surface  (of  r  sheets),  this  leads  to  the 
equation 

f 


(2r  +  2pf 


from  which 


Corollary*.  If  p  =p',  then  C  =  (2p  -  2)  (l  -  -\  .  Thus  -  >  1,  so  that 
(7  =  0,  and  the  correspondence  is  reversible. 

We  have,  herein,  excluded  the  case  when  some  of  the  poles  of  £  are  of 
higher  than  the  first  order.  In  that  case  the  new  surface  has  branch  places 
at  infinity.  The  number  of  finite  branch  places  is  correspondingly  less.  The 
reader  can  verify  that  the  general  result  is  unaffected. 

Ex.  In  the  example  previously  given  (§  5)  shew  that  the  function  £  takes  any  given 
value  at  two  points  of  the  original  surface  (other  than  the  branch  places  where  it  is 
infinite),  17  having  the  same  value  for  these  two  points,  and  that  there  are  six  places  at 
which  these  two  places  coincide.  (These  are  the  place  (#  =  0,  y  =  0)  and  the  five  places 
where  x=  —  2.) 

There  is  one  remark  of  considerable  importance  which  follows  from  the 
theory  here  given.  We  have  shewn  that  the  number  of  places  of  the  (x,  y) 

surface  which  correspond  to  one  place  of  the  (£,  97)  surface  is  -  ,  where  v  is  the 

order  of  £  and  r  is  not  greater  than  v,  being  the  number  of  sheets  of  the  (f  ,  77) 
surface  ;  hence,  if  there  were  a  function  £  of  order  1  the  correspondence  would 
be  reversible  and  therefore  the  original  surface  would  be  of  deficiency  1. 

7.  This  notion  of  the  transformation  of  a  Riemann  surface  suggests  an 
inference  of  a  fundamental  character. 

The  original  equation  contains  only  a  finite  number  of  terms  :  the  original 
surface  depends  therefore  upon  a  finite  number  of  constants,  namely,  the 
coefficients  in  the  equation.  But  conversely  it  is  not  necessary,  in  order  that 
the  equation  be  reversibly  transformable  into  another  given  one,  that  the 
equation  of  the  new  surface  contain  as  many  constants  as  that  of  the  original 
surface.  For  we  may  hope  to  be  able  to  choose  a  transformation  whose 
coefficients  so  depend  on  the  coefficients  of  the  original  equation  as  to  reduce 
this  number.  If  we  speak  of  all  surfaces  of  which  any  two  are  connected  by 
a  rational  reversible  transformation  as  belonging  to  the  same  class  f,  it  becomes 
a  question  whether  there  is  any  limit  to  the  reduction  obtainable,  by  rational 
reversible  transformation,  in  the  number  of  constants  in  the  equation  of  a 
surface  of  the  class. 

*  See  Weber,  Crelle,  76,  345. 

t  So  that  surfaces  of  the  same  class  will  be  of  the  same  deficiency. 


7]  BY  TRANSFORMATION.  9 

It  will  appear  in  the  course  of  the  book*  that  there  is  a  limit,  and  that 
the  various  classes  of  surfaces  of  given  deficiency  are  of  essentially  different 
character  according  to  the  least  number  of  constants  upon  which  they  depend. 
Further  it  will  appear,  that  the  most  general  class  of  deficiency  p  is 
characterised  by  3p  —  3  constants  when  p  >  1 — the  number  for  p  =  1  being 
one,  and  for  p  =  0  none. 

For  the  explanatory  purposes  of  the  present  Chapter  we  shall  content 
ourselves  with  the  proof  of  the  following  statement — When  a  surface  is 
reversibly  transformed  as  explained  in  this  Chapter,  we  cannot,  even  though 
we  choose  the  new  independent  variable  £  to  contain  a  very  large  number  of 
disposeable  constants,  prescribe  the  position  of  all  the  branch  points  of  the 
new  surface ;  there  will  be  3p  —  3  of  them  whose  position  is  settled  by  the 
position  of  the  others.  Since  the  correspondence  is  reversible  we  may  regard 
the  new  surface  as  fundamental,  equally  with  the  original  surface.  We 
infer  therefore  that  the  original  surface  depends  on  3p  —  3  parameters — 
or  on  less,  for  the  3/>  —  3  undetermined  branch  points  of  the  new  surface  may 
have  mutually  dependent  positions. 

In  order  to  prove  this  statement  we  recall  the  fact  that  a  function 
of  order  Q  contains^  Q—p  +  l  linearly  entering  constants  when  its  poles 
are  prescribed:  it  may  contain  more  for  values  of  Q<2p  —  1,  but  we 
shall  not  thereby  obtain  as  many  constants  as  if  we  suppose  Q  >  2p  —  2 
and  large  enough.  Also  the  Q  infinities  are  at  our  disposal.  We  can  then 
presumably  dispose  of  2Q-p  +  1  of  the  branch  points  of  the  new  surface. 
But  these  are,  in  number,  2Q  +  2p  —  2  when  the  correspondence  is  reversible. 
Hence  we  can  dispose  of  all  but  2Q  +  2p  -  2  -  (2Q  -p  +  1)  =  3p  -  3  of  the 
branch  points  of  the  new  surface  J. 

Ex.  1.     The  surface  associated  with  the  equation 

y*=x(l  -x]  (l-tfx)  (1  -XV)  (1  -MV)  (l-v*x)  (1  -p%) 
is  of  deficiency  3.     It  depends  on  5  =  2p- 1  parameters,  /c2,  X2,  /u2,  v2,  p2. 

Ex.  2.     The  surface  associated  with  the  equation 

y*+y*(x,  l\+y(x,  !),  +  (#,  1)4=0, 

wherein  the  coefficients  are  integral  polynomials  of  the  orders  specified  by  the  suffixes,  is 
of  deficiency  3.  Shew  that  it  can  be  transformed  to  a  form  containing  only  5  =  2^-1 
parametric  constants. 

*  See  the  Chapters  on  the  geometrical  theory  and  on  the  inversion  of  Abelian  Integrals.  The 
reason  for  the  exception  in  case  ^  =  0  or  1  will  appear  most  clearly  in  the  Chapter  on  the  self- 
correspondence  of  a  Riemann  surface.  But  it  is  a  familiar  fact  that  the  elliptic  functions  which 
can  be  constructed  for  a  surface  of  deficiency  1  depend  upon  one  parameter,  commonly  called 
the  modulus :  and  the  trigonometrical  functions  involve  no  such  parameter. 

t  Forsyth,  p.  459.  The  theorems  here  quoted  are  considered  in  detail  in  Chapter  III.  of  the 
present  book. 

£  Cf.  Kiemann,  Ges.  Werke  (1876),  p.  113.  Klein,  Ueber  Riemann's  Theorie  (Leipzig, 
Teubner,  1882),  p.  65. 


c; 

UN  I VI. 

Of  ~ >-. 


10  SELF-CORRESPONDENCE.  [8 

8.  But  there  is  a  case  in  which  this  argument  fails.  If  it  be  possible  to 
transform  the  original  surface  into  itself  by  a  rational  reversible  transforma 
tion  involving  r  parameters,  any  r  places  on  the  surface  are  effectively 
equivalent  with,  as  being  transformable  into,  any  other  r  places.  Then  the 
Q  poles  of  the  function  £  do  not  effectively  supply  Q  but  only  Q  —  r  dispose- 
able  constants  with  which  to  fix  the  new  surface.  So  that  there  are  3/>  —  3  +  r 
branch  points  of  the  new  surface  which  remain  beyond  our  control.  In  this 
case  we  may  say  that  all  the  surfaces  of  the  class  contain  3p  -  3  disposeable 
parameters  beside  r  parameters  which  remain  indeterminate  and  serve  to 
represent  the  possibility  of  the  self-transformation  of  the  surface.  It  will  be 
shewn  in  the  chapter  on  self-  transformation  that  the  possibility  only  arises 
for  p  =  0  or  p  =  1,  and  that  the  values  of  r  are,  in  these  cases,  respectively 
3  and  1.  We  remark  as  to  the  case  p  =  0  that  when  the  fundamental 
surface  has  only  one  sheet  it  can  clearly  be  transformed  into  itself  by 

a  transformation  involving  three  constants  x—   5      ,  :  and  in  regard  to  p  =  1, 

c%  -f  d 

the  case  of  elliptic  functions,  that  effectively  a  point  represented  by  the 
elliptic  argument  u  is  equivalent  to  any  other  point  represented  by  an 
argument  u  +  7.  For  instance  a  function  of  two  poles  is 


and  clearly  Fa>ft  has  the  same  value  at  u  as  has  Fa+y>p+y  at  u  -f  7  :  so  that  the 
poles  (a,  ft)  are  not,  so  far  as  absolute  determinations  are  concerned,  effective 
for  the  determination  of  more  than  one  point. 

9.     The  fundamental  equation 

a0yn  +  aiyn-l  +  ...+an  =  0, 

so  far  considered  as  associated  with  a  Riemann  surface,  may  also  be  regarded 
as  the  equation  of  a  plane  curve  :  and  it  is  possible  to  base  our  theory  on  the 
geometrical  notions  thus  suggested.  Without  doing  this  we  shall  in  the 
following  pages  make  frequent  use  of  them  for  purposes  of  illustration.  It  is 
therefore  proper  to  remind  the  reader  of  some  fundamental  properties*. 

The  branch  points  of  the  surface  correspond  to  those  points  of  the  curve 
where  a  line  x  =  constant  meets  the  curve  in  two  or  more  consecutive  points  : 
as  for  instance  when  it  touches  the  curve,  or  passes  through  a  cusp.  On  the 
other  hand  a  double  point  of  the  curve  corresponds  to  a  point  on  the  surface 
where  two  sheets  just  touch  without  further  connexion.  Thus  the  branch 
place  of  the  surface  which  corresponds  to  a  cusp  is  really  a  different  singu 
larity  to  that  which  corresponds  to  a  place  where  the  curve  is  touched  by  a 

*  Cf.  Forsyth,  Theory  of  Functions,  p.  355  etc.     Harkness  and  Morley,  Theory  of  Functions, 
p.  273  etc. 


9]  GEOMETRICAL   VIEW.  11 

line  x  =  constant,  being  obtained  by  the  coincidence  of  an  ordinary  branch 
place  with  such  a  place  of  the  Riemann  surface  as  corresponds  to  a  double 
point  of  the  curve. 

Properties  of  either  the  Riemann  surface  or  a  plane  curve  are,  in  the 
simpler  cases,  immediately  transformed.  For  instance,  by  Pliicker's  formulae 
for  a  curve,  since  the  number  of  tangents  from  any  point  is 

f-(n-l)n-2£-3/c, 

where  n  is  the  aggregate  order  in  a;  and  y,  it  follows  that  the  number  of 
branch  places  of  the  corresponding  surface  is 

w  =  t  +  K  =  (n  -  1)  n  -  2  (8  +  K) 

=  2n-2  +  2{iO-l)O-2)-S-4 

Thus  since  w  =  2n  —  2  -j^p,  the  deficiency  of  the  surface  is 

£0-1)0- 2)- S-K, 
namely  the  number  which  is  ordinarily  called  the  deficiency  of  the  curve. 

To  the  theory  of  the  birational  transformation  of  the  surface  corresponds 
a  theory  of  the  birational  transformation  of  plane  curves.  For  example,  the 
branch  places  of  the  new  surface  obtained  from  the  surface  f(x,  y)  =  0  by 
means  of  equations  of  the  form  <£  (x,  y}  —  ty  (x,  y)  =  0,  $  (x,  y)  —  77%  (x,  ?/)  =  0 
will  arise  for  those  values  of  £  for  which  the  curve  </>  (x,  y)  —  jfy  (x,  y)  —  0 
touches  f(x,  y}  =  0.  The  condition  this  should  be  so,  called  the  tact  inva 
riant,  is  known  to  involve  the  coefficients  of  <f>  (as,  y)  —  % \Jr  (x,  y~)  =  0,  and 
therefore  in  particular  to  involve  £,  to  a  degree*  n  (n  —  3)  —  28  —  3/c  +  2nn, 
where  n'  is  the  order  of  <£  (x,  y)  —  £i/r  (x,  y}  =  0.  Branch  places  of  the  new 
surface  also  arise  corresponding  to  the  cusps  of  the  original  curve.  The  total 
number  is  therefore  n  (n  —  3)  —  25  —  2*  +  Znri  =  *2p  —  2'+  2nn'.  Now  nri  is 
the  number  of  intersections  of  the  curves  f(x,  y)  =  Q  and  <£  (x,  y)  —  jfy  (x,  y)  =  0, 
namely  it  is  the  number  of  values  of  t]  arising  for  any  value  of  £,  and  is 
thus  the  number  of  sheets  of  the  new  surface,  which  we  have  previously 
denoted  by  v :  so  that  the  result  is  as  before. 

In  these  remarks  we  have  assumed  that  the  dependent  variable  occurs 
to  the  order  which  is  the  highest  aggregate  order  in  x  and  y  together — and 
we  have  spoken  of  this  as  the  order  of  the  curve.  And  in  regarding  two 
curves  as  intersecting  in  a  number  of  points  equal  to  the  product  of  their 
orders  we  have  allowed  count  of  branches  of  the  curve  which  are  entirely 
at  infinity.  Some  care  is  necessary  in  this  regard.  In  speaking  of  the 
Riemann  surface  represented  by  a  given  equation  it  is  intended,  unless  the 
contrary  be  stated,  that  such  infinite  branches  are  unrepresented.  As  an 
example  the  curve  y-  =  (x,  1)6  may  be  cited. 

Ex,     Prove  that  if  from  any  point  of  a  curve,  ordinary  or  multiple,  or  from  a  point  not 
on  the  curve,  t  be  the  number  of  tangents  which  can  be  drawn  other  than  those  touching 

*  See  Salmon,  Higher  Plane  Curves  (1879),  p.  81. 


12  GENERALITY  [9 

at  the  point,  and  K  be  the  number  of  cusps  of  the  curve — and  if  v  be  the  number  of 
points  other  than  the  point  itself  in  which  the  curve  is  intersected  by  an  arbitrary  line 
through  the  point— -then  t  +  K  —  2i/  is  independent  of  the  position  of  the  point.  If  the 
equation  of  the  variable  lines  through  the  point  be  written  u  —  gv  =  0,  interpret  the  result 
by  regarding  the  curve  as  giving  rise  to  a  Riemann  surface  whose  independent  variable 
fa  |*. 

10.  The  geometrical    considerations  here  referred  to  may  however  be 
stated  with  advantage  in  a  very  general  manner. 

In  space  of  any  (k)  dimensions  let  there  be  a  curve — (a  one-dimension 
ality).  Let  points  on  this  curve  be  given  by  the  ratios  of  the  k  +  1  homo 
geneous  variables  xly  ... ,  xk+1.  Let  u,  v  be  any  two  rational  integral  homo 
geneous  functions  of  these  variables  of  the  same  order.  The  locus  u  —  gv  =  0 
will  intersect  the  curve  in  a  certain  number,  say  v,  points — we  assume  the 
curve  to  be  such  that  this  is  the  same  for  all  values  of  £,  and  is  finite.  Let  all 
the  possible  values  of  £  be  represented  by  the  real  points  of  an  infinite  plane 
in  the  ordinary  way.  Let  w,  t  be  any  two  other  integral  functions  of  the 

w 

coordinates  of  the  same  order.      The  values  of  t]  =  —  at  the  points  where 

t 

u  —  %v  =  0  cuts  the  curve  for  any  specified  value  of  £  will  be  v  in  number. 
As  before  it  follows  thence  that  77  satisfies  an  algebraic  equation  of  order  v 
whose  coefficients  are  one- valued  functions  of  £.  Since  77  can  only  be  infinite 
to  a  finite  order  it  follows  that  these  coefficients  are  rational  functions  of  f . 
Thence  we  can  construct  a  Riemann  surface,  associated  with  this  algebraic 
equation  connecting  f  and  77,  such  that  every  point  of  the  curve  gives  rise  to 
a  place  of  the  surface.  In  all  cases  in  which  the  converse  is  true  we  may 
regard  the  curve  as  a  representation  of  the  surface,  or  conversely. 

Thus  such  curves  in  space  are  divisible  into  sets  according  to  their 
deficiency.  And  in  connexion  with  such  curves  we  can  construct  all  the 
functions  with  which  we  deal  upon  a  Riemann  surface. 

Of  these  principles  sufficient  account  will  be  given  below  (Chapter  VI.) : 
familiar  examples  are  the  space  cubic,  of  deficiency  zero,  and  the  most  general 
space  quartic  of  deficiency  1  which  is  representable  by  elliptic  functions. 

11.  In  this  chapter  we  have  spoken  primarily  of  the  algebraic  equation 
— and  of  the  curve  or  the  Riemann  surface  as  determined  thereby.     But  this 
is  by  no  means  the  necessary  order.     If  the  Riemann  surface  be  given,  the 
algebraic  equation  can  be  determined  from  it — and  in  many  forms,  according 
to  the  function  selected  as  dependent  variable  (y).     It  is  necessary  to  keep 
this  in  view  in  order  fully  to  appreciate  the  generality  of  Riemann's  methods. 
For  instance,  we  may  start  with  a  surface  in  space  whose  shape  is  that  of  an 

*  The  reader  who  desires  to  study  the  geometrical  theory  referred  to  may  consult : — 
Cayley,  Quart.  Journal,  vn. ;  H.  J.  S.  Smith,  Proc.  Lond.  Math.  Soc.  vi. ;  Noether,  Math.  Annul. 
9  ;  Brill,  Math.  Annal.  16  ;  Brill  u.  Noether,  Math.  Annul.  7. 


11]  OF  THE   THEORY.  13 

anchor  ring*,  and  construct  upon  this  surface  a  set  of  elliptic  functions.  Or 
we  may  start  with  the  surface  on  a  plane  which  is  exterior  to  two  circles 
drawn  upon  the  plane,  and  construct  for  this  surface  a  set  of  elliptic  functions. 
Much  light  is  thrown  upon  the  functions  occurring  in  the  theory  by  thus 
considering  them  in  terms  of  what  are  in  fact  different  independent  variables. 
And  further  gain  arises  by  going  a  step  further.  The  infinite  plane  upon 
which  uniform  functions  of  a  single  variable  are  represented  may  be  regarded 
as  an  infinite  sphere ;  and  such  surfaces  as  that  of  which  the  anchor  ring 
above  is  an  example  may  be  regarded  as  generalizations  of  that  simple  case. 
Now  we  can  treat  of  branches  of  a  multiform  function  without  the  use  of  a 
Riemann  surface,  by  supposing  the  branch  points  of  the  function  marked  on 
a  single  infinite  plane  and  suitably  connected  by  barriers,  or  cuts,  across  which 
the  independent  variable  is  supposed  not  to  pass.  In  the  same  way,  for  any 
general  Riemann  surface,  we  may  consider  branches  of  functions  which  are 
not  uniform  upon  that  surface,  the  branches  being  separated  by  drawing 
barriers  upon  the  surface.  The  properties  obtained  will  obviously  generalize 
the  properties  of  the  functions  which  are  uniform  upon  the  surface. 

*  Forsyth,  p.  318 ;  Kiemann,  Ges.  Werke  (1876),  pp.  89,  415. 


[12 


CHAPTER    II. 

THE  FUNDAMENTAL  FUNCTIONS  ON  A  RTEMANN  SURFACE. 

12.  IN  the  present  chapter  the  theory  of  the  fundamental  functions  is 
based    upon    certain    a   priori    existence    theorems*,   originally  given    by 
Riemann.     At  least  two  other  methods  might  be  followed  :  in  Chapters  IV. 
and   VI.  sufficient  indications  are  given  to  enable  the  reader  to  establish 
the    theory   independently    upon    purely   algebraical    considerations  :    from 
Chapter  VI.  it  will  be  seen  that  still  another  basis  is  found  in  a  preliminary 
theory  of  plane  curves.     In  both  these  cases  the  ideas  primarily  involved  are 
of  a  very  elementary  character.     Nevertheless   it   appears  that  Riemann's 
descriptive  theory  is  of  more  than  equal  power  with  any  other  ;    and  that 
it  offers  a  generality  of  conception  to  which  no  other  theory  can  lay  claim. 
It  is  therefore  regarded  as  fundamental  throughout  the  book. 

It  is  assumed  that  the  Theory  of  Functions  of  Forsyth  will  be  accessible 
to  readers  of  the  present  book  ;  the  aim  in  the  present  chapter  has  been  to 
exclude  all  matter  already  contained  there.  References  are  given  also  to 
the  treatise  of  Harkness  and  Morley*. 

13.  Let  t  be  the  infinitesimal  f  at  any  place  of  a  Riemann  surface  :  if  it  is 
a  finite  place,  namely,  a  place  at  which  the  independent  variable  x  is  finite, 
the  values  of  x  for  all  points  in  the  immediate  neighbourhood  of  the  place 
are  expressible  in  the  form  x  =  a  +  tw+1  :    if  an  infinite  place,  x  =  t~(w+1>. 
There  exists  a  function  which  save  for  certain  additive  moduli  is  one-valued 
on  the  whole   surface   and  everywhere  finite  and   continuous,  save  at  the 
place  in  question,  in  the  neighbourhood  of  which  it  can  be  expressed  in  the 
form 


*  See  for  instance  :  Forsyth,  Theory  of  Functions  of  a  Complex  Variable,  1893  ;  Harkness  and 
Morley,  Treatise  on  the  Theory  of  Functions,  1893  ;  Schwarz,  Gesam.  math.  Abhandlungen,  1890. 
The  best  of  the  early  systematic  expositions  of  many  of  the  ideas  involved  is  found  in 
C.  Neumann,  Vorlesungen  ilber  Riemann's  Theorie,  1884,  which  the  reader  is  recommended  to 
study.  See  also  Picard,  Traite  d"  Analyse,  Tom.  n.  pp.  273,  42  and  77. 

t  For  the  notation  see  Chapter  I.  §§  2,  3. 


14]  ELEMENTARY   NORMAL   INTEGRALS.  15 

Herein,  as  throughout,  P  (t)  denotes  a  series  of  positive  integral  powers  of  t 
vanishing  when  t  =  0,  G,  A,  ...  ,  Ar^,  are  constants  whose  values  can  be 
arbitrarily  assigned  beforehand,  and  r  is  a  positive  integer  whose  value  can  be 
assigned  beforehand. 

We  shall  speak  of  all  such  functions  as  integrals  of  the  second  kind  : 
but  the  name  will  be  generally  restricted  to  that  *  particular  function  whose 
behaviour  near  the  place  is  that  of 


This  function  is  not  entirely  unique.  We  suppose  the  surface  dissected 
by  2p  cutsf,  which  we  shall  call  period  loops;  they  subserve  the  purpose  of 
rendering  the  function  one-valued  over  the  whole  of  the  dissected  surface. 
We  impose  the  further  condition  that  the  periods  of  the  function  for  transit 
across  the  p  loops  of  the  first  kind  j  shall  be  zero  ;  then  the  function  is  unique 
save  for  an  additive  constant.  It  can  therefore  be  made  to  vanish  at  an 
arbitrary  place.  The  special  function§  so  obtained  whose  infinity  is  that 

of  -  -  is  then  denoted  by  Tax>  c,  c  denoting  the  place  where  the  function 
vanishes  and  as  the  current  place.  When  the  infinity  is  an  ordinary  place, 

at  which  either  sc  =  a  or  #  =  oo  ,  the  function  is  infinite  either  like  ---- 

x  —  a 

or  -  x.  The  periods  of  T/'  *  for  transit  of  the  period  loops  of  the  second 
kind  will  be  denoted  by  fl1}  ...,  flp. 

14.  Let  Oi^/i),  (#ay2)  be  any  two  places  of  the  surface:  and  let  the 
infinitesimals  be  respectively  denoted  by  tlt  L,  so  that  in  the  neighbourhood 
of  these  places  we  have  the  equations  x  —  xl  =  £1W]+1,  ac  —  x2  =  t.?'*+1.  Let  a 
cut  be  made  between  the  places  (a?,^),  (#2<y2).  There  exists  a  function,  here 
denoted  by  n*1  c  ,  which  (a)  is  one-valued  over  the  whole  dissected  surface, 

3-1,  <<2 

(/3)  has  p  periods  arising  for  transit  of  the  period  loops  of  the  second  kind 
and  has  no  periods  at  the  period  loop  of  the  first  kind,  (7)  is  everywhere 
continuous  and  finite  save  near  (a^)  and  (x.,ij.^),  where  it  is  infinite  re 
spectively  like  log£j  and  -logt,,  and,  (8),  vanishes  when  the  current  place 
denoted  by  x  is  the  place  denoted  by  c.  This  function  is  unique.  If  the 
cut  between  (a?^),  (aray2)  be  not  made,  the  function  is  only  definite  apart 
from  an  additive  integral  multiple  of  2iri,  whose  value  depends  on  the 

*  This  particular  function  is  also  called  an  elementary  integral  of  the  second  kind. 

t  Those  ordinarily  called  the  a,  b  curves;  see  Forsyth,  p.  354.  Harkness  and  Morley, 
p.  242,  etc. 

£  Those  called  the  a  cuts.  ^,- 

§  The  fact  that  the  function  has  no  periods  at  the  period  loops  of  the  first  kind  is  gene 
rally  denoted  by  calling  the  function  a  normal  integral  of  the  second  kind. 


16 


ELEMENTARY   NORMAL   INTEGRALS. 


[14 


path  by  which  the  variable  is  supposed  to  pass  from  c.    It  will  be  called*  the 
integral  of  the  third  kind  whose  infinity  is  like  that  of  Iog(tift2). 

15.  Beside  these  functions  there  exist  also  certain  integrals  of  the  first 
kind — in  number  p.  They  are  everywhere  continuous  and  finite  and  one- 
valued  on  the  dissected  surface.  For  transit  of  the  period  loops  of  the 
first  kind,  one  of  them,  say  Vi,  has  no  periods  except  for  transit  of  the  iih  loop, 
ai.  This  period  is  here  taken  to  be  1.  The  periods  of  Vi  for  transit  of  the 
period  loops  of  the  second  kind  are  here  denoted  by  rtV  ...,  T;P.  We  may 
therefore  form  the  scheme  of  periods 


a. 

do 

dp 

frl 

k 

•Si 

1 

0 

0 

TU 

T1P 

v.2 

0 

1 

0 

T21 

T2P 

• 

VP 

0 

0 

1 

Tfl 

Tpp 

Each  of  these  functions  v^  is  unique  when  a  zero  is  given.  They  will  there 
fore  be  denoted  by  v*'  °,  ...,  vpx>  c,  the  zero  denoted  by  c  being  at  our  disposal. 
The  periods  ry-  have  certain  properties  which  will  be  referred  to  in  their 
proper  place  :  in  particular  ry-  =  T^,  so  that  they  are  certainly  not  equivalent 
to  more  than  %p  (p  +  1)  algebraically  independent  constants.  As  a  fact,  in 
accordance  with  the  previous  chapter,  when  p  >  1  they  are  subject  to 
l)-  (3p  -  3)  =  %(p  -  2)  (p  -  3)  relations. 


16.  In  regard  to  these  enunciations,  the  reader  will  notice  that  the  word 
period  here  used  for  that  additive  constant  arising  for  transit  of  a  period  loop 
—  namely,  in  consequence  of  a  path  leading  from  one  edge  of  the  period  loop 
to  the  opposite  edge  —  would  be  more  properly  called  the  period  for  circuit  of 
this  path  than  the  period  for  transit  of  the  loop. 

The  integrals  here  specified  are  more  precisely  called  the  normal  ele 
mentary  integrals  of  their  kinds.  The  general  integral  of  the  first  kind  is  a 
linear  function  of  Vj  ,  .  .  .  ,  vp  with  constant  coefficients  ;  its  periods  at  the  first 
p  loops  will  not  have  the  same  simple  forms  as  have  those  of  ^  ...  vp.  The 
general  integral  of  the  third  kind,  infinite  like  C  log  (t^/t^,  G  being  a  constant, 
is  obtained  by  adding  a  general  integral  of  the  first  kind  to  CHJ  x  ;  similarly 
for  the  general  integral  of  the  second  kind. 

The  function  II*'  °    hasf  the  property  expressed  by  the  equation 


X,  C 


*  More  precisely,  the  normal  elementary  integral  of  the  third  kind, 
t  Forsyth,  p.  453.     Harkness  and  Morley,  p.  445. 


16]         VARYING  PARAMETER  NEARLY  EQUAL  TO  ARGUMENT.          17 

A  more  general  integral  of  the  third  kind  having  the  same  property  is 

wherein  the  arbitrary  coefficients  satisfy  the  equations  Ay  =  Aji.  The  pro 
perty  is  usually  referred  to  as  the  theorem  of  the  interchange  of  argument 
(a1)  and  parameter  (a^). 

The  property  allows  the  consideration  of 


Il 

*1  ,     2 

as  a  function  of  x^  for  fixed  positions  of  x,  c,  x».     In  this  regard  a  remark 
should  be  made  : 

For  an  ordinary  position  of  x,  the  function 


is  a  finite  continuous  function  of  ar/  when  #/  is  in  the  neighbourhood  of  x. 
But  if  xl  be  a  branch  place  where  w+l  sheets  wind,  and  #/,  x  be  two 
positions  in  its  neighbourhood,  the  functions  of  x 

IT,'    -log  (a?/-*),    Ux'c    --  —  1log(a;  ,-x) 

*1  ,  *2  *„  X2  W+l 

are  respectively  finite  as  x  approaches  #/  and  aclt  so  that 


is  not  a  finite  and  continuous  function  of  x/  for  positions  of  a-/  up  to  and 
including  the  branch  place  a?lt 

In  this  case,  let  the  neighbourhood  of  the  branch  place  be  conformally 
represented  upon  a  simple  plane  closed  area  and  let  £,  £/,  £  be  the  represent 
atives  thereon  of  the  places  xlt  a:/,  x.  Then  the  correct  statement  is  that 


is  a  continuous  function  of  ar/  or  |/  up  to  and  including  the  branch  place  a^. 
This   is  in  fact  the  form  in  which  the  function  n*1''*2  arises  in  the  proof 

X,  C 

of  its  existence  upon  which  our  account  is  based*. 
In  a  similar  way  the  function 

-p*.  c 

regarded  as  a  function  of  #/,  is  such  that 


is  a  finite  continuous  function  of  £'  in  the  immediate  neighbourhood  of  x. 

*  The  reader  may  consult  Neumann,  p.  220. 
B-  2 


18  ONE   INFINITY   AT   A   BRANCH   PLACE.  [17 

17.     It  may  be  desirable  to  give  some  simple  examples  of  these  integrals. 
(a)     For  the  surface  represented  by 

y*=x(x-al)...(x-aap  +  l), 

wherein  alt  ...,  a2p  +  i  are  a^  finite  and  different  from  zero  and  each  other,  consider  the 
integral 

i  (dxfy+ri    y+m\ 
^  J  y  \*-k    *-&/ 

(£>  "?))  (£i>  »?i)  being  places  of  the  surface  other  than  the  branch  places,  which  are 

(0,  0),(alt  0),  ...,  (a2p  +  1,  0). 
It  is  clearly  infinite  at  these  places  respectively  like  log  (x  -  £),  -  log  (x  -  £  t). 

It  is  not  infinite  at  (£,   -r,),  (&,   -7l);  for  (y  +  ?)/(#  -  £),  (y  +  ih)/(*  -  &)  are  finite  at 
these  places  respectively. 

At  a  place  #=00  ,  where  .«  =  r1,  y  =  ft-f~l  (l+P^t}},  t  being  ±1,  and  P1(t)  a  series  of 
positive  integral  powers  of  t  vanishing  for  t  =  0,  we  have 


and  the  integral  has  the  form 


A  being  a  constant.     It  is  therefore  finite. 
At  a  place  y  =  0,  for  instance  where 

B  being  a  constant,  the  integral  has  the  form 

C 
C  being  a  constant,  and  is  finite. 

Thus  it  is  an  elementary  integral  of  the  third  kind  with  infinities  at  (£,  »/),  (£1} 
It  may  be  similarly  shewn  that  the  integral 

,    [dx  fy     y  +  r)i\ 

*j^U~^rJ 

is  infinite  at  (|1}  j^)  like  —  log(.r-  £j)  and  is  not  elsewhere  infinite  except  at  (0,  0). 
Near  (0,  0),  we  have  x=P,y  =  Dt  [1  +P5  (t2)]  and  this  integral  is  infinite  like 

Cdt 


It  is  therefore  an  elementary  integral  of  the  third   kind   with  one  infinity  at  the 
branch  place  (0,  0)  and  the  other  at  (glt  rjj). 

Consider  next  the  integral 

(dx  d 


where  rf  =  -^.     It  can  easily  be  seen  that  it  is  not  infinite  save  at  (£,  17).     Writing  for  the 
ag 

neighbourhood  of  this  place,  which  is  supposed  not  to  be  a  branch  place, 


17]  ONE   INFINITY   AT   A   DOUBLE   POINT.  19 

the  integral  becomes 

(_dx 

](x- 

which  is  equal  to 


Thus  the  integral  is  there  infinite  like  --  ^,  and  is  thus  an  elementary  integral  of 

x~  £ 
the  second  kind. 

The  elementary  integral  of  the  second  kind  for  a  branch  place,  say  (0,  0),  is  a  multiple  of 

»/*. 

2  ]xy 
In  fact  near  #  =  0,  writing  x=tz,  y  =  Dt[l  +P(t2)],  this  integral  becomes 


which  is  equal  to 


as  desired. 

The  integral  is  clearly  not  infinite  elsewhere. 

Example  1.     Verify  that  the  integral  last  considered  is  the  limit  of 

y~ 


y  L#-f 

as  the  place  (£,  rf)  approaches'  indefinitely  near  to  (0,  0). 

Example  2.     Shew  that  the  general  integral  of  the  first  kind  for  the  surface  is 
[dx  I  A       A  A         _n 

y     1  P-I       • 

(/9)  We  have  in  the  first  chapter  §§  2,  3  spoken  of  a  circumstance  that  can  arise,  that 
two  sheets  of  the  surface  just  touch  at  a  point  and  have  no  further  connexion,  and  we 
have  said  that  we  regard  the  points  of  the  sheets  as  distinct  places.  Accordingly  we  may 
have  an  integral  of  the  third  kind  which  has  its  infinities  at  these  two  places,  or  an  integral 
of  the  third  kind  having  one  of  its  infinities  at  one  of  these  places.  For  example,  on  the 
surface 

/(#»  y)  =  (y-  »h#)  (y  -  m??)  +  (#,  y)3 + (x,  y\ = 0 

where  (x,  y)3,  (.?:,  y\  are  integral  homogeneous  polynomials  of  the  degrees  indicated  by  the 
suffixes,  with  quite  general  coefficients,  and  ml,  mz  are  finite  constants,  there  are  at  #=0 
two  such  places,  at  both  of  which  y  =  0. 

In  this  case 

dx 


f'(yY 

where  f(y)  =  g- ,  is  a  constant  multiple  of  an  integral  of  the  third  kind  with  infinities  at 

these  two  places  (0,  0) ;  and 

'-mlx  +  A  x2 +Bxy  +  Cyz   dx 

2—2 


20  EXAMPLES.  [17 

is  a  constant  multiple  of  an  integral  of  the  third  kind,  provided  A  ,  B,  C  be  so  chosen  that 
y  —  iri]X-\-  Ax2  +  Bxy  +  Cy2  vanishes  at  one  of  the  two  places  other  than  (0,  0)  at  which 
Lx+My  is  zero.  Its  infinities  are  at  (i)  the  uncompensated  zero  of  Lx  +  My  which  is  not 
at  (0,  0),  (ii)  the  place  (0,  0)  at  which  the  expression  of  y  in  terms  of  x  is  of  the  form 

y  =  m^x  +  Px2  +  Qx3  +  ... 

In  fact,  at  a  branch  place  of  the  surface  where  x  =  a  +  t'2,  f'(y)  is  zero  of  the  first  order, 

[  dx 
and  dx=2tdt;  thus  I-^TT-^  is  finite  at  the  branch  places.     At  each  of  the  places  (0,  0), 


f(y]  is  zero  of  the  first  order,  Lx  +  My  is  zero  of  the  first  order  and  y  -  m^x  -f-  A  x2  +  Exy  -f  Oy2 
is  zero  at  these  places  to  the  first  and  second  order  respectively.  These  statements  are 
easy  to  verify  ;  they  lead  immediately  to  the  proof  that  the  integrals  have  the  character 
enunciated. 

The  condition  given  for  the  choice  of  A  ,  B,  C  will  not  determine  them  uniquely  —  the 
integral  will  be  determined  save  for  an  additive  term  of  the  form 

dx 


'f'(yY 

where  P,  Q  are  undetermined  constants.  The  reader  may  prove  that  this  is  a  general 
integral  of  the  first  kind.  The  constants  P,  Q  may  be  determined  so  that  the  integral  of 
the  third  kind  has  no  periods  at  the  period  loops  of  the  first  kind,  whose  number  in  this 
case  is  two.  The  reasons  that  suggest  the  general  form  written  down  will  appear  in  the 
explanation  of  the  geometrical  theory. 

(•y)     The  reader  may  verify  that  for  the  respective  cases 

^/4 _ —  ( /\t fy\  ( M J\\    //v» Ci 

the  general  integrals  of  the  first  kind  are 

fdx  ,       *  w         ^ 

I      _    (3C       0)  (3C      C)  * 

Jy6 

'dx          . 
—z(x~c^ 


I 


—a(x-  c)2  [A y2  +  By  (x  -  c)  +  C  (x  -  c)2], 
f 

where  A,  B,  C  are  arbitrary  constants. 

See  an  interesting  dissertation  "de  Transformatione  aequationis  yn  =  R(x}.."  Eugen. 
Netto  (Berlin,  Gust.  Schade,  1870). 

(S)    Ex.     Prove  that  if  F  denote  any  function  everywhere  one  valued  on  the  Riemann 
surface  and  expressible  in  the  neighbourhood  of  every  place  in  the  form 


the  sum  of  the  coefficients  of  the  logarithmic  terms  log  t  of  the  integral    /   Fdx,  for  all 
places  where  such  a  term  occurs,  is  zero. 


18]  PERIODS   OF   INTEGRAL   OF   SECOND    KIND.  21 

It  is  supposed  that  the  number  of  places  where  negative  powers  of  t  occur  in  the 
expansion  of  F  is  finite,  but  it  is  not  necessary  that  the  number  of  negative  powers  be 

finite.  The  theorem  may  he  obtained  by  contour  integration  of  I  Fdx,  and  clearly 
generalizes  a  property  of  the  integral  of  the  third  kind. 

18.     The  value  of  the  integral*  jr*'c  dv*'°  taken  round  the  p  closed  curves 

formed  by  the  two  sides  of  the  pairs  of  period  loops  (alt  b^\  ...,  (av,  bp\  in  such 
a  direction  that  the  interior  of  the  surface  is  always  on  the  left  hand,  is  equal 
to  the  value  taken  round  the  sole  infinity,  namely  the  place  a,  in  a  counter 
clockwise  direction.  Round  the  pair  ar,  br  the  value  obtained  is 

flr  I  dv*'C   , 

taken  once  positively  in  the  direction  of  the  arrow  head  round  what  in  the 
figure  is  the  outer  side  of  br.  This  value  is  Qr(-  a)ir),  where  a>ir  denotes  the 
period  of  vt  for  transit  of  ar,  namely,  from  what  in  the  figure  is  the  inside  of 
the  oval  ar  to  the  outside. 


The  relations  indicated  by  the  figure  for  the  signs  adopted  for  wir,  rir  and 
the  periods  of  T*'  °  will  be  preserved  throughout  the  book. 

Since  a>ir  is  zero  except  when  r  =  i,  the  sum  of  these  p  contour  integrals 
18  —  <>>i ,i^i-     Taken  in  a  counter-clockwise  direction,  round  the  pole  of  F*** 

a     ' 

where 


the  integral  gives 

-  \  +  A  +  Bt  +  CP  +  ...1  \Dv*c  +  t&va.'c  +  -...left, 

where  D  denotes      .     Hence,  as  wit  t  =  1, 


*  Cf.  Forsyth,  pp.  448,  451.     Harkness  and  Morley,  p.  439. 


22  ALL    INTEGRALS   AND   RATIONAL   FUNCTIONS  [IS 

This  is  true  whether  a  be  a  branch  place  or  a  place  at  infinity  (for  which, 
if  not  a  branch  place,  x  =  t-1)  or  an  ordinary  finite  place.     In  the  latter  case 


.  d  (  x, 


x,c\ 

v.       . 

*    / 


j- 
dx\ 

Similarly  the  reader  may  prove  that  the  periods  of  11^'      are 

Orv 
,   ......   0, 


In  this  case  it  is  necessary  to  enclose  x±  and  xz  in  a  curve  winding  Wi  +  1 
times  at  x1}  w2  +  1  times  at  #2,  in  order  that  this  curve  may  be  closed. 

19.  From  these  results  we  can  shew  that  the  integral  of  the  second  kind 
is  derivable  by  differentiation  from  the  integral  of  the  third  kind.  Apart 
from  the  simplicity  thus  obtained,  the  fact  is  interesting  because,  as  will 
appear,  the  analytical  expression  of  an  integral  of  the  third  kind  is  of  the 
same  general  form  whether  its  infinities  be  branch  places  or  not  ;  this  is  not 
the  case  for  integrals  of  the  second  kind. 

We  can  in  fact  prove  the  equation 


namely,  if,  to  take  the  most  general  case,  x±  be  a  winding  place  and  #/  a  place 
in  its  neighbourhood  such  that  #/  =  xl  +  t™    ,  the  equation, 


For,  let  the  neighbourhood  of  the  branch  place  xl  be  conformally  represented 
upon  a  simple  closed  area  without  branch  place,  by  means  of  the  infinitesimal 
of  x,  as  explained  in  the  previous  chapter.  Let  £/,  &  be  the  representatives 
of  the  places  #/,  #1}  and  f  the  representative  of  a  place  x  which  is  very  near 
to  #!,  but  is  so  situate  that  we  may  regard  #/  as  ultimately  infinitely  closer 
to  #1  than  x  is. 

Then  x-x^  =  (f  -  £)w+1, 


where  C  does  not  vanish  for  #/  =  x, 

and  E«!/*«  =  1°£  (x  ~  ^i')  +  3*'  =  l°g  (f  -  £0  +  9  > 

where  <£'  is  finite  for  the  specified  positions  of  the  places  and  remains  finite 
when  gi  is  taken  infinitely  near  to  £j  (§  16). 

X   C 

Also  II  '      = n  log  («  —  a,)  +  d>  =  log  (£  —  tj)  4-  9, 

Xi.  X*  nil  _i_lC>x  '  '  O^3  ;>/  I 


19]  DERIVABLE   FROM    INTEGRAL   OF   THIRD    KIND.  23 

where  <f>  is  also  finite.     Therefore 


X,',  a^  *„  x, 


rn*',c  -  n*'c  ~i         i 

im.  -^r? — fc~^'~~ '    =  ~~  e — fc 


and  thus 

lim 

where  \/r  is  finite. 

Now  as  £/  moves  up  to  £ ,  for  a  fixed  position  of  £,  we  have 

i 

fc '  _  fc   —  (T  '  _  ™  yt!+l  —  / 
?i       <Ti  —  y^i       *i/          ~  •*!  > 

and  rx' e  =  r!1  °  = :L  +  «y, 

%\  «1  ^  £j 

where  ^  is  finite. 

Hence  Dtx  H*' r   -  r*' c 

is  finite  when  x  is  near  to  a;^ 

Moreover  it  does  not  depend  on  #2.     For  from  the  equation 

U*'c    =I%'X2, 

•*J\  j  2/2  •*'»  " 

we  may  regard  H^'  c^  as  a  function  of  xl ,  which  is  determinate  save  for  an 
additive  constant  by  the  specification  of  a;  and  c  only.  This  additive  constant, 
which  is  determined  by  the  condition  that  the  function  vanishes  when  x^  =xz, 
is  the  only  part  of  the  function  which  depends  on  a?2.  It  disappears  in  the 
differentiation. 

Finally,  by  the  determination  of  the  periods  previously  given,  it  follows 
that 

has  no  periods  at  the  2p  period  loops.  Hence  it  is  a  constant,  and  therefore 
zero  since  it  vanishes  when  x  =  c. 

Corollary  i. 

Hence  D,^  =  I>tfDt^^D^Dtx^'  =  D,^'',     \     : 

of  which  neither  depends  on  the  constant  position  c. 

Corollary  ii. 
The  functions 


24  PROOF   FOR   RATIONAL   FUNCTIONS.  [19 

are  respectively  infinite  like 

111 

tx  2 '        tx  3 '        tx  4 '  — 

We  shall  generally  write  DXi,  D2Xi,  ...  instead  of  Dtv ,  D\v .....     When  XT 
is  an  ordinary  place  DXi  will  therefore  mean  -=—  ,  etc. 

Corollary  iii. 

By  means  of  the  example  (8)  of  §  17  it  can  now  be  shewn  that  the  infinite 
parts  of  the  integral 

\Fdx, 


J 


in  which  F  is  any  uniform  function  of  position  on  the  undissected  surface 
having  only  infinities  of  finite  order,  are  those  of  a  sum  of  terms  consisting  of 
proper  constant  multiples  of  integrals  of  the  third  kind  and  differential 
coefficients  of  these  in  regard  to  the  parametric  place. 

20.  One  particular  case  of  Cor.  iii.  of  the  last  Article  should  be  stated. 
A  function  which  is  everywhere  one-valued  on  the  undissected  surface  must 
be  somewhere  infinite.  As  in  the  case  of  uniform  functions  on  a  single 
infinite  plane  (which  is  the  particular  case  of  a  Riemann  surface  for  which 
the  deficiency  is  zero),  such  functions  can  be  divided  into  rational  and 
transcendental,  according  as  all  their  infinities  are  of  finite  order  and  of  finite 
number  or  not.  Transcendental  functions  which  are  uniform  on  the  surface 
will  be  more  particularly  considered  later.  A  rational  uniform  function  can 
be  expressed  rationally  in  terms  of  x  and  y*.  But  since  the  function  can  be 
expressed  in  the  neighbourhood  of  any  of  its  poles  in  the  form 

A          A  A 

n  _L     1  _j_     2  _i_        i  •"•»». 
T  +  ^+">+~r 

we  can,  by  subtracting  from  the  function  a  series  of  terms  of  the  form 


obtain  a  function  nowhere  infinite  on  the  surface  and  having  no  periods  at  the 
first  p  period  loops.  Such  a  function  is  a  constant  f.  Hence  F  can  also  be 
expressed  by  means  of  normal  integrals  of  the  second  kind  only.  Since  F 
has  no  periods  at  the  period  loops  of  the  second  kind  there  are  for  all  rational 
functions  certain  necessary  relations  among  the  coefficients  Alt...,Am. 
These  are  considered  in  the  next  Chapter. 

*  Forsyth,  p.  369.     Harkness  and  Morley,  p.  262. 
t  Forsyth,  p.  439. 


21]  SPECIAL   RATIONAL   FUNCTIONS.  25 

21.  Of  all  rational  functions  there  are  p  whose  importance  justifies  a 
special  mention  here  ;  namely,  the  functions 

dvi     dv2          dvp 
dx  '   dx  '        dx 

In  the  first  place,  these  cannot  be  all  zero  for  any  ordinary  finite  place  a  of 
the  surface.  For  they  are,  save  for  a  factor  2?™',  the  periods  of  the  normal 
integral  F*1  c.  If  the  periods  of  this  integral  were  zero,  it  would  be  a  rational 
uniform  function  of  the  first  order;  in  that  case  the  surface  would  be  repre- 
sentable  conformally  upon  another  surface  of  one  sheet*,  £=  F/-6  being  the 
new  independent  variable  ;  and  the  transformation  would  be  reversible 
(Chap.  I.  §  6).  Hence  the  original  surface  would  be  of  deficiency  zero  ; 
in  which  case  the  only  integral  of  the  first  kind  is  a  constant.  The  functions 
are  all  infinite  at  a  branch  place  a.  But  it  can  be  shewn  as  here  that  the 
quantities  to  which  they  are  there  proportional,  namely  J)avly  ...,  Davp,  cannot 
be  all  zero.  The  functions  are  all  zero  at  infinity,  but  similarly  it  can  be 
shewn  that  the  quantities,  Dv1}  ...  ,  Dvp>  cannot  be  all  zero  there. 

Thus  p  linearly  independent  linear  aggregates  of  these  quantities  cannot  all  vanish  at 
the  same  place.  We  remark,  in  connexion  with  this  property,  that  surfaces  exist  of  all 
deficiencies  such  that  p  -  1  linearly  independent  linear  aggregates  of  these  quantities 
vanish  in  an  infinite  number  of  sets  of  two  places.  Such  surfaces  are  however  special,  and 
their  equation  can  be  putf  into  the  form 

y  =  w  "•  /2P  +  2  • 

We  have  seen  that  the  statement  of  the  property  requires  modification 
at  the  branch  places,  and  at  infinity  ;  this  particularity  is  however  due  to  the 
behaviour  of  the  independent  variable  x.  We  shall  therefore  state  the  pro 
perty  by  saying:  there  is  no  place  at  which  all  the  differentials  dvlt  ...,  dvp 
vanish.  A  similar  phraseology  will  be  adopted  in  similar  cases.  For  instance, 
we  shall  say  that  each  of  dvl}  dv^,  ...  ,  dvp  has|  2p  —  2  zeros,  some  of  which 
may  occur  at  infinity. 

In  the  next  place,  since  any  general  integral  of  the  first  kind 


must  necessarily  be  finite  all  over  any  other  surface  upon  which  the  original 
surface  is  conformally  and  reversibly  represented  and  therefore  must  be  an 
integral  of  the  first  kind  thereon,  it  follows  that  the  rational  function 


dx  p  dx 

*  I  owe  this  argument  to  Prof.  Klein.  +  See  below,  Chap.  V. 

J  See  Forsyth,  p.  461.     Harkness  ami  Morley,  p.  450. 


26  INVARIANCE    OF   THEIR   RATIOS.  [21 

is  necessarily  transformed  with  the  surface  into 

dV 


where  Vi  =  Vt  is  an  integral  of  the  first  kind,  not  necessarily  normal,  on  the 
new  surface,  f  being  the  new  independent  variable,  and  M  =  ~  . 

(LOG 

Thus,  the  ratios  of  the  integrands  of  the  first  kind  are  transformed 
into  ratios  of  integrands  of  the  first  kind ;  they  may  be  said  to  be  invariant 
for  birational  transformation. 

This  point  may  be  made  clearer  by  an  example.  The  general  integral 
of  the  first  kind  for  the  surface 

y-  =  (as,  1)8 
can  be  shewn  to  be 

'dx  , 


y 

A,  B,  C  being  arbitrary  constants. 

If  then  0!  :  0o  :  03  denote  the  ratios  of  any  three  linearly  independent 
integrands  of  the  first  kind  for  this  surface,  we  have 

for  proper  values  of  the  constants  altbi,  ... ,  c3, 
and  hence 


Such  a  relation  will  therefore  hold  for  all  the  surfaces  into  which  the  given 
one  can  be  birationally  transformed. 

22.  It  must  be  remarked  that  the  determination  of  the  normal  integrals 
here  described  depends  upon  the  way  in  which  the  fundamental  period  loops 
are  drawn.  An  integral  of  the  first  kind  which  is  normal  for  one  set  of 
period  loops  will  be  a  linear  function  of  the  integrals  of  the  first  kind  which 
are  normal  for  another  set ;  and  an  integral  of  the  second  or  third  kind,  which 
is  normal  for  one  set  of  period  loops,  will  for  another  set  differ  from  a  normal 
integral  by  an  additive  linear  function  of  integrals  of  the  first  kind. 


27 


CHAPTER   III. 

THE  INFINITIES  OF  RATIONAL  UNIFORM  FUNCTIONS. 

23.  IN  this  chapter  and  in  general  we  shall  use  the  term  rational  function 
to  denote  a  uniform  function  of  position  on  the  surface  of  which  all  the 
infinities  are  of  finite  order,  their  number  being  finite.  We  deal  first  of  all 
Avith  the  case  in  which  these  infinities  are  all  of  the  first  order. 

If  k  places  of  the  surface,  say  a^,  a2  •••«*,  be  arbitrarily  assigned  we  can 
always  specify  a  function  with  p  periods  having  these  places  as  poles,  of  the 
first  order,  and  otherwise  continuous  and  uniform  ;  namely,  the  function  is  of 
the  form 


where  the  coefficients  /*0,  /^  ...  /A^  are  constants,  the  zeros  of  the  functions  F 
being  left  undetermined.  Conversely,  as  remarked  in  the  previous  chapter 
(§  20),  a  rational  function  having  a,,  ...,  a^  as  its  poles  must  be  of  this  form. 
In  order  that  the  expression  may  represent  a  rational  function  the  periods 
must  all  be  zero.  Writing  the  periods  of  F£  in  the  form  fij  (a),  ...,£lp  (a), 
this  requires  the  equations 


(cr.a)  +  .  .  .  +  A**n,-  (at)  =  0, 

for  all  the  p  values,  i  =  1,  2,  .  .  .  ,  p,  of  i.  In  what  follows  we  shall  for  the  sake 
of  brevity  say  that  a  place  c  depends  upon  r  places  c1}  c2,  ...,  cr  when  for  all 
values  of  i,  the  equations 

fli  (C)  =f&i  (C,)  +  .  .  .  +/A  (C,.) 

hold  for  finite  values  of  the  coefficients  fi,--',fr,  these  coefficients  being 
independent  of  i.  Hence  we  may  also  say  : 

In  order  that  a  rational  function  should  exist  having  k  assigned  places  as 
its  poles,  each  simple,  one  at  least  of  these  places  must  depend  upon  the  others. 

24.     Taking  the  k  places  c^,  a2,  ...,  a*  in  the  order  of  their  suffixes,  it  may 
of  course  happen  that  several  of  them  depend  upon  the  others,  say  a,+i,  ...,««,- 


28  DEPENDENCE    OF    POLES   OF    A    RATIONAL    FUNCTION  [24 

upon  ttx,  ...,  as,  the  latter  set  an  .  ..,  as  being  independent:   then  we  have 
equations  of  the  form 


,+lf 


fti  (a*)    =  nt,  !  fti  (aO    +  .  .  .  +  nk>  ,  Of  (a,), 

the  coefficients  in  any  of  the  rows  here  being  the  same  for  all  the  p  values  of 
i.  In  particular,  if  s  be  as  great  as  p  and  alt  ...  ,  as  be  independent,  equations 
of  this  form  will  hold  for  all  positions  of  as+1,  ...,  ak.  For  then  we  have 
enough  disposeable  coefficients  to  satisfy  the  necessary  p  equations. 

When  it  does  so  happen,  that  a8+1,...,ak  depend  upon   0,1...  at,  there 
exist  rational  functions,  of  the  form 


i      — 


wherein  cr4+1  ...  o-^,  Xs+1  ...  X^  are  constants,  which  are  all  infinite  once  in 
ttj  ...  as  and  are,  beside,  infinite  respectively  at  as+1)  ...,  a^  ;  and  the  most 
general  function  uniform  on  the  dissected  surface,  which  is  infinite  to  the 
first  order  at  a1,  .  .  .  ,  a^  ,  being,  as  remarked,  of  the  form 


/*<>  +  PI  r  4- 

can  be  written  in  the  form 


4 

+  /%|r-     ^*   -hn*.  i     It,  +  ......  +nktS    F^- 

\_^k 

namely,  in  the  form 

v0  +  z/ir*i  +  ......  +  v,  F^  +  vg+1Rt+1  +  ......  +vkRk. 

If  this  function  is  to  have  no  periods,  the  equations 

vini(al)  +  ......  +  v.n»  (a.)  =  0,     (i=l,  2,  ...,p), 

must  hold.  Since  a1}  ...,as  are  independent,  such  equations  can  only  hold 
when  Vi  =  0  =  .  .  .  =  vg.  Thus  the  most  general  rational  function  having  k 
poles  of  the  first  order,  at  a1}  ...,  a*,  is  of  the  form 

i/o  +  vs+lJRg+1  +  ......  +  vkRk, 

and  involves  k  —s+  I  linearly  entering  constants,  s  being  the  number  of 
places  among  alf  ...  ,  ak  which  are  independent.  These  constants  will  generally 
be  called  arbitrary  :  they  are  so  only  under  the  convention  that  a  function 


25]  DETERMINES    EXPRESSION   OF   FUNCTION.  29 

which  has  all  its  poles  among  a1}  ...,ak  be  reckoned  a  particular  case  of  a 
function  having  each  of  these  as  poles  ;  for  it  is  clear  that,  for  instance,  Rk  is 
only  infinite  at  a1(  ...,  at,  ak.  The  proposition  with  a  slightly  altered  enuncia 
tion,  given  below  in  §  27  and  more  particularly  dealt  with  in  §  37,  is  called 
the  Riemann-Roch  Theorem,  having  been  first  enunciated  by  Riemann*, 
and  afterwards  particularized  by  Rochf. 

25.  Take  now  other  places  ak+l,  ak+2,  ...  upon  the  surface  in  a  definite 
order,  and  consider  the  possibility  of  forming  a  rational  function,  which  beside 
simple  infinities  at  alt  ...,  ak  has  other  simple  poles  at,  say,  ak+1,  ak+z,  ...,ah. 
By  the  first  Article  of  the  present  chapter  it  follows  that  the  least  value 
of  h  for  which  this  will  be  possible  will  be  that  for  which  ah  depends 
on  ch  ...  akak+l  ...  a/,-i,  that  is,  depends  on  a^  .  .  .  as  ak+l  .  .  .  «&_!.  This  will 
certainly  arise  at  latest  when  the  number  of  these  places  a^  ...  as  ak+l  .  .  .  ah-i 
is  as  great  as  p,  namely  h  —  l=k  +  p  —  s,  and  if  none  of  the  places  ak+l  .  .  .  «/,_! 
depend  upon  the  preceding  places  ax  ...  as,  it  will  not  arise  before:  in  that 
case  there  will  be  no  rational  function  having  for  poles  the  places 


ak+j 
for  any  value  of  j  from  1  to  p  —  s. 

But  in  order  to  state  the  general  case,  suppose  there  is  a  value  of  j  less 
than  or  equal  to  p  —  s,  such  that  each  of  the  places 

ak+j+i  ......  ah 

depends  upon  the  places 


the  smallest  value  of  j  for  which  this  occurs  being  taken,  so  that  no  one  of 
ak+1  .  .  .  ak+j  depends  on  the  places  which  precede  it  in  the  series 


Then  there  exists  no  rational  function  with  its  poles  at  a,  ...  ak  ak+l  ...  ak+j, 
but  there  exist  functions 


ia 


,s  1  as  ~  nk+j+i,k+i  1  ak  +  l  ~  ......  ~  nk+}+i,k+j  1  ak  +  i  J  > 

whose  poles  are  respectively  at 


for  all  values  of  i  from  1  to  h  —  k  —  j. 

*  Riemann,  Ges.  Werke,  1876,  p.  101  (§  5)  and  p.  118  (§  14)  and  p.  120  (§  16). 
t  Crelle,  64.     Cf.  also  Forsyth,  pp.  459,  464.     The  geometrical  significance  of  the  theorem 
has  been  much  extended  by  Brill  and  Noether.     (Math.  Ann.  vii.) 


30  STATEMENT   OF   COMPLETE    RESULT.  [25 

Then  the  most  general  rational  function  with  poles  at 


is  in  fact 


and  involves  k  —  s  +  i  +  1  arbitrary  constants,  namely  the  same  number  as 
that  of  the  places  of  the  set 


which  depend  upon  the  places  that  precede  them. 
For  such  a  function  must  have  the  form 


-1-  P-k+j  lak 

namely, 


—  s 

"i"    ^    Ps+r      ^         -tts+r  T  ^s+r,  I  *•  «,  T  ......  T  ^s+r,s  *•  a,        C 

r=l  L^-«+r  ^-s+r 

1  T& 

AfcffH  +  nk+}+t,i  !«,  +  ...... 

H 

r"31    .  rix  n* 

t,  s  1  a,  +  Vk+j+t,  k+i  i  ak  +  1  +  ......  +  Kk+j+t,  k+j  A  ak  +, 


which  is  of  the  form 

V0  +  Vi  t\^  +  ......  +  V8 

+  vk+l  r^  +  1  +  ...... 

and  the  p  periods  of  this,  each  of  the  form 
Vi  H  (ttj)  +  ......  +  i/»ft  (a,.)  +  i>t+1  ft 

cannot  be  zero  unless  each  of  vl  ...  vsvk+i  •••  »k+j  be  zero,  for  it  is  part  of 
the  hypothesis  that  none  of  ak+1  .  .  .  ak+j  depend  upon  preceding  places. 

26.  Proceeding  in  this  way  we  shall  clearly  be  able  to  state  the  following 
result  — 

Let  there  be  taken  upon  the  surface,  in  a  definite  order,  an  unlimited 
number  of  places  al}  a2,  —  Suppose  that  each  of  al...a,Q_  is  inde 
pendent  of  those  preceding  it,  but  each  of  a^,^  ...  aQi  depends  on 
a,  ...  a«  Suppose  that  each  of  an  ,  ,  a~  ^  .  .  an  is  independent  of 

Ifc—fl  Vi  +  l     Vi  +  4  Va~9i 

those  that  precede  it  in  the  series  a,  ...  an      an,....an         but  each   of 

VI  -9i     9fT*  V2~9a' 

aQ,-^i  •••  %  dePends  uP°n  «i  •••  aQl-qiaQl+i  •••  aQt.qt'  This  requires  that 


26]  EXPRESSION   OF    FUNCTION    OF   ASSIGNED   POLES.  31 

Suppose  that  each  of  aQ  +l  .  .  .  aQ  _  is  independent  of  those  that  precede  it 
in  the  series  a,  ...  a~  a~  ,  .  .  .  .  an  «„  ,  .  .  .  .  an  ,  but  each  of  an  .....  an 

Qi-9i     Ci+l  Qi-<lt     Qs+l  Qi-Qs  §3-93+1  Qa 

depends  upon  the  places  of  this  series.     This  requires  that 

Qi-qi  +  [Q2-q^-Qi]  +  [Q3-q3-Q2]>p- 

Let  this  enumeration  be  continued.  We  shall  eventually  come  to  places 
aQ  +i'aQ  +2'  "•  ao  -  '  eac^  ^dependent  of  the  places  preceding,  for  which 
the  total  number  of  independent  places  included,  that  is,  of  places  which 
do  not  depend  upon  those  of  our  series  which  precede  them,  is  p  —  so  that 
the  equation 


will  hold.     Then  every  additional  place  of  our  series,  those,  namely,  chosen 
in  order  from  aQ  _    +l,aQ  _    +2,  ...  will  depend  on  the  preceding  places  of  the 

whole  series. 

This  being  the  case,  it  follows,  using  Rf  as  a  notation  for  a  rational 
function  having  its  poles  among  al  ...  a/,  that  rational  functions 


do  not  exist. 

The  number  of  these  non-existent  functions  is  p. 

For  all  other  values  off,  a  rational  function  Rj  exists. 

To  exhibit  the  general  form  of  these  existing  rational  functions  in  the 
present  notation,  let  m  be  one  of  the  numbers  1,  2,  ...,  h;  i  be  one  of  the 
numbers  1,  2,  ...  qtn,  and  let  the  dependence  of  aQ  _  .  upon  the  preceding 

places  arise  by  p  equations  of  the  form 


then,  denoting  P*   by  F,.,  there  is  a  rational  function 


which  has  its  poles  at 

a'  •'•  aft-7,'  %+!•••  aQ.>-<,.>>  •—  aQn 
and  the  general  rational  function  having  its  poles  at 


~'a<jm-9m> 


32  THERE   ARE  p  GAPS.  [26 

is  of  the  form 


and  involves  ql  +  qz  +  .  .  .  4-  <?m_i  +  i  +  1  arbitrary  coefficients. 

The  result  may  be  summarised  by  putting  down  the  line  of  symbols 


(&-?,  +  !),..,&,  &  +  !,...  ,&-,  +  !,  ...,(&-?*),  (&-?*+!),... 
with  a  bar  drawn  above  the  indices  corresponding  to  the  places  which  depend 
upon  those  preceding  them  in  the  series.  The  bar  beginning  over  Qh  —  qh  +  I 
is  then  continuous  to  any  length.  The  total  number  of  indices  over  which 
no  bar  is  drawn  is  p.  There  exists  a  rational  function  Rf,  in  the  notation 
above,  for  every  index  which  is  beneath  a  bar. 

The  proposition  here  obtained  is  of  a  very  fundamental  character.  Sup 
pose  that  for  our  initial  algebraic  equation  or  our  initial  surface,  we  were  able 
only  to  shew,  algebraically  or  otherwise,  that  for  an  arbitrary  place  a  there 
exists  a  function  Kxa,  discontinuous  at  a  only  and  there  infinite  to  the  first 
order,  this  function  being  one  valued  save  for  additive  multiples  of  &  periods, 
and  these  periods  finite  and  uniquely  dependent  upon  a,  then,  taking  arbitrary 
places  a1}  a2,  ...  upon  the  surface,  in  a  definite  order,  and  considering  func 
tions  of  the  form 


that  is,  functions  having  simple  poles  at  al}  ...,  a#,  we  could  prove,  just  as 
above,  that  there  are  k  values  of  N  for  which  such  functions  cannot  be  one 
valued  ;  and  obtain  the  number  of  arbitrary  coefficients  in  uniform  functions 
of  given  poles.  Namely,  the  proposition  would  furnish  a  definition  of  the 
characteristic  number  k  —  which  is  the  deficiency,  here  denoted  byp  —  based 
upon  the  properties  of  the  uniform  rational  functions. 

We    shall    sometimes    refer    to    the    proposition    as    Weierstrasss   gap 
theorem*. 

27.     When  a  place  a  is,  in  the  sense  here  described,  dependent  upon  places 
bi}  62,  ...  ,  br,  it  is  clear  that  of  the  equations 

*  "  Liickensatz."  The  proposition  has  been  used  by  Weierstrass,  I  believe  primarily  under 
the  form  considered  below,  in  which  the  places  ax,  a2,  ...  are  consecutive  at  one  place  of  the 
surface,  as  the  definition  of  p.  Weierstrass's  theory  of  algebraic  functions,  preliminary  to  a  theory 
of  Abelian  functions,  is  not  considered  in  the  present  volume.  His  lectures  are  in  course  of 
publication.  The  theorem  here  referred  to  is  published  by  Schottky  :  Conforme  Abbildung 
mehrfach  zusammenhangender  ebener  Flachen,  Crelle  Bd.  83.  A  proof,  with  full  reference  to 
Schottky,  is  given  by  Noether,  Crelle  Bd.  97,  p.  224. 


27]  TRANSPOSITION   OF  THE   LINEAR  CONDITIONS.  33 


A.n,  (br)  +  .  .  .  +  Apfip  (br)  =  o 

A.fl^a)  +...  +  Apflp(a)  =  0 

the  last  is  a  consequence  of  those  preceding  —  and  conversely  that  when  the 
last  equation  is  a  consequence  of  the  preceding  equations  the  place  a  depends 
upon  the  places  b1}  b2,  ...,  br. 

Hence  the  conditions  that  the  linear  aggregate 

0  (as)  =  A&  (as)  +  .  .  .  +  Apnp  (as) 
should  vanish  at  the  places 

^"•aQlaQi+l--'aQ3aQ,+l'"aQm-<)a+i' 

wherein  i$>  qm,  are  equivalent  to  only 


or 


linearly  independent  equations. 

If  then  r  +  1  be  the  number  of  linearly  independent  linear  aggregates  of 
the  form  £1  (as),  which  vanish  in  the  Qm  -  qm  -f  i  specified  places,  we  have 

T  +  1  =p  -  (Qm  -  ql  -  ...  -  qm). 

Denoting  Qm  —  qm  +  i  by  Q,  and  the  number  of  constants  in  the  general 
rational  function  with  poles  at  the  Q  specified  places,  of  which  constants  one 
is  merely  additive,  by  q  +  1, 

q  +  1  =  q,  +  q2  +  ...  +  qm^  +  i  +  1. 
We  therefore  have 

Q-q=p-(r  +  i). 

Recalling  the  values  of  fl^ar)...  Clp(x)  and  the  fact  (Chapter  II.  §  21) 
that  every  linear  aggregate  of  them  vanishes  in  just  2p  -  2  places,  we  see 
that  when  Q  is  greater  than  2p  -  2,  T  +  1  is  necessarily  zero. 

In  the  case  under  consideration  in  the  preceding  article  the  number 
T  +  1  for  the  function  EQ  ,  namely  the  number  of  linearly  independent 
linear  aggregates  ft  (as)  which  vanish  in  the  places 


is  given,  by   taking  m  =  h-l   and  i  =  qh_,  in  the  formula  of  the  present 
article,  by  the  equation 


r  +  1  =  p  - 

=  Qh 
B. 


34  POLES   AT   ONE   PLACE.  [27 

Hence  one  such  linear  aggregate  vanishes  in  the  places 


and  therefore 

&-?*-!  >2p-2 

or,  the  index  associated  with  the  last  place  aQ  _    of  our  series,  corresponding  to 

^h       'k 

which  a  rational  function  RQ  _    does  not  exist,  is  not  greater  than  2p  —  1.    A 

^A      ^A 

case  in  which  this  limit  is  reached,  which  also  furnishes  an  example  of  the 
theory,  is  given  below  §  37,  Ex.  2. 

28.  A  limiting  case  of  the  problem  just  discussed  is  that  in  which  the 
series  of  points  a1}  a.2,  ...  are  all  consecutive  at  one  place  of  the  surface. 

A  rational  function  which  becomes  infinite  only  at  a  place,  a,  of  the 
surface,  and  there  like 

GI          GZ  Cf 

t       P  tr  ' 

where  any  of  the  constants  Glt  C2,  ...  Cr_lt  but  not  Cr,  maybe  zero,  t  being  the 
infinitesimal,  is  said  to  be  there  infinite  to  the  rth  order.  If—  A.t-  =  G[/(i  —  1)!, 
such  a  function  can  be  expressed  in  a  form 

x  +  XjF*  +  x2z>ar*  +  ...  +  vo^rs 

where,  in  order  that  the  function  be  one  valued  on  the  undissected  surface, 
the  p  equations 

X,  flf  (a)  +  \2Da  nf  (a)  +  .  .  .  +  X^"1  «;  (a)  =  0 

must  be  satisfied  :  and  conversely  these  equations  give  sufficient  conditions 
for  the  coefficients  X1;  Xg,  ...  ,  X,.. 

In  other  words,  since  Xr  cannot  be  zero  because  the  function  is  infinite  to 
the  ?'th  order,  the  p  differential  coefficients  D^~lCli(a),  each  of  the  r—  1th 
order,  must  be  expressible  linearly  in  terms  of  those  of  lower  order, 


with  coefficients  which  are  independent  of  i.  We  imagine  the  p  quantities 
Du~1fli(a),  for  i  =  l,  2,  ...,p,  written  in  a  column,  which  we  call  the  rth 
column  ;  and  for  the  moment  we  say  that  the  necessary  and  sufficient  con 
dition  for  the  existence  of  a  rational  function,  infinite  of  the  rth  order  at  a, 
and  not  elsewhere  infinite,  is  that  the  rth  column  be  a  linear  function 
of  the  preceding  columns. 

Then  as  before,  considering  the  columns  in  succession,  they  will  divide 
themselves  into  two  categories,  those  which  are  linear  functions  of  the  pre 
ceding  ones  and  those  which  are  not  so  expressible.  And,  since  the  number 
of  elements  in  a  column  is  p,  the  number  of  these  latter  independent  columns 


30]  CORRESPONDING  TRANSPOSITION   OF   LINEAR  CONDITIONS.  35 

will  be  just  p.  Let  them  be  in  succession  the  ^th,  &2th,  ...,kpt\\.  Then 
there  exists  no  rational  function  infinite  only  at  a,  and  there  to  these 
orders  klt  k2,  ...,  kp,  though  there  are  integrals  of  the  second  kind  infinite 
to  these  orders.  But  if  Q  be  a  number  different  from  klt  ...,  kp,  there  does 
exist  such  a  rational  function  of  the  Qth  order,  its  most  general  expression 
being  of  the  form 

xQD(?-ir*  +  XQ-xA?-2^  +  ...  +  xxr*  +  x, 

namely,  the  integral  of  the  second  kind  whose  infinity  is  of  order  Q  is 
expressible  linearly  by  integrals  of  the  second  kind  of  lower  order  of  infinity, 
with  the  addition  of  a  rational  function. 

If  q  +  1  be  the  number  of  linearly  independent  coefficients  in  this  function, 
one  being  additive,  we  have  an  equation 

Q-q=P-(r  +  i), 

where  p  —  (r  +  1)  is  the  number  of  the  linearly  independent  equations  of  the 
form 

\iflf  (a)  +  X2Z)nt-(a)  +  ...  +  \QD^fli  (a)  =  0,      (i  =  1,  2,  ...,  p), 

from  which  the  others  may  be  linearly  derived.  As  before,  r  +  I  is  the 
number  of  linearly  independent  linear  aggregates  of  the  form 


which  satisfy  the  Q  conditions 

A.D^,  (a)  +  ...  +  ApDrnp  (a)  =  0 
forr  =  0,  1,2,  ...,Q-1. 

29.  In  regard  to  the  numbers  ^  .  .  .  kp  we  remark  firstly  that,  unless  p  =  0, 
&!  =  1  —  for  if  there  existed  a  rational  function  with  only  one  infinity  of  the 
first  order,  the  positive  integral  powers  of  this  function  would  furnish  rational 
functions  of  all  other  orders  with  their  infinity  at  this  one  place,  and  there 
would  be  no  gaps  (compare  the  argument  Chapter  II.  §  21);   and  further 
that  in  general  they  are  the  numbers  1,  2,  3  ...  p,  that  is  to  say,  there  is  only 
a  finite  number  of  places  on  the  surface  for  which  a  rational  function  can  be 
formed  infinite  there  to  an  order  less  than  p  +  1  and  not  otherwise  infinite. 
We  shall  prove  this  immediately  by  finding  an  upper  and  a  lower  limit  to 
the  number  of  such  places  (§  31). 

30.  Some  detailed  algebraic  consequences  of  this  theory  will  be  given  in 
Chapter  V.     It  may  be*  here  remarked,  what  will  be  proved  in  Chapter  VI. 
in  considering  the  geometrical  theory,  that  the  zeros  of  the  linear  aggregate 


It   is  possible  that  the  reader  may  find  it  more  convenient  to  postpone  the  complete 
discussion  of  §  30  until  after  reading  Chapter  vi. 

3—2 


36  ILLUSTRATION   FROM   THE   SUBSEQUENT  [30 

can  be  interpreted  in  general  as  the  intersections  of  a  certain  curve,  of  the 
form 

</>  =  A^  (x)  +  ...+  Ap(f>p  O)  =  0, 

wherein  ^...^>p  are  integral  polynomials  in  x  and  y,  with  the  curve  repre 
sented  by  the  fundamental  equation  of  our  Riemann  surface.  In  such 
interpretation,  the  condition  for  the  existence  of  a  rational  function  of  order  Q 
with  poles  only  at  the  place  a,  is  that  the  fundamental  curve  be  of  such 
character  at  this  place  that  every  curve  <£,  obtained  by  giving  different  values 
to  A1...  Ap,  which  there  cuts  it  in  Q—  1  consecutive  points,  necessarily  cuts 
it  in  Q  consecutive  points.  As  an  instance  of  such  property,  which  seems 
likely  also  to  make  the  general  theory  clearer,  we  may  consider  a  Riemann 
surface  associated  with  an  equation  of  the  form 

f(x,  y)  =  K  +  (x,  y\  +  (x,  y\  +  (x,  y)3  +  (x,  y\  =  0, 

wherein  (x,  y)r  is  a  homogeneous  integral  polynomial  of  the  rth  degree,  with 
quite  general  coefficients,  and  K  is  a  constant.  Interpreted  as  a  curve,  this 
equation  represents  a  general  curve  of  the  fourth  degree ;  it  will  appear 
subsequently  that  the  general  integral  of  the  first  kind  is 

dx    (A+Bx+Cy), 


where  f  (y)  =  df/dy,  and  A  ,  B,  0  are  arbitrary  constants  ;  and  thence,  if  we 
recall  the  fact  that  flj  (as),  ...,£lp(x)  are  differential  coefficients  of  integrals 
of  the  first  kind,  that  the  zeros  of  the  aggregate 


may  be  interpreted  as  the  intersections  of  the  quartic  with  a  variable  straight 
line. 

Take  now  a  point  of  inflexion  of  the  quartic  as  the  place  a.  Not  every 
straight  line  there  intersecting  the  curve  in  one  point  will  intersect  it  in  any 
other  consecutive  point  ;  but  every  straight  line  there  intersecting  the  curve 
in  two  consecutive  points  will  necessarily  intersect  it  there  in  three  consecu 
tive  points.  Hence  it  is  possible  to  form  a  rational  function  of  the  third 
order  whose  only  infinities  are  at  the  place  of  inflexion  ;  in  fact,  if 


be  the  equation  of  the  inflexional  tangent,  and 


be  the  equation  of  any  line  through  the  fourth  point  of  intersection  of  the 
inflexional  tangent  with  the  curve,  the  ratio  of  the  expressions  on  the  left 
hand  side  of  these  equations,  namely 

Ax  +  By  +  1 


30]  GEOMETRICAL  THEORY.  37 

is  a  general  rational  function  of  the  desired  kind,  as  is  immediately  obvious 
on  consideration  of  the  places  where  it  can  possibly  be  infinite.  Thus  for  the 
inflexional  place  the  orders  of  two  non-existent  rational  functions  are  1,  2. 
It  can  be  proved  that  in  general  there  is  no  function  of  the  fourth  order  —  the 
gaps  at  the  orders  1,  2,  4  are  those  indicated  by  Weierstrass'  theorem. 

In  verification  of  a  result  previously  enunciated  we  notice  that  since 
Ax  +  By+  1  =  0  may  be  taken  to  be  any  definite  line  through  the  fourth 
intersection  of  the  inflexional  tangent  with  the  curve,  the  function  contains 
#  +  1  =  2  arbitrary  constants.  From  the  form  of  the  integrals  of  the  first 
kind  which  we  have  quoted,  it  follows  that  p  =  3  ;  thus  the  formula 


wherein  Q  =  3,  requires  r  +  1  =  1  ;  now  by  §  28  r  +  1  should  be  the  number 
of  straight  lines  which  can  be  drawn  to  have  contact  of  the  second  order  with 
the  curve  at  the  point  :  this  is  the  case. 

If  the  quartic  possess  also  a  point  of  osculation,  a  straight  line  passing 
through  two  consecutive  points  of  the  curve  there  will  necessarily  pass 
through  three  consecutive  points  and  also  necessarily  through  four.  Hence, 
for  such  a  place,  we  can  form  a  rational  function  of  the  third  order  and  one 
of  the  fourth.  In  fact,  if  A<p  +  B0y  +  1=0  be  the  tangent  at  the  point  of 
osculation  and  A^x  +  BJJ  +  1  =  0  be  any  other  line  through  this  point,  while 
\£c  +  fj,y+v  =  0  is  any  other  line  whatever,  these  functions  are  respectively, 
in  their  most  general  forms, 

A^x  +  B$  +  1        Xx  +  fjuy  +j/ 

'  +  **  A«x  +  B0y  +  1  '   A^i+B0y  +  l  ' 

wherein  X,  p,  v  are  arbitrary  constants. 

It  can  be  shewn  that  in  general  we  cannot  form  a  rational  function  of  the 
fifth  order  whose  only  infinity  is  at  the  place  of  osculation.  Thus  the  gaps 
indicated  by  Weierstrass's  theorem  occur  at  the  orders  1,  2,  5.  (Cf.  the 
concluding  remark  of  §  34.) 

In  case,  however,  the  place  a  be  an  ordinary  point  of  the  quartic,  the 
lowest  order  of  function,  whose  only  infinity  is  there,  is  p  +  1  =  4  :  it  will 
subsequently  become  clear  that  a  general  form  of  such  a  function  in  S'/S, 
where  S  =  0  is  any  conic  drawn  to  intersect  the  quartic  in  four  con 
secutive  points  at  a,  and  S'  =  0  is  the  most  general  conic  drawn  through 
the  other  four  intersections  of  S  with  the  quartic.  S'  will  in  fact  be  of  the 
form  \S  +  p,T,  where  T  is  any  definite  conic  satisfying  the  conditions  for  S', 
and  X,  /j,  are  arbitrary  constants;  the  equation  Q—  q=p  —  (r  +  1)  is  clearly 
satisfied  by  Q  =  4,  q  =  1,  p  =  3,  T  +  1  =  0. 

The  present  article  is  intended  only  by  way  of  illustration  ;  the  examples 
given  appear  to  find  their  proper  place  here.  The  reader  will  possibly 


38 


FUNCTION    OF   ORDEK 


[30 


find  it  desirable  to  read  them  in  connexion  with  the  geometrical  account 
given  in  Chapter  VI. 

31.     Consider  now  what  places  of  the  surfaces  are  such  that  we  can  form 
a  rational  function  infinite,  only  there,  to  an  order  as  low  as  p. 

For  such  a  place,  as  follows  from  §  28,  the  determinant 

A  = 


>    (r\    DP"1  O    (v\  T}P— !  O    ff\ 

4i  v*v>  ^    i£2vv> >-L/    ***v~y 

must  vanish.  Assume  for  the  present  that  none  of  the  minors  of  A  vanish 
at  that  place.  It  is  clear  by  §  28  that  A  only  vanishes  at  such  places  as  we 
are  considering. 

Let  v  be  any  integral  of  the  first  kind.     We  can  write 


/  \      dvi  .      ,      „         dv  dvi 
(x)  =  -j-  in  the  form  -=-  —  , 
at  at  av 


and  similarly  put 


and  so  write 


where  D  is  the  determinant  whose  rth  row  is  formed  with  the  quantities 


dvr  ' 


'   dvr 


Now  -T*  is  a  rational  function;  and  it  is  infinite  only  at  the  zeros  of  dv, 


whose  aggregate  number  is  2p  —  2;  and  -y-0*  is  a  rational  function   of  the 

(4>p  —  4)th  order,  its  poles  being  also  at  the  zeros  of  dv;  and  a  similar  state 
ment  can  be  made  in  regard  to  the  other  rows  of  D. 

Hence  D  is  a  rational  function  whose  infinities  are  of  aggregate  number 

(2p  -  2)  (1  +  2  +  ...  +p)  =  (p  -  l)p  (p  +  1), 
and  this  is  therefore  the  number  of  zeros  of  D. 


32]  EXISTS   ONLY    FOR  CERTAIN    PLACES.  39 

Now  A  can  vanish  either  by  the  vanishing  of  the  factor  D  or  by  the 

(dv\%p  (.P+I) 
—  I  The  zeros  of  the  last  factor  are,  however, 

dtj 

the  poles  of  D.  Hence  the  aggregate  number  of  zeros  of  A  is  (p  —  1)  p  (p  +  1). 
We  shall  see  immediately  that  these  zeros  do  not  necessarily  occur  at  as 
many  as  (p  —  I)p  (p  +  1)  distinct  places  of  the  surface. 

In  order  that  a  rational  function  should  exist  of  order  less  than  p,  its 
infinity  being  entirely  at  one  place,  say  of  order  p  —  r,  it  would  be  necessary 
that  the  r  determinants  formed  from  the  matrix  obtained  by  omitting  the 
last  r  rows  of  A  should  all  vanish  at  that  place.  We  can,  as  in  the  case  of 
A,  shew  that  each  of  these  minors  will  vanish  only  at  a  finite  number  of 
places.  It  is  therefore  to  be  expected  that  in  general  these  minors  will  not 
have  common  zeros  ;  that  is,  that  the  surface  will  need  to  be  one  whose 
3/;  —  3  moduli  are  connected  in  some  special  way. 

Moreover  it  is  not  in  general  true  that  a  rational  function  of  order  p  +  1 
exists  for  a  place  for  which  a  function  of  order  p  exists,  these  functions  not 
being  elsewhere  infinite.  For  then  we  could  simultaneously  satisfy  the  two 
sets  of  p  equations 

(a)  +  \DCli  (a)  +  ......  +  Xp^DP-2^  (a)  +  \pDf~1  Ot-  (a)  =  0, 

(a)  +  ^Dtli  (a)  +  ......  +  ffv-lDP-afli  (a)  +  /v,.,  jDPflf  (a)  =  0, 


namely,  A  and  -7-  would  both  be  zero  at  such  a  place.     The  condition  that 
at 

this  be  so  would  require  that  a   certain    function   of  the    moduli   of  the 
surface  —  what  we  may  call  an  absolute  invariant  —  should  be  zero. 

Therefore  when  of  the  p  gaps  required  by  Weierstrass's  theorem,  p  —  1 
occur  for  the  orders  1,  2,  ...,  p  —  1,  the  other  will  in  general  occur  for  the 
order  p+l.  The  reader  will  see  that  there  is  no  such  reason  why,  when  a 
function  of  order  p  exists,  a  function  of  order  p  +  2  or  higher  order  should 
not  exist. 

32.  The  reader  who  has  followed  the  example  of  §  30  will  recall  that  the 
number  of  inflexions  of  a  non-singular  plane  quartic*  is  24  which  is  equal  to 
the  value  of  (p  -  1)  p  (p  +  1)  when  p  =  3.  The  condition  that  the  quartic 
possess  a  point  of  osculation  is  that  a  certain  invariant  should  vanish^. 

When  the  curve  has  a  double  point,  there  are  only  two  integrals  of  the 
first  kind  J,  and  p  is  equal  to  two.  Thus  in  accordance  with  the  theory  above, 
there  should  be  (p  —  1)  p  (p  +  1)  =  6  places  for  which  we  can  form  functions 

*  Salmon,  Higher  Plane  Curves  (1879),  p.  213. 

t  The  equation  can  be  written  so  as  to  involve  only  5  =  3/>  -  3  -  1  parametric  constants 
(Chap.  V.  p.  98,  Exs.  1,  2). 

+  Their  forms  are  given  Chapter  II.  §  17  /3.  lleasons  are  given  in  Chapter  VI.  The  reader 
may  compare  Forsyth,  p.  395. 


40  EXAMPLES.  [32 

of  the  second  order  infinite  only  at  one  of  these  places.  In  fact  six  tangents 
can  be  drawn  to  the  curve  from  the  double  point  :  if  A^c  +  B9y  =  0  be  the 
equation  of  one  of  these  and  \  (Ax  +  By)  +  fi(A0x  +  B0y)  =  0  be  the  equation 
of  any  line  through  the  double  point,  the  ratio 

fc         Ax  +  By 
XA^  +  B0y  +  f* 

represents  a  function  of  second  order  infinite  only  at  the  point  of  contact  of 


For  the  point  of  contact  of  one  of  these  tangents  the^)  gaps  occur  for  the 
orders  1  and  3. 

The  quartic  with  a  double  point  can  be  biratioually  related  to  a  surface  expressed  by 
an  equation  of  the  form 


£  being  the  function  above.     The  reader  should  compare  the  theory  in  Chapter  I.  and  the 
section  on  the  hyperelliptic  case,  Chapter  V.  below. 

33.     Ex.    For  the  surface  represented  by  the  equation 


where  the  brackets  indicate  general  integral  polynomials  of  the  order  of  the  suffixes,  p  is 
equal  to  4,  and  the  general  integral  of  the  first  kind  is 


r 

where  f(y  )  =  +  .    Prove  that  at  the  (p  -  1  )  p  (p  +  1  )  =  60  places  for  which  rational  functions 
of  the  4th  order  exist,  infinite  only  at  these  places,  the  following  equations  are  satisfied 

2/7</-3(/'/y)2=o, 

2f  3  s3/  ff2  83/,3i 

>*  +  6  a^ap  fvfx  ~  ap  J*  J 


Where  y'='  etc-'^='  etc> 

Explain  how  to  express  these  functions  of  the  fourth  order. 
Enumerate  all  the  zeros  of  the  second  differential  expression  here  given. 

Ex.  2.  In  general,  the  corresponding  places  are  obtained  by  forming  the  differential 
equation  of  the  pth  order  of  all  adjoint  <f>  curves.  In  a  certain  sense  A  is  a  differential 
invariant,  for  all  reversible  rational  transformations.  (See  Chapter  VI.) 

*  Here  the  number  of  integrands  of  the  integrals  of  the  first  kind,  which  are  of  the  form 
(Lx  +  My)lf'(y)  (cf.  Chapter  III.  §  28),  which  vanish  in  two  consecutive  points  at  the  point  of 
contact  of  Avx  +  H0y  =  0,  is  clearly  1,  or  T  +  1  =  1  :  hence  the  formula  Q  -  q  -p  -  (r  +  1)  is  verified 
by  Q  =  2,  q  =  l,  p  =  2,  so  that  the  form  of  function  of  the  second  order  given  in  the  text  is  the 
most  general  possible. 


34] 


CONSIDERATION    OF   THESE    EXCEPTIONAL   PLACES, 


41 


34.     We  pass  now  to  consider  whether  the  (p  —  1)  p  (p  +  1)  zeros  of  A 
will  in  general  fall  at  separate  places*. 

Consider  the  determinant 

V  =     0     fl  (x}  fl  (x) 


wherein  flj^  ((?)=*  J5f Of  (£•),  and  k1}  ...,  kp  are  the  orders  of  non-existent 
rational  functions  for  a  place  £,  in  ascending  order  of  magnitude,  (A^  =  1) ; 
and  let  its  value  be  denoted  by 


so 


that  ur  =  I  (i>r  (x)  dtx  is  an  integral  of  the  first  kind. 

Then  wr(x)  vanishes  at  %  to  the  (kr  —  l)th  order. 
For  <w,.  (x)  is  the  determinant 

v.-r-i 


now  the  (kr  —  l)th  differential  coefficient  of  this  determinant  (in  regard  to 
the  infinitesimal  at  x)  has  at  £  a  value  which  is  in  fact  the  minor  of  the 
element  (1,  1)  of  V,  save  for  sign.  That  this  minor  does  not  vanish  is  part 
of  the  definition  of  the  numbers  k1}  k2,  ...,  kp.  But  all  differential  coeffi 
cients  of  Vr  of  lower  than  the  (kr  —  l)th  order  do  vanish  at  £:  some,  because 
for  a;  =  £  they  are  determinants  having  the  first  row  identical  with  one  of 
the  following  rows,  this  being  the  case  for  the  differential  coefficients  of 
orders  ^  —  1,  &2  —  1,  ...  ;  others,  because  when  /*  is  not  one  of  the  numbers 
fcj,  k2,  ...,  kp,  D^ifli^)  is  a  linear  function  of  those  of  Dk'~1Cli(^), 
Lb~* {li(g),  ...  for  which  p  is  greater  than  klf  k.2,  ...  ,  the  coefficients  of  the 
linear  functions  being  independent  of  i.  This  proves  the  proposition. 

It  is  clear  that  the  &rth  differential  coefficient  of  Vr  may  also  vanish  at  £. 
In  particular  Wi(x)  does  not  vanish  at  £:  a  result  in  accordance  with  a 
remark  previously  made  (Chapter  II.  §  21),  that  there  is  no  place  at  which 
the  differentials  of  all  the  integrals  of  the  first  kind  can  vanish. 

*  The  results  in  §§  34,  35,  36  are  given  by  Hunvitz,  Math.  Annul.  41,  p.  409.     They  will 
be  useful  subsequently. 


42  AND   OF   THE   NON-EXISTING-ORDERS.  [34 

An  important  corollary  is  that  the  highest  order  for  which  no  rational 
function  exists,  infinite  only  at  the  place  £,  is  less  than  2p.  For  wp  (x)  vanishes 
only  2p  —  2  times,  namely,  kp  —  1  <  2p  —  2. 

35.  We  can  now  prove  that  if  k2  >  2,  the  sum  of  the  orders  k\,  &2>  •••  ,  kp 
is  less  than  p2.  For  if  there  be  a  rational  function  of  order  in,  infinite  only 
at  £,  and  r  be  one  of  the  non-existent  orders*  ^  ...  kp,  r  —  m  is  also  one  of 
these  non-existent  orders — otherwise  the  product  of  the  existent  rational 
function  of  order  i —  m  with  the  function  of  order  m  would  be  an  existent 
function  of  order  r.  The  powers  of  the  function  of  order  m  are  existent 
functions,  hence  none  of  kl . . .  kp  are  divisible  by  in. 

Let  Ti  be  the  greatest  of  the  non-existent  orders  k^  ...  kp  which  is  con 
gruent  to  i(<  m)  for  the  modulus  m  :  then,  by  the  remark  just  made, 

TI,  Ti  —  in,  Ti  —  2m,  ... ,  m  +  i,  i 

are  all  non-existent  orders — and  all  congruent  to  i  for  the  modulus  m.     Since 
i'i  occurs  among  ki...kp,  all  these  also  occur.     Take  i  in  turn  equal  to 

1,    2,   ...   771-1. 

Then,  the  number  of  non-existent  orders  being  p, 

p  = 


so  that  T!  +  r2  +  . . .  +  rm_^  =  mp  —  \  m  (m  —  1) 

=  \  m(2p  —  m+  1). 

Now  the  sum  of  the  non-existent  orders  is 

m-l 

2   [ri  +  (n  -  m)  +  (n  -  2m)  +  ...  +  i]  , 
which  is  equal  to 


+  lm  (m  -  1)  -  TL  (in  -  1)  (2m  -  1), 
and,  since  Sr^  =  ^  m  (%p  —  m  +  1),  this  is  equal  to 

~  Sr,  [r,  -  (2p  -  1)]  +  I  [4p»  -  (m  -  Vf\  +  ^  (m  -  1)  (m  +  1), 
or  ^-r2-l-r-m-lm-2. 


*  i.e.  orders  of  rational  functions,  infinite  only  at  £,  which  do  not  exist:  and  similarly  in 
what  follows. 


36] 


LEAST   NUMBER   OF   THESE    EXCEPTIONAL    PLACES. 


Since,  by  the  corollary  of  the  preceding  article,  2p  —  1  is  not  less  than  riy 
this  is  less  than  p-  unless  m  is  1  or  2.  Now  m  cannot  be  equal  to  1  ;  and  if 
it  is  2  then  also  k2  >  2.  Hence  the  statement  made  at  the  beginning  of  the 
present  Article  is  justified. 

When  there  is  a  rational  function  of  order  2,  it  is  easy  to  prove  that 
there  are  places  for  which  L\  ...  kp  are  the  numbers  1,  3,  5,  ...  ,  2p  —  1,  whose 
sum*  is^>2.  An  example  is  furnished  by  §  32  above. 

Ex.     For  the  surface 


for  which  p  =  3,  there  is,  at  #=ao  ,  only  one  place,  and  the  non-existent  orders  are  1,  2,  5  : 
whose  sum  is  p*  —  l. 

36.     We  have  in  §  34  defined  p  integrals  of  the  first  kind 
I  wl(x)dtx,  ...  ,  I  wp(x)dtx 

by  means  of  a  place  £.  Since  the  differential  coefficients  of  these  vanish  at  £ 
to  essentially  different  orders,  these  integrals  cannot  be  connected  by  a  homo 
geneous  linear  equation  with  constant  coefficients.  Hence  a  linear  function 
of  them  with  parametric  constant  coefficients  is  a  general  integral  of  the  first 
kind.  Therefore  each  of  ^(x)  ...  O^  (x)  is  expressible  linearly  in  terms  of 
o>!  (x)  ...  wp  (x)  in  a  form 

&i  0)  =  Cn$r(»  +  .  .  .  +  Cip&p  (x}, 

where  the  coefficients  are  independent  of  x.  Thus  the  determinant  A  (§  31), 
which  vanishes  at  places  for  which  functions  of  order  less  than  p  +  1  exist,  is 
equal  to 

>i(x)         ,  ......  ,  <op(x) 

xwl(x)    ,  ......  ,  DXG>P(X) 


where  C  is  the  determinant  of  the  coefficients  c,-j.     It  follows  from  the  result 
of  §  34  that  the  determinant  here  multiplied  by  C  vanishes  at  £  to  the  order 


Thus,  the  determinant  A  vanishes  at  any  one  of  its  zeros  to  an  order  equal 
to  the  sum  of  the  non-existent  orders  for  the  place  diminished  by  %p(p  +  l). 

For  example,  it  vanishes  at  a  place  where  the  non-existent  orders  are 
1,  2,  ...  ,  p-  1,  p  +  1  to  an  order  $p(p-~L)+p  +  l-^p(p  +  l)  or  to  the 
first  order.  We  have  already  remarked  that  such  places  are  those  which 
most  usually  occur. 


*  Cf.  Burkhardt,  Math.  Annal.  32,  p.  388,  and  the  section  iu  Chapter  V.,  below,  on  the  hyper- 
elliptic  case. 


44  RIEMANN-ROCH   THEOREM.  [36 

Hence,  since  fa  -f  .  .  .  +  kp  ^  p2,  A  vanishes  at  one  of  its  zeros  to  an  order 


Further,  if  r  be  the  number  of  distinct  places  where  A  vanishes,  and 
mly  m2,  .  ..,  mr  be  the  orders  of  multiplicity  of  zero  at  these  places,  it  follows, 
from 


and  raa  +  ...  +  mr  <  r  %p(p  —  1), 

that  r  >  2p  +  2,  or 

there  are  at  least  2p  +  2  distinct  places  for  which  functions  of  less  order 
than  p  +  1,  infinite  only  thereat,  exist]  this  lower  limit  to  the  number  of 
distinct  places  is  only  reached  when  there  are  places  for  which  functions  of 
the  second  order  exist. 

Ex.     For  the  surface  given  by 


p  is  equal  to  3  ;  there  are  12  =  2^  +  6  distinct  places  where  A  vanishes. 

37.  We  have  called  attention  to  the  number  of  arbitrary  constants  con 
tained  in  the  most  general  rational  function  having  simple  poles  in  distinct 
places  (§  27)  and  to  the  number  in  the  most  general  function  infinite  at  a 
single  place  to  prescribed  order  (§  28)  :  in  this  enumeration  some  of  the  con 
stants  may  be  multipliers  of  functions  not  actually  becoming  infinite  in  the 
most  general  way  allowed  them,  that  is,  either  of  functions  which  are  not 
really  infinite  at  all  the  distinct  places  or  of  functions  whose  order  of  infinity 
is  not  so  high  as  the  prescribed  order. 

It  will  be  convenient  to  state  here  the  general  result,  the  deduction  of 
which  follows  immediately  from  the  expression  of  the  function  in  terms  of 
integrals  of  the  second  kind  :  — 

Let  tt1;  a.,,  ...  be  any  finite  number  of  places  on  the  surface,  the  infinitesi 
mals  at  these  places  being  denoted  by  tl}  t.2,  ....  The  most  general  rational 
function  whose  expansion  at  the  place  di  involves  the  terms 

JL      JL      _L 

&'  W  t*<'  '" 

—  whose  number  is  finite,  =  Q»  say,  —  and  no  other  negative  powers,  involves 
q  +  1  linearly  entering  arbitrary  constants,  of  which  one  is  additive,  q  being 
given  by  the  formula 

Q-q=P-(r  +  i), 

where  Q  is  the  sum  of  the  numbers  Q{,  and  r  +  1  is  the  number  of  linearly 
independent  linear  aggregates  of  the  form 

fl(a;)  =  A  A  (a;)  +  ...  +  ApQ,p(x\ 


37]  EXAMPLE.  45 

which  satisfy  the  sets  of  Qi  relations,  whose  total  number  is  Q,  given  by 
A,  DV-1  f^  (at)  +  A,D^  02  (ai)  +  .  .  .  +  ApD*--1  np  (tti)  =  0, 
Ail>-1  nt  (a;)  +  4a  J>  -i  n2  (a<)  +  .  .  .  +  ^I>  -1  Op  (a,-)  =  0, 


As  before,  this  general  function  will  as  a  rule  be  an  aggregate  of  functions 
of  which  not  every  one  is  as  fully  infinite  as  is  allowed,  and  it  is 
clear  from  the  present  chapter  that  in  the  absence  of  further  information  in 
regard  to  the  places  a1}  a.2,  ...  it  may  quite  well  happen  that  not  one  of  these 
functions  is  as  fully  infinite  as  desired,  the  conditions  analogous  to  those  stated 
in  §§  23,  28  not  being  satisfied.  See  Example  2  below. 

The  equation  Q  —  q=p  —  (r  +  l)  will  be  referred  to  as  the  Riemann-Roch 
Theorem. 

Ex.  1.  For  a  rational  function  having  only  simple  poles  or,  more  gene 
rally,  such  that  the  numbers  X;,  /^t-,  vi,  ...  for  any  pole  are  the  numbers 
1,  2,  3,  ...  Qit 

if  Q  >  2p  —  2,  r  +  1  is  zero,  since  fl  (x)  has  only  an  aggregate  number 
2p  —  2  of  zeros  :  the  function  involves  Q  —  p  +  1  constants, 

if  Q  =  2p  —  2,  r  +  1  cannot  be  greater  than  1  ;  for  the  ratio  of  two  of  the 
aggregates  £l(x)  then  vanishing  at  the  poles,  being  expressible  in  a  form 

dV 

_™  ,  where  V,  W  are  integrals  of  the  first  kind,  would  be  a  rational  function 

a  w 

without  poles,  namely  a  constant  ;  then  the  linear  aggregates  fl  (#)  would  be 
identical  :  thus  the  function  involves  Q  —  p  +  I  or  Q  —  p  +  2,  constants, 
namely  p  —  1  or  p  constants, 

if  Q=  2p  —  3,  T+  1  cannot  be  greater  than  1,  since  the  ratio  of  two  of 
the  aggregates  H  (x)  then  vanishing  at  the  poles  would  be  a  rational  function 
of  the  first  order  and  therefore  p  be  equal  to  unity  —  in  which  case  2p  —  3  is 
negative  :  thus  the  function  involves  p  —  2  or  p  —  1  constants, 

if  Q  =  2p  —  4,  and  T  +  1  be  greater  than  unity,  the  ratio  of  two  of  the 
vanishing  aggregates  fl  (#)  would  be  a  rational  function  of  the  second  order  : 
we  have  already  several  times  referred  to  this  possibility  as  indicative  that 
the  surface  is  of  a  special  character  —  called  hyperelliptic  —  and  depends  in 
fact  only  on  2p  —  1  independent  moduli.  In  general  such  a  function  would 
involve  p  —  3  constants. 

Ex.  2.  Let  V  be  an  integral  of  the  first  kind  and  a  be  an  arbitrary 
definite  place  which  is  not  among  the  2p  —  2  zeros  of  dV.  We  can  form  a 
rational  function  infinite  to  the  first  order  at  the  2p  —  2  zeros  of  dV  and  to 
the  second  order  at  a;  the  general  form  of  such  a  function  would  contain 
2j9  —  2  +  2—  p  +  I  =p  +  1  arbitrary  constants.  But  there  exists  no  rational 
function  infinite  to  the  first  order  at  the  zeros  of  dV  and  to  the  first  order  at 


46  IMPORTANT   EXAMPLE.  [37 

the  place  a.  Such  a  function  would  indeed  by  the  Riemann-Roch  theorem 
here  stated,  contain  2p  —  2  +  1—  p  -{•  l=p  arbitrary  constants  :  but  the  coeffi 
cients  of  these  constants  are  in  fact  infinite  only  at  the  zeros  of  d  V.  For  when 
the  places  a1}  ...  ,  0^-2  are  all  zeros  of  an  aggregate  of  the  form 

AA(a;)  +  ...+Apnp(ac), 
the  conditions  that  the  periods  of  an  expression 


be  all  zero,  namely  the  equations 

Xj  nt  (aO  +  .  .  .  +  \2p_2  fli  (oap-a)  +  fjLfli  (a)  =  0,   (i  =  1,  2,  .  .  .  ,  p), 
lead  to 

p,  [AfMa)  +  ...  +  Apflp(d)]  =  0, 

and  therefore  to  /JL  —  0. 

Thus  the  function  in  question  will  be  a  linear  aggregate  of  p  functions 
whose  poles  are  among  the  places  a1}  ...  ,  a^-s-  As  a  matter  of  fact,  if  W  be 
a  general  integral  of  the  first  kind,  expressible  therefore  in  the  form 

2F2  +  ...+\PVP, 


dW 

wherein   V2,  ...,  Vp  are  integrals  of  the  first  kind,    v^   involves  the  right 

a  v 

number  of  constants  and  is  the  function  sought. 

In  this  case  the  place  a  does  not,  in  the  sense  of  §  23,  depend  upon  the 
places  a1}  ...  ,  0^-2  j  ^ne  symbol  suggested  in  §  26  for  the  places  a1}  ...  ,  a^-a, 
a,  ...  is 


1,2,3,  .. .,^-1,^+1,  ...,2p-2,  2^-1,  2^,2^  +  1,.... 

It  may  be  shewn  quite  similarly  that  there  is  no  rational  function  having 
simple  poles  in  a1}  a2,  ... ,  a2p_2  and  infinite  besides  at  a  like  the  single 

term  —  ,  t  being  the  infinitesimal  at  the  place  a. 

v 

Ex.  3.  The  most  general  rational  function  R  which  has  the  value  c  at 
each  of  Q  given  distinct  places,  R  —  c  being  zero  of  the  first  order  at  each  of 
these  places,  is  obviously  derivable  by  the  remark  that  l/(R  —  c)  is  infinite  at 
these  places. 


38] 


CHAPTER    IV. 

SPECIFICATION  OF  A  GENERAL  FORM  OF  RIEMANN'S  INTEGRALS. 

38.  IN  the  present  chapter  the  problem  of  expressing  the  Riemann 
integrals  is  reduced  to  the  determination  of  certain  fundamental  rational 
functions,  called  integral  functions.  The  existence  of  these  functions,  and 
their  principal  properties,  is  obtained  from  the  descriptive  point  of  view 
natural  to  the  Riemann  theory. 

It  appears  that  these  integral  functions  are  intimately  related  to  certain 
functions,  the  differential-coefficients  of  the  integrals  of  the  first  kind,  of 
which  the  ratios  have  been  shewn  (Chapter  II.  §  21)  to  be  invariant  for 
birational  transformations  of  the  surface.  It  will  appear,  further,  in  the 
next  chapter,  that  when  these  integral  functions  are  given,  or,,  more  pre 
cisely,  when  the  equations  which  express  their  products,  of  pairs  of  them,  in 
terms  of  themselves,  are  given,  we  can  deduce  a  form  of  equation  to  re 
present  the  Riemann  surface  ;  thus  these  functions  may  be  regarded  as 
anterior  to  any  special  form  of  fundamental  equation. 

Conversely,  when  the  surface  is  given  by  a  particular  form  of  fundamental 
equation,  the  calculation  of  the  algebraic  forms  of  the  integral  functions  may 
be  a  problem  of  some  length.  A  method  by  which  it  can  be  carried  out  is 
given  in  Chapter  V.  (§§  72  ff.).  Compare  §  50  of  the  present  chapter. 

It  is  convenient  to  explain  beforehand  the  nature  of  the  difficulty  from  which  the 
theory  contained  in  §§  38  —  44  of  this  chapter  has  arisen.  Let  the  equation  associated 
with  a  given  Riemann  surface  be  written 


wherein  A,  A1,...,  An  are  integral  polynomials  in  x.  An  integral  function  is  one  whose 
poles  all  lie  at  the  places  .r=o>  of  the  surface;  in  this  chapter  the  integral  functions 
considered  are  all  rational  functions.  If  y  be  an  integral  function,  the  rational 
symmetric  functions  of  the  n  values  of  y  corresponding  to  any  value  of  .r,  whose 
values,  given  by  the  equation,  are  -AJA,  Ay/A,  -A^A,  etc.,  will  not  become  infinite 


48  RATIONAL   FUNCTIONS   WHOSE   POLES  [38 

for  any  finite  value  of  x,  and  will,  therefore,  be  integral  polynomials  in  x.    Thus  when 
y  is  an   integral  function,   the  polynomial  A   divides  all  the    other   polynomials    Alt 
A  2,  ......  ,  An.     Conversely,  when  A  divides  these  other  polynomials,  the  form   of  the 

equation  shews  that  y  cannot  become  infinite  for  any  finite  value  of  x,  and  is  therefore 
an  integral  function. 

When  y  is  not  an  integral  function,  we  can  always  find  an  integral  polynomial  in 
x,  say  /3,  vanishing  to  such  an  order  at  each  of  the  finite  poles  of  y,  that  /3y  is  an 
integral  function.  Then  also,  of  course,  |32/2,  /33y  3,  .  .  .  are  integral  functions:  though  it 
often  happens  that  there  is  a  polynomial  /32  of  less  order  than  /32,  such  that  /32y2  *s 
an  integral  function,  and  similarly  an  integral  polynomial  #3  of  less  order  than  /33, 
such  that  ft3y*  is  an  integral  function  ;  and  similarly  for  higher  powers  of  y. 

In  particular,  if  in  the  equation  given  we  put  Ay  =  rj,  the  equation  becomes 

r,n  +  AlT)n-l  +  A2Ar,n-2  +  ...  +  AnAn-l  =  0, 
and  T)  is  an  integral  function. 

Suppose  that  y  is  an  integral  function.  Then  any  rational  integral  polynomial  in 
x  and  y  is,  clearly,  also  an  integral  function.  But  it  does  not  follow,  conversely, 
though  it  is  sometimes  true,  that  every  integral  rational  function  can  be  written  as  an 
integral  polynomial  in  x  and  y.  For  instance  on  the  surface  associated  with  the 
equation 

f  +  Bfx  +  Cyx*  +  Dtf  -E(f-  A-2)  =  0  , 

the  three  values  of  y  at  the  places  .r  =  0  may  be  expressed  by  series  of  positive  integral 
powers  of  x  of  the  respective  forms 


,        y—  - 

Thus,  the  rational  function  (/•  —  Ey^x  is  not  infinite  when  #=0.  Since  y  is  an 
integral  function,  the  function  cannot  be  infinite  for  any  other  finite  value  of  x. 
Hence  (y2  -  Ey}jx  is  an  integral  function.  And  it  is  not  possible,  with  the  help  of  the 
equation  of  the  surface,  to  write  the  function  as  an  integral  polynomial  in  x  and  y. 
For  such  a  polynomial  could,  by  the  equation  of  the  surface,  be  reduced  to  the  form 
of  an  integral  polynomial  in  x  and  y  of  the  second  order  in  y  ;  and,  in  order  that  such 
a  polynomial  should  be  equal  to  (y^-Ey^lx,  the  original  equation  would  need  to  be 
reducible. 

Ex.  Find  the  rational  relation  connecting  x  with  the  function  77  =  (#2  —  Ey}jx  ;  and 
thus  shew  that  17  is  an  integral  function. 

39.  We  concern  ourselves  first  of  all  with  a  method  of  expressing  all 
rational  functions  whose  poles  are  only  at  the  places  where  x  has  the  same 
finite  value.  For  this  value,  say  a,  of  x  there  may  be  several  branch  places  : 
the  most  general  case  is  when  there  are  k  places  specified  by  such  equations  as 

x  -  a  =  £ri+1,  •  •  •  ,  x-  a  =  tkwk+\ 

The  orders  of  infinity,  in  these  places,  of  the  functions  considered,  will  be 
specified  by  integral  negative  powers  of  tlf  .  ..,  tk  respectively.  Let  F  be 
such  a  function.  Let  o-  +  1  be  the  least  positive  integer  such  that  (x  —  aY+lF 
is  finite  at  every  place  x  =  a.  We  call  <r  +  1  the  dimension  of  F.  Let 
f(xt  y)  =  0  be  the  equation  of  the  surface.  In  order  that  there  may  be  any 
branch  places  at  x  =  a,  it  is  necessary  that  df/dy  should  be  zero  for  this  value 


39]  ARISE    FOR   THE   SAME   VALUE   OF   X.  49 

of  x.  Since  this  is  only  true  for  a  finite  number  of  values  of  x,  we  shall  suppose 
that  the  value  of  x  considered  is  one  for  which  there  are  no  branch  places. 

We  prove  that  there  are  rational  functions  h1}  ...,  hn^  infinite  only  at 
the  n  places  x  =  a,  such  that  every  rational  function  whose  infinities  occur 
only  at  these  n  places  can  be  expressed  in  the  form 

(—     >  l]   +(—      >  l)    h+.  ..+(-?—  ,  l]       hn.  ..(A), 

\ao  -a      J\     \x-a'     A,  \x  -  a'     Jx^ 

in  such  a  way  that  no  term  occurs  in  this  expression  which  is  of  higher 
dimension  than  the  function  to  be  expressed  :  namely,  if  a  +  1  be  the  dimen 
sion  of  the  function  to  be  expressed  and  o-;  +  1  the  dimension  of  hi,  the 
function  can  be  expressed  in  such  a  way  that  no  one  of  the  integers 

X,  AX  +  al  +  1,  .  .  .  ,  A,^  +  a-n^  +  1 

is  greater  than  cr  +  1.  We  may  refer  to  this  characteristic  as  the  condition 
of  dimensions.  It  is  clear  conversely  that  every  expression  of  the  form  (A) 
will  be  a  rational  function  infinite  only  for  x  =  a. 

Let  the  sheets  of  the  surface  at  x  =  a  be  considered  in  some  definite 
order.  A  rational  function  which  is  infinite  only  at  these  n  places  may  be 
denoted  by  a  symbol  (R1}  R2>  ...  ,  Rn),  where  R1}  R2,  ...  ,  Rn  are  the  orders  of 
infinity  in  the  various  sheets.  We  may  call  Rlf  R2,  ...  ,  Rn  the  indices  of  the 
function.  Since  the  surface  is  unbranched  at  x  —  a,  it  is  possible  to  find  a 

certain  polynomial  in  -     -  ,  involving  only  positive  integral  powers  of  this 

SO  ^~  CL 

1      \  72 

quantity,  the  highest  power  being  [-     -)     ,  such  that  the  function 

\x  —  a  i 


l),  =  (£,$,,  ...,,SU,0)say  .........  (i), 

'•" 


—  a. 
is  not  infinite  in  the  nth  sheet  at  a;  =  a. 

Consider  then  all  rational  functions,  infinite  only  at  x  =  a,  of  which  the 
nth  index  is  zero.  It  is  in  general  possible  to  construct  a  rational  function 
having  prescribed  values  for  the  (n  -  1)  other  indices,  provided  their  sum  be 
p  +  1.  When  this  is  not  possible  a  function  can  be  constructed*  whose  indices 
have  a  less  sum  than  p  +  1,  none  of  them  being  greater  than  the  prescribed 
values.  Starting  with  a  set  of  indices  (p  +  1,  0,  ...  ,  0),  consider  how  far  the 
first  index  can  be  reduced  by  increasing  the  2nd,  3rd,  ...  ,  (n  -  l)th  indices. 
In  constructing  the  successive  functions  with  smaller  first  index,  it  will  be 
necessary,  in  the  most  general  case,  to  increase  some  of  the  2nd,  3rd,  ..., 
(n  —  l)th  indices,  and  there  will  be  a  certain  arbitrariness  as  to  the  way  in 
which  this  shall  be  done.  But  if  we  consider  only  those  functions  of  which 
the  sum  of  the  indices  is  less  than  p  +  2,  there  will  be  only  a  finite  number 

*  The  proof  is  given  in  the  preceding  Chapter,  (§§  24,  28). 
B.  4 


50  SPECIFICATION  [39 

possible  for  which  the  first  index  has  a  given  value.  There  will  therefore 
only  be  a  finite  number  of  functions  of  the  kind  considered*,  for  which  the 
further  condition  is  satisfied  that  the  first  index  is  the  least  possible  such  that 
it  is  not  less  than  any  of  the  others.  Let  this  least  value  be  r1}  and  suppose 
there  are  ^  functions  satisfying  this  condition.  Call  them  the  reduced 
functions  of  the  first  class — and  in  general  let  any  function  whose  nth  index 
is  zero  be  said  to  be  of  the  first  class  when  its  first  index  is  greater  or  not 
less  than  its  other  indices.  In  the  same  way  reckon  as  functions  of  the 
second  class  all  those  (with  nth  index  zero)  whose  second  index  is  greater 
than  the  first  index  and  greater  than  or  equal  to  the  following  indices.  Let 
the  functions  whose  second  index  has  the  least  value  consistently  with  this 
condition  be  called  the  reduced  functions  of  the  second  class ;  let  their 
number  be  k2  and  their  second  index  be  r2.  In  general,  reckon  to  the  ith 
class  (i  <  n)  all  those  functions,  with  nth  index  zero,  whose  t'th  index  is 
greater  than  the  preceding  indices  and  not  less  than  the  succeeding  indices. 
Let  there  be  ki  reduced  functions  of  this  class,  with  iih  index  equal  to  i\. 
Clearly  none  of  the  integers  t\,  ... ,  rn_j  are  zero. 

Let  now  (^  ...  s;_!  r{Si+1  ...  sn_i  0), 

where  r{  >slt  ... ,  i\  >  st-_,,  n  >  si+l,  ... ,  n  >  sn-i, 

be  any  definite  one  of  the  ki  reduced  functions  of  the  iih  class.  Make  a 
similar  selection  from  the  reduced  functions  of  every  class.  And  let 

($!  . . .  $£_!  R{  Si+l  . . .  Sn-i  0) 
be  any  function  of  the  iih  class  other  than  a  reduced  function,  so  that 

Ri  > Si,  ... ,  Ri>  Si-i,  Ri >  Si+1 ,  . . . ,  Ri  > Sn-i- 
Then  by  choice  of  a  proper  constant  coefficient  X  we  can  write 

(&  . . .  £<_!  Ri  Si+i . . .  Sn_!  0)  -  X  (x  -  a)~(Ri~Ti)  (sl . . .  «;_!  n si+l . . .  sn_!  0) 

in  the  form 

(^...T^R/T^-.-Tn^Ri-ri) (ii), 

where  R{  <  Ri',  2\  may  be  as  great  as  the  greater  of  S1}  Ri  —  (n -  s^,  but  is 
certainly  less  than  Ri]  and  similarly  T2,  ... ,  T^  are  certainly  less  than  Rt', 
while  T{+1  may  be  as  great  as  the  greater  of  $f+1,  Ri  —  (rt  —  si+l),  and  is  there 
fore  not  greater  than  R^,  and  similarly  Ti+2, ... ,  Tn^  are  certainly  not  greater 
than  Ri. 

*  Functions  which  have  the  same  indices  are  here  regarded  as  identical.  Of  course  the 
general  function  with  given  indices  may  involve  a  certain  number  of  arbitrary  constants.  By  the 
function  of  given  indices  is  here  meant  any  one  such,  chosen  at  pleasure,  which  really  becomes 
infinite  in  the  specified  way. 


39] 


OF   A    FUNDAMENTAL   SYSTEM. 


51 


Further,  if 


,  1 


be  a  suitable  polynomial  of  order  Ri  —  r\  in 
1 


\.x  —  a 
(x  —  a)~l,  we  can  write 

\iv  —  a        /  tii-Vi 

/<y          a/        -p>>    a'  &'       r\\  (\\\\ 

—  (/o  i  ...  io  i—i  £L  i  ij  i+i  ...  ij  n_i  \}) V111^' 

where  R"i  may  be  as  great  as  the  greater  of  R'{,  R{  —  rit  but  is  certainly  less 
than  Ri;  S\  may  be  as  great  as  the  greater  of  1\,  Ri  —  r{,  but  is  certainly  less 
than  Ri;  and  similarly $'2,  ...,  $';_!  are  certainly  less  than  R^;  while  S'i+l 
may  be  as  great  as  the  greater  of  7\-+1,  Ri—ri,  and  is  certainly  not  greater 
than  RI\  and  similarly  S'i+2,  ... ,  S'n-\  are  certainly  not  greater  than  Rt. 

Hence  there  are  two  possibilities. 

(1)  Either   (S\  . . .  £'f_i  R"i  S'i+1 . . .  £'n_i  0)    is   still  of  the  ith   class, 
namely,  R"i  >  Slf  ... ,  R"i  >  S'i^ ,  R"i  >  S'i+1 ,  . . . ,  R"t  >  £'„_, , 

and  in  this  case  the  greatest  value  occurring  among  its  indices  (R"i)  is  less 
than  the  greatest  value  occurring  in  the  indices  of  (Si...  Si-i  Ri  Si+1 . . .  $n_j  0). 

(2)  Or  it  is  a  function  of  another  class,  for  which  the  greatest  value 
occurring  among  its  indices  may  be  smaller  than  or  as  great  as  Rt  (though 
not  greater) ;  but  when  this  greatest  value  is  Ri,  it  is  not  reached  by  any  of 
the  first  i  indices. 

If  then,  using  a  term  already  employed,  the  greatest  value  occurring 
among  the  indices  of  any  function  (Ri,  ...,  Rn)  be  called  the  dimension  of 
the  function,  we  can  group  the  possibilities  differently  and  say,  either 

(S\  . . .  S'i^i  R"i  S'i+i  . . .  S'n-i  0)  is  of  lower  dimension  than 

(Si  ...  Si-i  Ri  Si+1  . . .  Sn-i  0), 

or  it  is  of  the  same  dimension  and  then  belongs  to  a  more  advanced  class, 
that  is,  to  an  (i  +  &)th  class  where  k  >  0. 

In  the  same  way  if  (^  ...  ^  r{  ti+i  . . .  tn-i  0)  be  any  reduced  function  of 
the  t'th  class  other  than  (^  ...  st-_i  rf  si+1  . . .  sn^  0),  we  can,  by  choice  of  a 
suitable  constant  coefficient  p,,  write 

(t-L  ...  ti—iTi  t-+  ...  t  —  0)  —  /x (s  ...  s-_  r-s-         s      0) 

where  r'i<ri,  t\...  £';_i  may  be  respectively  as  great  as  the  greater  of  the 
pairs  (ti,  s^  ...  (^_j,  Si_i)  but  are  each  certainly  less  than  rit  while  similarly 
no  one  of  t'i+1,  ...  ,  t'n-i  is  greater  than  rt. 

The  function  (t\  ...  t'^i  r{  tft+1  ...  £'n_i  0)  cannot  be  of  the  ith  class,  since 
no  function  of  the  tth  class  has  its  tth  index  less  than  rt :  and  though  the 
greatest  value  reached  among  its  indices  may  be  as  great  as  rt  (and  not 
greater),  the  number  of  indices  reaching  this  value  will  be  at  least  one  less 

4—2 


52  EXAMPLE  [39 

than  for  (s1 . . .  s;_j  rt  si+1 . . .  sn^  0).  Namely  (t\  . . .  JV-i  r'i  t'i+l . . .  t'n^  0)  is 
certainly  of  more  advanced  class  than  (si  . . .  £;_!  Vi  Si+1 . . .  sn^  0),  and  not  of 
higher  dimension  than  this. 

Denote  now  by  hlt  ... ,  hn^  the  selected  reduced  functions  of  the  1st, 
2nd,  ...,  (n  —  l)th  classes.  Then,  having  regard  to  the  equations  given  by 
(ii),  (iii),  (iv),  we  can  make  the  statement, 

Any  function  (Sl...  $;_j  Rt  Si+l ...  $n_j  0)  can  be  expressed  as  a  sum  of  (I) 
an  integral  polynomial  in  (x  —  a)~l,  (2)  one  ofhly  ... ,  An_j  multiplied  by  such 
a  polynomial,  (3)  a  function  F  which  is  either  of  lower  dimension  than  the 
function  to  be  expressed  or  is  of  more  advanced  class. 

In  particular  when  the  function  to  be  expressed  is  of  the  (n  —  l)th  class 
the  new  function  F  will  necessarily  be  of  lower  dimension  than  the  function 
to  be  expressed. 

Hence  by  continuing  the  process  as  far  as  may  be  needful,  every  function 

f=(S1...  Si-!  Ri  Si+1 . . .  Sn-i  0) 
can  be  expressed  in  the  form 

(—  ,  l]    +  (—  ,  l)    h*. ..  +  (—,  l]       hn^+F,, (v) 

Ve-a       A      U-a'     AI  \ac-a'     An_, 

where  F^  is  of  lower  dimension  thany! 

Applying  this  statement  and  recalling  that  there  are  lower  limits  to  the 
dimensions  of  existent  functions  of  the  various  classes,  namely,  those  of  the 
&!  +  . . .  +  kn-!  reduced  functions,  and  noticing  that  the  reduction  formula  (v) 
can  be  applied  to  these  reduced  functions,  we  can,  therefore,  put  every  func 
tion  f=(S1...  Si-! Ri Si+l . . .  Sn-i 0)  into  a  form 

f—    ,     l)      +  (—    ,     l)        hl+...   +   (—    ,     l)  hn-!. 

\at-a       J\      \x-a       /\l  \x-a       /x^ 

Now  it  is  to  be  noticed  that  in  the  equations  (ii),  (iii),  (iv),  upon  which 
this  result  is  based,  no  terms  are  introduced  which  are  of  higher  dimension 
than  the  function  which  it  is  desired  to  express :  and  that  the  same  remark 
is  applicable  to  equation  (i). 

Hence  every  function  (R1}  ... ,  Rn)  can  be  written  in  the  form  (A)  in  such  a 
way  that  the  condition  of  dimensions  is  satisfied. 

40.  In  order  to  give  an  immediate  example  of  the  theory  we  may  take 
the  case  of  a  surface  of  four  sheets,  and  assume  that  the  places  x  =  a  are  such 
that  no  rational  function  exists,  infinite  only  there,  whose  aggregate  order  of 
infinity  is  less  than  p  +  1.  In  that  case  the  specification  of  the  reduced 
functions  is  an  easy  arithmetical  problem.  The  reduced  functions  of  the  first 
class  are  (m1}  w2,  m3,  0),  where  mx  is  to  be  as  small  as  possible  without  being 
smaller  than  m2  or  w3 :  by  the  hypothesis  we  may  take 

Wj  +  m3  +  m3  =  p  +  I. 


40] 


OF  THE   FUNDAMENTAL   SYSTEM. 


53 


Those  of  the  second  class  require  m2  as  small  as  possible  subject  to 
ml  +  w2  +  ra3  =  p  +  1,  m2>ml,  ra2  >  w3 : 

those  of  the  third  class  require  w3  greater  than  m1  and  w2  but  otherwise  as 
small  as  possible  subject  to  n^  +  m2  +  ws  =  p  +  1.  We  therefore  immediately 
obtain  the  reduced  functions  given  in  the  2nd,  3rd  and  4th  columns  of  the 
following  table.  The  dimension  of  any  function  of  the  t'th  class  being  denoted 
by  <Ti  +  1,  the  values  of  <rt-  are  given  in  the  fifth  column,  and  the  sum 
ar1  +  a~2  +  0-3  in  the  sixth.  The  reason  for  the  insertion  of  this  value  will 
appear  in  the  next  Article. 


P 

Reduced  functions  of 
the  first  class 

Reduced  functions  of 
the  second  class 

Reduced  functions  of 
the  third  class 

°"l>    ff-2>  ff3 

ff1  +  ff.2  +  ffx 

=  3H-1 

(M,  M,  M,  0) 

(M-2,  M+l,  M  +  l,  0) 
(M-l,  M+1,M,  0) 
(M,  M+l,  M-l,  0) 

(M-l,  M,  M+l,  0) 

M-1,M,  M 

3M-1 

=  3N-2 

(N,N,N-1,0) 
(N,N-1,N,0) 

(N-l,  N,  N,  0) 

(N-I,N-1,N  +  1,0) 

N-1,N-1,N 

3^-2 

=  3P 

(P+l,  P,  P,  0) 
(P  +  1,P  +  1,P-1,0) 
(P+1,P-1,P  +  1,0) 

(P-l,  P  +  l,  P  +  l,  0) 
(P,  P  +  l,  P,  0) 

(P,  P,  P  +  l,  0) 

P,  P,  P 

3P 

Here  the  reduced  functions  of  the  various  classes  are  written  down  in 
random  order.  Denoting  those  first  written  by  h1}  h2,  h3,  we  may  exemplify 
the  way  in  which  the  others  are  expressible  by  them  in  two  cases. 

(a)  When  p  =  3M  —  1,  we  have,  /*  being  such  a  constant  as  in  equa 
tion  (iv)  above  (§  39), 

(M,  M  +  1,  M- 1,  0)  -fi(M-  2,  M  + 1,  M  + 1,  0)=  {M,  M,  M  +  1,  0}, 

the  right  hand  denoting  a  function  whose  orders  of  infinity  in  the  various 
sheets  are  not  higher  than  the  indices  given.  If  the  order  in  the  third  sheet 
be  less  than  M  +  1,  the  right  hand  must  be  a  function  of  the  first  class  and 
therefore  the  order  in  the  third  sheet  must  be  M.  In  that  case,  since  a 
general  function  of  aggregate  order  p  +  1  contains  two  arbitrary  constants, 
we  have  an  expression  of  the  form 

(M,  M  +  1,  M  -  1,  0)  =  fjih,  +  Ah,  +  B, 
for  suitable  values  of  the  constants  A,  B. 


If  however  there  be  no  such  reduction,  we  can  choose  a  constant  \  so 


that 


{M,  M,  M  +  I,  0}  -  \(M-  1,  M,  M+l,  0)  =  {M,  M,  M,  0}  =  A'h,  -f 


54  SUM   OF   DIMENSIONS   OF   FUNDAMENTAL   SYSTEM 

and  thus  obtain  on  the  whole 

(M,M+1,M-  1,  0)  =  fJis  +  \h3  +  A'h,  +  B', 
for  suitable  values  of  the  constants  A',  B'. 
(b)     When  p  =  3P  we  obtain 

(P  +  1,  P  +  1,  P  -  1,  0)  -  \k,  +  A(P,P  +  1,P,0)  +  B 
=  \h1  +  A  \fiht  +  Ch3  +  D}+B. 

Ex.  1.     Shew  for  a  surface  of  three  sheets  that  we  have  the  table 


[40 


p 

*Ii   h2 

o-i.  0-2 

(Tj  +  O-2 

odd 

/p  +  l    p  +  i       \    /p-i    ^  +  3       \ 

p-1    p  +  l 

V    2    '       2     '     )  \    2    '      2    '     ) 
(p  +  2    p       \  fp    p  +  2       \ 

2    '       2 

\    2    '   2'     /  \2'       2    '     / 

2'   2 

* 

2£c.  2.  Shew,  for  a  surface  of  n  sheets,  that  if  the  places  x  =  a  be  such  that  it  is 
impossible  to  construct  a  rational  function,  infinite  only  there,  whose  aggregate  order  of 
infinity  is  less  than  _£>  +  !,  a  set  of  reduced  functions  is  given  by 

kP.Jtr+l'-(k,..Jk,t-l,..^k-l,<)\(k-ltkt.JLtk-l+.^-l,Q)  ......  (k-l,...,k-  !,£,...£,(>) 

/<r  +  2..  A-i  =  (£-  1,  ...,k-l,k  +  l,  k,  ...k,  G)(k-I,  ...,  £-1,  k,k  +  l,  k,  ...A,  0)  ...... 

(k-l,  ...,k-l,k,  ...k,k+l,  0) 

wherein  p  +  I  =  (n—l)k  —  r  (r<»—  1)  and,  in  the  first  row,  there  are  r  numbers  ^  —  1  in 
each  symbol,  and,  in  the  second  row,  there  are  r+l  numbers  k—\  in  each  symbol.  In 
each  case  k,  ...k  denotes  a  set  of  numbers  all  equal  to  k  and  £—1,  ...,  £—1  denotes  a  set  of 
numbers  all  equal  to  k  —  1. 

The  values  of  crj,  ...,  cr,.  +  1  are  each  k  —  l,  those  of  o-,.  +  2»  •••>  «"n-i  are  each  ^-     Hence 
0-J+.  ..  +o>  +  !  +  o-r  +  2+.  .  .+<rn_1  =  (r  +  !)(&-  l)  +  (n-r-  2)  A  =  (n-l)*-r-  1  =^?. 

^!r.  3.  Shew  that  the  resulting  set  of  reduced  functions  is  effectively  independent  of 
the  order  in  which  the  sheets  are  supposed  to  be  arranged  at  x=a. 

41.  For  the  case  where  rational  functions  exist,  infinite  only  at  the  places 
x  =  a,  whose  aggregate  order  of  infinity  is  less  than  ^  +  1,  the  specification 
of  their  indices  is  a  matter  of  greater  complexity. 

But  we  can  at  once  prove  that  the  property  already  exemplified  and 
expressed  by  the  equation  o-1  +  ...  +  <rn_^  =  p,  or  by  the  statement  that  the  sum 
of  the  dimensions  of  the  reduced  functions  is  p  +  n  —  1,  is  true  in  all  cases. 

For  consider  a  rational  function  which  is  infinite  to  the  rth  order  in  each 
sheet  at  x  —  a  and  not  elsewhere  :  if  r  be  taken  great  enough,  such  a  function 
necessarily  exists  and  is  an  aggregate  of  nr  —  p  +  1  terms,  one  of  these  being 
an  additive  constant  (Chapter  III.  §  37).  By  what  has  been  proved,  such  a 
function  can  be  expressed  in  the  form 


-  a 


, 


x  -  a 


,,_, 


42]  EXPRESSED   BY   THE   DEFICIENCY   OF   THE   SURFACE.  55 

where  the  dimensions  of  the  several  terms,  namely  the  numbers 

X,   Xj  +  (T}  +  1 ,    . . .  ,   Xn_!  +  0"n-l  +    1 , 

are  not  greater  than  the  dimension,  r,  of  the  function. 

Conversely*,  the  most  general  expression  of  this  form  in  which  X^X^  ..., 
Xn_!  attain  the  upper  limits  prescribed  by  these  conditions,  is  a  function  of  the 
desired  kind. 

But  such  general  expression  contains 

(X  +  1)  +  (Xj  +  1)  +  ...  +  (Xn-,  +  1), 

that  is  (r  +  1)  +  (r  -  O  +  . . .  +  (r  -  cr,^), 

or  nr  —  (a1+...+  o^)  +  1 

arbitrary  constants. 

Since  this  must  be  equal  to  nr  —p+  1  the  result  enunciated  is  proved. 

The  result  is  of  considerable  interest — when  the  forms  of  the  functions  hl...hn-l  are 
determined  algebraically,  we  obtain  the  deficiency  of  the  surface  by  finding  the  sum  of  the 
dimensions  of  //x. . ,hn _  l .  It  is  clear  that  a  proof  of  the  value  of  this  sum  can  be  obtained  by 
considerations  already  adopted  to  prove  Weierstrass's  gap  theorem.  That  theorem  and 
the  present  result  are  in  fact,  here,  both  deduced  from  the  same  fact,  namely,  that  the 
number  of  periods  of  a  normal  integral  of  the  second  kind  is  p. 

42.     Consider  now  the  places  x  =  oo  :  let  the  character  of  the  surface  be 
specified  by  k  equations 

_—fWi  +  l  —  fWk+l 

—  »l          » •  ••  i       —  "k    k      > 

X  X 

there  being  k  branch  places.  A  rational  function  g  which  is  infinite  only 
at  these  places  will  be  called  an  integral  function.  If  its  orders  of  infinity 
at  these  places  be  respectively  rlt  r.2,...,  rk  and  G  [n-/(Wi+l)J  be  the  least 
positive  integer  greater  than  or  equal  to  ^/(w;  +  1),  and  p  +  1  denote  the 
greatest  of  the  k  integers  thus  obtained,  then  it  is  clear  that  p  +  1  is  the 
least  positive  integer  such  that  or*^1'  g  is  finite  at  every  place  x  =  oo .  We 
shall  call  p  +  1  the  dimension  of  g. 

Of  such  integral  functions  there  are  n  —  1  which  we  consider  particularly, 
namely,  using  the  notation  of  the  previous  paragraph,  the  functions 

(x  -  a)^+l  hlt ,(x-  a)°n-i+1  hn^ , 

which  by  the  definitions  of  a-1} ,  o-n_!  are  all  finite  at  the  places  x  =  a, 

and  are  therefore  infinite  only  for  x  =  oo  .  Denote  (x  —  a)0^"1"1  hi  by  </;.  If  hi 
do  not  vanish  at  every  place  x  =  oo ,  it  is  clear  that  the  dimension  of  <ft  is 

*  It  is  clear  that  this  statement  could  not  be  made  if  any  of  the  indices  of  the  function  to  be 
expressed  were  less  than  the  dimension  of  the  function.  For  instance  in  the  final  equation  of 
§  40  (a),  unless  /t,  X,  A'  be  specially  chosen,  the  right  hand  represents  a  function  with  its  third 
index  equal  to 


56  PARTICULAR   CASE   OF   INTEGRAL   FUNCTIONS.  [42 

o-j  +  1.  If  however  hi  do  so  vanish,  the  dim'ension  of  gi  may  conceivably  be 
less  than  o-^  +  l;  denote  it  by  pi  4  1,  so  that  pi  <  a-^  Then  x~(?i+v  gi}  and 
therefore  also  (x  —  a)~(pi+l]gi)  =  (x  —  aYi~i>ihi,  is  finite  at  all  places  #=oo  : 
hence  (#  —  a)'Y~pi  /^  is  a  function  which  only  becomes  infinite  at  the  places 
x  =  a.  But,  in  the  phraseology  of  §  39,  it  is  clearly  a  function  of  the  same 
class  as  hi,  it  does  not  become  infinite  in  the  nth  sheet  at  x  =  a,  and  is  of 
less  dimension  than  hi  if  a^  >  p^  That  such  a  function  should  exist  is 
contrary  to  the  definition  of  hi.  Hence,  in  fact,  o\-  =  p^.  The  reader  will 
see  that  the  same  result  is  proved  independently  in  the  course  of  the  present 
paragraph. 

Let  now  F  denote  any  integral  function  of  dimension  p  4  1.  Then 
#-(P+I)  F  [s  finite  at  all  places  x  =  oo  :  and  therefore  so  also  is  (x  —  a)~(p+1}  F. 
This  latter  function  is  one  of  those  which  are  infinite  only  at  places  x  =  a  ;  if 
F  do  not  vanish  at  all  places  x=a,  the  dimension  cr  +  1  of  (x  —  a)~(p+1)  F 
will  be  p  +  1  :  in  general  we  shall  have  a-  <  p. 

By  §  39  we  can  write 


x-a      /Al  \x-a 

where  cr  -f  1  >  Xi  +  o-^  +  1, 

and  therefore,  a  fortiori, 

p  +  1  >  \  +  <Ti  +  1   >  \i  +  pi  +  1. 

Hence  we  can  also  write 

F=  (1,  a;  -  a)x  O  -  a)'-*  +  (!,«-  a)Al  (*  -  a)"-A^'  &  4  ...... 

4  (1,  a?  -  a)An-x  («  -  a)"-A»-r%-i  ^^j, 
or  say 

^=(1,^4(1,^,0!  4  ......  +  (l,«U-i0n-i,  ............  (B) 

where  /Ai4pi  4  1  =/)  -cr.  +  p^4  1  =p  +  1  -(^  -  pf)  <p  +  1, 

namely,  there  is  no  term  on  the  right  whose  dimension  is  greater  than  that 
of  F  (and  each  of  /-i,  p,lt  ......  ,  fin_1  is  a  positive  integer). 

Hence    the    equation   (B)   is    entirely   analogous   to   the   equation   (A) 
obtained  previously  for  the  expression  of  functions  which  are  infinite  only 
at  places  x  =  a.     The  set  (1,  glf  ......  ,  gn-i)  will  be  called  a  fundamental  set 

for  the  expression  of  rational  integral  functions*. 

It  can  be  proved  precisely  as  in  the  previous  Article  that  p1  4  p2  4  ...... 

4  pn-\  =  P-     For  this  purpose  it  is  only  necessary  to  consider  a  function 

*  The  idea,  derived  from  arithmetic,  of  making  the  integral  functions  the  basis  of  the  theory 
of  all  algebraic  functions  has  been  utilised  by  Dedekind  and  Weber,  Theor.  d.  alg.  Funct.  e. 
Verdnd.  Crelle,  t.  92.  Kronecker,  U.  die  Discrim.  alg.  Fctnen.  Crelle,  t.  91.  Kronecker,  Grundziige 
e.  arith.  Theor.  d.  algebr.  Grossen,  Crelle,  t.  92  (1882). 


43]  GENERAL    PROPERTIES   OF   FUNDAMENTAL    SYSTEMS.  57 

which  is  infinite  at  the  places  #=oc  respectively  to  orders  r  (Wj  +  1),  ..., 
r  (wk  +  1).  And  the  equations  Sp  =  Scr  =  p,  taken  with  <7f  >  pit  suffice  to  shew 
that  a-i  =  pt.  It  can  also  be  shewn  that  from  the  set  gl  .  .  .  gn^  we  can 
conversely  deduce  a  fundamental  set  1,  (x  —  6)~(pi+1)  <ft,  ...,(x  —  b)~lpn-rl}  gn-i 
for  the  expression  of  functions  infinite  only  at  places  x=b;  these  have  the 
same  dimensions  as  1,  (ft,  ...,  gn-i*- 

43.  Having  thus  established  the  existence  of  fundamental  systems  for 
integral  rational  functions,  it  is  proper  to  refer  to  some  characteristic  pro 
perties  of  all  such  systems. 

(a)  If  Gl  ...  Gn-:  be  any  set  of  rational  integral  functions  such  that 
every  rational  integral  function  can  be  expressed  in  the  form 

(x,  l\  +  (x,  l\  £x+  ......  +  0,  1)AB_1  Gn-,  ...............  (C), 

there  can  exist  no  relations  of  the  form 

(X)  iv  +  (*,  IV,  0i  +  ......  +  (x,  i  V^  £„_!  =  o. 

For  if  k  such  relations  hold,  independent  of  one  another,  k  of  the  functions 
(TJ  ...  6rn_i  can  be  expressed  linearly,  with  coefficients  which  are  rational 
in  x,  in  terms  of  the  other  n  —  1  —  k.  Hence  also  {3$,  (32y2,.  .  .  ,  (3n-i-k  yn~l~k, 
@n-kyn~k>  which  are  integral  functions  when  &,...,$„_*  are  proper  poly 
nomials  in  x,  can  be  expressed  linearly  in  terms  of  the  n—  1—  k  linearly 
independent  functions  occurring  among  Gi...Gn-i,  with  coefficients  which 
are  rational  in  x.  By  elimination  of  these  n  —  1  —  k  functions  we  therefore 
obtain  an  equation 

A  +  A,y  +  ......  +  An_kyn-k  =  0, 

whose  coefficients  A,  Al}  ......  ,  An-k  are  rational  in  x.     Such  an  equation  is 

inconsistent  with  the  hypothesis  that  the  fundamental  equation  of  the  surface 
is  irreducible. 

(6)   Consider   two   places   of  the   Riemann  surface  at  which   the  inde 
pendent   variable,  x,  has  the  same  value  :   suppose,  first  of  all,  that   there 
are  no  branch  places  for  this  value  of  x.     Let  X,  \lt  ......  ,  \n-i  be  constants. 

Then  the  linear  function 

A.  +  Xj  GI  +  ......  +  \i-i  Gn-i 

cannot    have   the   same   value   at   these   two   places  for   all   values   of  \, 


For  this  would  require  that  each  of  G1}  ......  ,  Gn-\  has  the  same  value 

at   these   two   places.     Denote   these   values  by  a1}  ......  ,  an_i  respectively. 

We  can  choose  coefficients  filt  ......  ,  /zn_!  such  that  the  function 


*  The  dimension  of  an  integral  function  is  employed  by  Hensel,  Crelle,  t.  105,  109,  111  ;  Acta 
Math.  t.  18.  The  account  here  given  is  mainly  suggested  by  Hensel's  papers.  For  surfaces 
of  three  sheets  see  also  Baur,  Math.  Aniuil.  t.  43  and  Math.  Annal.  i.  46. 


58  GENERAL  PROPERTIES  OF  [43 

which  clearly  vanishes  at  each  of  the  two  places  in  question,  vanishes  also 
at  the  other  n  —  2  places  arising  for  the  same  value  of  x.  Denoting  the 
value  of  x  by  c,  it  follows,  since  there  are  no  branch  places  for  a;  =  c,  that 
the  function 

[l*i(Gi  ~  ai)  +  ......  +  Pn-i(Gn-i  -  a«_i)]/0  -  c) 

is  not  infinite  at  any  of  the  places  x  =  c.  It  is  therefore  an  integral 
rational  function. 

Now  this  is  impossible.  For  then  the  function  could  be  expressed  in 
the  form 

(x,  1)A  +  (x,  1)^  G,  +  ......  +  (a?,  !)„  GW_a  , 

and  it  is  contrary  to  what  is  proved  under  (a)  that  two  expressions  of 
these  forms  should  be  equal  to  one  another. 

Hence  the  hypothesis  that  the  function 

A  +  A!  GI  +  ......  +  Xn_j  6rn_] 

can  have  the  same  value  in  each  of  two  places  at  which  x  has  the  same 
value,  is  disproved. 

If  there  be  a  branch  place  at  x  =  c,  at  which  two  sheets  wind,  and  no 
other  branch  place  for  this  value  of  x,  it  can  be  proved  in  a  similar  way, 
that  a  linear  function  of  the  form 


cannot  vanish  to  the  second  order   at  the  branch   place,  for  all  values  of 
A!,  ......  ,  A7l_i  namely,  not  all  of   G1}  ......  ,  Gn-L  can  vanish  to  the  second 

order  at  the  branch  place.     For  then  we  could  similarly  find  an  integral 
function  expressible  in  the  form 


......  +  pn-i  £»-i)/0  -  c). 

More  generally,  whatever  be  the  order  of  the  branch  place  considered, 
at  x  =  c,  and  whatever  other  branch  places  may  be  present  for  x  =  c,  it  is 
always  true  that,  if  all  of  Gly  ......  ,  Gn-i  vanish  at  the  same  place  A  of 

the  Riemann  surface,  they  cannot  all  vanish  at  another  place  for  which  x 
has  the  same  value;  and  if  A  be  a  branch  place,  they  cannot  all  vanish 
at  A  t()  the  second  order. 

Ex.  1.     Denoting  the  function 


by  K,  and  its  values  in  the  n  sheets  for  the  same  value  of  x  by  K(l\  /if  <-),...,  K(n\  we 
have  shewn  that,  for  a  particular  value  of  x,  we  can  always  choose  X,  X1)t..,  Xn_1(  so 
that  the  equation  K(l)  =  KW  is  not  verified.  Prove,  similarly,  that  we  can  always 
choose  X,  A!,...,  Xn_x  so  that  an  equation  of  the  form 


)  =  0, 
where  m1,...,  mlc_1,  mk  are  given  constants  whose  sum  is  zero,  is  not  verified. 


43] 


FUNDAMENTAL   SYSTEMS. 


59 


Ex.  2.  Let  x  =  ylt...,yic  be  k  distinct  given  values  of  x:  then  it  is  possible  to 
choose  coefficients  X,  A!,...,  p,  Mi)"-)  finite  in  number,  such  that  the  values  of  the 
function 


at  the  places  x=y1,  shall  be  all  different,  and  also  the  values  of  the  function,  at  the 
places  x=yz,  shall  be  all  different,  and,  also,  the  values  of  the  function,  for  each  of 
the  places  #=y3,...,  yt,  shall  be  all  different. 

(c)     If  1,  HI,  H2, ,  Hn-i  be  another  fundamental  set  of  integral 

functions,   with    the    same   property   as    1,    Glt ,  Gn-\,   we   shall   have 

linear  equations  of  the  form 
1  =  1 

where  a;,  j  is  an  integral  polynomial  in  x. 

Now  in  fact  the  determinant 
For  if  I 


j  \   is  a  constant  (i=  1,  2,  ...,  n  —  1  ; 
denote  the  value  of  Hi,  for  a  general  value 


j  =  1,  2,  ...,  n  —  1). 

of  x,  in  the  rth  sheet  of  the  surface,  we  clearly  have  the  identity 


1,         1, 


,1 


10                ,0 

1,        1,. 

1 

'          '• 

.  £,<"> 

/-»        (i\    ri        (2) 
w  n—  i     >  "n—  1     >••••> 

Gn-i(n} 

ff          (1)      ff          (2)  ff          («) 

JJ  n  -i     >  •"  n— i     i )  L±  11—1 

If  we  form  the  square  of  this  equation,  the  general  term  of  the  square  of 

the  left  hand  determinant,  being  of  the  form  H^H^  + +  Hi{n)Hj(n},  will 

be  a  rational  function  of  x  which  is  infinite  only  for  infinite  values  of  x ;  it 
is  therefore  an  integral  polynomial  in  x.  We  shall  therefore  have  a  result 
which  we  write  in  the  form 


TB_1)  =  V«  .  A  (1,  <?,,  G,,  .......  Gn^\ 

aitj  \.     A  (1,  H1}  ......  ,  Hn^)  may  be  called  the 


A  (1,  H,t  ......  , 

where  V  is  the  determinant 
discriminant  of  1  ,  H^  ,  ......  ,  Hn^. 

If  /3  be  such  an  integral  polynomial  in  x  that  fty,  =  77,  say,  is  an  integral 
function,  an    equation    of  similar  form   exists  when   1,  tj,  if,  ......  ,  ijn~l  are 

written  instead  of  1,  Hl}  ......  ,  Hn^.     Since  then  A  (1,  77,  rf,  ......  ,  V1"1)  does 

not  vanish  for  all  values  of  x  it  follows  that  A  (1,  G1}  G.2  .......  ,  G^n-i)  does 

not  vanish  for  all  values  of  x.     (Cf.  (a),  of  this  Article.) 

But  because  1,  Hlt  H«,  ......  ,  Hn_±  are  equally  a  set  in  terms  of  which  all 

integral  functions  are  similarly  expressible,  it  follows  that  A  (1,H1,  ......  ,Hn_^) 

does  not  vanish  for  all  values  of  x,  and  that 

A  (1,  Glt  ......  ,  G_1)  =  Vi2  A  (1,  H,,  ......  ,  #„.,), 

where  V!  is  an  integral  function  rationally  expressible  by  x  only. 


60  FUNDAMENTAL   SYSTEMS.  [43 

Hence  V2  .  Vt2  =  1  :  thus  each  ofV  and  Vl  is  an  absolute  constant. 

Hence  also  the  discriminants  A  (1,  Glt ,  Gn_^)  of  all  sets  in  terms  of 

which  integral  functions  are  thus  integrally  expressible,  are  identical,  save 
for  a  constant  factor. 

Let  A  denote  their  common  value  and  771,..., rjn  denote  any  n  integral 
functions  whatever ;  then  if  A  fa,  i)2,  ...,  rjn)  denote  the  determinant  which  is 
the  square  of  the  determinant  whose  (s,  r)th  element  is  T/'J1,  we  can  prove,  as 
here,  that  there  exists  an  equation  of  the  form 

A  (%,%,...,  *»)  =  JfsAt 

wherein  M  is  an  integral  polynomial  in  x.  The  function  A  (77!,  rj2,...,  r)n)  is 
called  the  discriminant  of  the  set  77!,  tj2,...,  rjn.  Since  this  is  divisible  by  A, 
it  follows,  if,  for  shortness,  we  speak  of  1,  Hl,...,  #„_,,  equally  with  77^ 
i}2>-">  *7n>  as  a  set  of  n  integral  functions,  that  A  is  the  highest  divisor  common 
to  the  discriminants  of  all  sets  of  n  integral  functions. 

(d)     The    sets   (1,  GI, ,  Gn-i),  (1,  H1} ,  Hn^)   are    not   supposed 

subject  to  the  condition  that,  in  the  expression  of  an  integral  function  in 
terms  of  them,  no  term  shall  occur  of  higher  dimension  than  the  function  to 

be  expressed.     If  (1,  gl} ,  gn-i)  be  a  fundamental  system  for  which  this 

condition  is  satisfied,  the  equation  which  expresses   Gi  in  terms  of  1,  (ft, 

g.2, ,  gn-i    will    not    contain    any    of  these    latter   which    are    of  higher 

dimension  than  that  of  G*     Let  the  sets  G1 , ,  Gn-! ,  g1 , ,  gn^  be  each 

arranged  in  the  ascending  order  of  their  dimensions.     Then  the  equations 

which  express  Gly  G2, ,  Gk  in  terms  of  gl, ,  gn_l  must  contain  at  least 

k  of  the  latter  functions ;  for  if  they  contained  any  less  number  it  would  be 
possible,  by  eliminating  those  of  the  latter  functions  which  occur,  to  obtain 
an  equation  connecting  G1} ,  Gk  of  the  form 

(as,  !)*  +  (*,  l)Al  0,+ +  (x,  l\  0*  =  0; 

this  is  contrary  to  what  is  proved  under  (a). 

Hence  the  dimension  of  g^  is  not  greater  than  the  dimension  of  Gk  '• 

hence  the  sum  of  the  dimensions  of  Glf  G2> ,  Gn-i  is  not  less  than  the 

sum  of  the  dimensions  of  g1}  g2, ,  gn-i-     Hence,  the  least  value  which  is 

possible  for  the  sum  of  the  dimensions  of  a  fundamental  set  (1,  G1} ,  Gn-J 

is  that  which  is  the  sum  of  the  dimensions  for  the  set  (1,  <ft, ,  gn-i),  namely, 

the  least  value  is  p  +  n  —  1. 

We  have  given  in  the  last  Chapter  a  definition  of  p  founded  on 
Weierstrass's  gap  theorem :  in  the  property  that  the  sum  of  the  dimensions 
of  (ft,...,  gn--i  is  p  +  n  —  1  we  have,  as  already  remarked,  another  definition, 
founded  on  the  properties  of  integral  rational  functions. 

Ex.  1.     Prove  that  if  (1,  glt  ...,  gn^v\  (1,  hlt  ...,  hn_l)  be  two  fundamental  sets  both 
having  the  property  that,  in  the  expression  of  integral  functions  in  terms  of  them,  no  terms 


44]  THE   COMPLEMENTARY   FUNCTIONS.  61 

occur  of  higher  dimension  than  the  function  to  be  expressed,  the  dimensions  of  the 
individual  functions  of  one  set  are  the  same  as  those  of  the  individual  functions  of  the 
other  set,  taken  in  proper  order. 

Ex.  2.     Prove,  for  the  surface 

y«_ 

that  the  function 

rt 

satisfies  the  equation 

rf  -  Crj2  +  a2br)  -  «22ai  =  0  > 
and  that 

A  (1,  y,  rj)  =  bW  +  lSa^bc  -  27<Va22  -  4a1c3  -  4a263, 

A(l,  y,  /)  =  a12  A(l,  y,  ij)     A(l,  77,  ^2)  =  «22A(1,  y,  r,)     A  (y,  y\  r,)  =  a*<*  A(l,  y,  ij). 
In  general  1,  y,  rj  are  a  fundamental  set  for  integral  functions,  in  this  case. 

44.     Let  now  (1,  glt  g.,,  ......  ,  gn-\)  be  any  set  of  integral  functions  in 

terms  of  which  any  integral  function  can  be  expressed  in  the  form 

(x,  1)M  +  (x,  1  V,  <7i  +  ......  +  O,  1  ^  <7n_i  , 

and  let  the  sum  of  the  dimensions  of  g1}  ......  ,  #H_X  be  p  +  n  —  1. 

There  will  exist  integral  polynomials  in  x,  (3lt  /32,  ......  ,/37l_i,  such  that 

ftiy1  is  an  integral  function:    expressing  this  by  glt  ......  ,  gn-i  in  the  form 

above  and  solving  for  g^  ......  ,  gn-i  we  obtain*  expressions  of  which  the 

most  general  form  is 

_  /*i,  n-i 
9i 


where  /*;,«_!,  ......  >  Pi,i,  f*>i,  Di  are  integral  polynomials  in  x.     Denote  this 

expression  by  gi  (y,  x}. 

Let   the   equation    of   the   surface,   arranged   so   as   to   be   an   integral 
polynomial  in  x  and  y,  be  written 

f(y,x)  =  Q«yn  +  Qiyn-1+  ......  +  Qn-i  y  +  Qn  =  o, 

and  let  ^  (y,  x)  denote  the  polynomial 

Qo  y*+  &3T1  +  ......  +  Q,--i  y  +  Qt-, 

so  that  ^0  (y,  #)  is  Q0. 

Let  ^>0',  0i',  ......  ,  ^'n_!  be  quantities  determined  by  equating  powers  of  y 

in  the  identity 


*  Since  JT,,  ...,  <;n_j  are  linearly  independent. 


62                                              ALTERNATIVE   DEFINITIONS   OF  [44 

in  other  words,  if  the   equations  expressing  1,  y,  y2, ,  yn-1  in  terms  of 


1-1, 


iin~l  —  n         4-  n  «    4-  -I-/7  n 

y          ~  "'n— l  T  W'n— i,  i  </i    r T  <*n— i,  n— l  J/n— u 

where  the  coefficient  G^J  is  an  integral  polynomial  in  x  divided  by  /:?;,  then 

r  O  /x^1 — 1   V«7   *       s  1  s\,^ 2  \,7   >       /     r  •  •  •  •  •  •    i     **"n — 1  /^Q 

So  that  if  we  write 
n  being  the  matrix  of  the  transformation,  we  have 

where  %/  =  %;  (y',  #),  and  H  represents  a  transformation  whose  rows  are  the 
columns  of  H,  its  columns  being  the  rows  of  D. 

But  if  (Q)  denote  the  substitution 

Qn-2,       Qn-3, ,  Qo,       0 

ft,       ft,      0,    

Q0,       0,      

we  have 

Hence,  changing  y'  to  y  in  fa'  and  writing  therefore  fa  for  fa',  we  may  write 
Either  this,  or  the  original  definition,  which  is  equivalent  to 

y'-y 
=  %o  y"-1  +  y71-2  %i  (y',  «)  + +  y %n-2 (y',  <*)  +  x«-i  (y,  *) (F), 

may  be  used  as  the  definition  of  the  forms  fa,  fa, ,  <£n_j. 

The  latter  form  will  now  be  further  changed  for  the  purposes  of  an 
immediate  application  :  let  ylf ,  yn  denote  the  values  of  y  corresponding 


44] 


THE   COMPLEMENTARY   FUNCTIONS. 


63 


to  any  general  value  of  x  for  which  the  values  of  y  are  distinct.     Denote 
fc  (Vr,  *),  ffi  (yr,  *),  by  fc<",  <7*(r)>  etc. 

Then  putting  in  (F)  in  turn  y  =  tf  =  y1  and  y'  =  ylly  =  y»,  we  obtain 


=  2'  3> 


Hence  if,  with  arbitrary  constant  coefficients  cfl,  c1} ,  Cn_i,  we  write 

Co<£o(1>  +  C^1"  + +  C,^  ^  =  </>(1), 

we  have 

'  c0     Cj      cn_!        ^>(1)         =  0, 

1  n   I1)  rt          I1'          / 

1        .<7i    ' yn-i          J 


or 


/'(* 


1 

1  ^1(1) 


^n-i 


1     ^ 


0 
r        0 

1      9^ 


Cji— i 


ffn-i 


(n) 


.(G); 


and  we  shall   find   this    form   very  convenient:   it   clearly  takes   an   inde 
terminate  form  for  some  values  of  x. 

If  we  put  all  of  d,  ......  ,  Cn-i,  =  0  except  cr,  and  put  cr  =  1,  and  multiply 

both  sides  of  this  equation  by  the  determinant  which  occurs  on  the  left  hand, 
the  right  hand  becomes 


where,  if  sijj  =  gi^  #/>  +  g 
in  the  determinant 


+  ......  +^"1'  g}™,  Sitj  means  the  minor  of  sitj 


$1  *1,  1  ^1,  2 


1,  n— i 


Sn— i   Sn—i,  i    *n— i,  2 *n— i,  n— i 


Since  this  is  true  for  every  sheet,  we  therefore  have 

<f>r      _  Sr  +  Srt  ij(/i+ +  Sr>  n-i  ffn-i 

" 


^aA      !_  3A  1    ^A_ 


64  INVERSE   DETERMINATION  [44 

and  therefore,  also 


The  equation  (H)  has  the  remarkable  property  that  it  determines  the 
functions  ,,(  .  from  the  functions  gt  with  a  knowledge  of  these  latter  only. 

J        \<y  x 

But  we  can  also  express  g1}  ......  ,  gn-i  so  that  they  are  determined  from 

y    ,      y    ,  ......  ,  -FTJ\  ,  with  a  knowledge  of  these  only. 

For  let  these  latter  be  denoted  by  70,  71,  ......  ,  yn-i'  and,  in  analogy  with 

« 
the  definition  of  sr,  i,  let  a-ft  f  =  "2  <yr{s}  7t(s). 

s=l 

Then  from  equation  (H) 

n  I    T  1 

S  7r(S)  #<«>  =  X      >SU  +  Sr,  i  «i,  i  +  ......  +  Sr,  n-i  Si,  n-i 

«=i  ^  L 

=  0  or  1  according  as  z  =}=  r  or  t  =  r. 

Therefore,  also,  by  equation  (H), 


+i  ......          • 

s=i 

1 


so  that  equation  (H)  may  be  written 

Jr  =  <Tr,  o  +  °V,  1  9\  +  ......  +  °V,  n-i  ^n-i- 

If  then  Sr,  i  denote  the  minor  of  ov,  <  in  the  determinant  of  the  quantities 
<rr  ti  —  which    determinant   we   may   call   V  (y0,  <y1}  ......  ,7*1-1)  —  we   have,   in 

analogy  with  (H), 

gr=^  (Sr  7o  +  Sril  7!+  ......  +  Srin_!7»_i)  ...............  (K)*. 

Of  course  V  =  -^  and  2r>  i  =  -r-  s.r>  t-,  and  equation  (K)  is  the  same  as  (H'). 
Ex.  1.     Verify  that  if  the  integral  functions  ffi,  ...,  gn-i  have  the  forms 


wherein  Z)15  ...,!>„_!  are  integral  polynomials  in  x,  then  <£0,  ...,  0n_!  are  given  by 


*  The  equations  (H)  and  (K)  are  given  by  Hensel.    In  his  papers  they  arise  immediately  from 
the  method  whereby  the  forms  of  >t  ,  y2  ,  ......  are  found. 


45]  EXPRESSION    OF   INTEGRAL   OF   THE   THIRD   KIND. 

Ex.  2.     Prove  from  the  expressions  here  obtained  that 


65 


and  infer  that  2  (dv/d.v)i  =  0, 

8=1 

v  being  any  integral  of  the  first  kind. 

45.     We  are  now  in  a  position  to  express  the  Riemann  integrals. 

Let  P£  £  be  a  general  integral  of  the  third  kind,  infinite  only  at  the 
places  xlt  scz.  Writing,  in  the  neighbourhood  of  xl,  x  —  xl  =  tlWt+l,  dP/dx 
will  (§§  14,  16)  be  infinite  like 


namely,  like 


dP 
y 


thus    (x  —  #1)  ^  is  finite  at  the  place  x1  and   is  there   equal  to 


Similarly  (x  —  xz)  -,--  is  finite  at  #2  and  there  equal  to 


w2+  1' 

Assume  now,  first  of  all,  for  the  sake  of  simplicity,  that  at  neither  x  =  x± 
nor  x  —  x%  are  there  any  branch  places ;   let  the  finite  branch  places  be  at 


At  any  one  of  these  where,  say,  x  =  a  +  tw+1,  dPjdx  is  infinite  like 
1          d 


(w  +  l)f 
dP  . 


-V +...], 


and  therefore  (x  —  a)  -=-  is  zero  to  the  first  order  at  the  place. 
7  dx 

Hence,  if  a  =  (x  —  aa)  (x  —  a,). . . 

be  the  integral  polynomial  which  vanishes  at  all  the  finite  branch  places  of 
the  surface,  and  g  be  any  integral  function  whatever,  the  function 

K.a.g.(»-^)(,-^ 

is  a  rational  function  which  is  finite  for  all  finite  values  of  x  and  vanishes  at 
every  finite  branch  place. 

Therefore  the  sum  of  the  values  of  K  in  the  n  sheets,  for  any  value  of  x, 
being  a  symmetrical  function  of  the  values  of  K  belonging  to  that  value  of  x, 
is  a  rational  function  of  x  only,  which  is  finite  for  finite  values  of  x  and  is 
therefore  an  integral  polynomial  in  x.  Since  it  vanishes  for  all  the  values  of 


66  EXPRESSION   OF    INTEGRAL   OF  [45 

x  which  make  the  polynomial  a  zero,  it  is  divisible  by  a,  and  may  be  written 
in  the  form  aJ. 

Let  the  polynomial  J  be  written  in  the  form 

Xx  (x  -  a;2)  -  X2  (x  -  X-L)  +  (x  -  x^  (x  -  x2)  H, 

wherein  7^  and  X2  are  constants  and  H  is  an  integral  polynomial  in  x.     This 
is  uniquely  possible.     Let  H  be  of  degree  ^  -  1  in  x  ;  denote  it  by  (x,  \Y~\ 

Then,  on  the  whole, 

(g  =  -       -  -  --  +  (..  I)-'. 

— 


Multiply  this  equation  by  a;  —  a^  and  consider  the  case  when  x  =  xl}  there 
being  by  hypothesis  no  branch  place  at  as  =  xt.  Thus  we  obtain  the  value  of 
Xj  ;  namely,  it  is  the  value  of  g  at  the  place  x^  This  we  denote  by  g(xly  y^. 
Similarly  X,,  is  g  (ara,  y2).  Further,  at  an  infinite  place  where  as  =  t-(w+l), 

dP  =       tw+^  dP 
dx         w  +  1  dt 

so  that  x^dPjdx  is  finite  at  all  places  x  =  oc  .  Hence  if  p  +  1  be  the  dimen 
sion  of  the  integral  function  g,  and  we  write 


a-P-i  (^  _  tfj)      ^p-1  (a;  -  x.2) 
we  can  infer,  since  p  cannot  be  negative,  that  yu,  is  at  most  equal  to  p. 

Hence,  taking  g  in  turn  equal  to  1,  glt  ...,  gn-i,  the  dimensions  of  these 
functions  being  denoted  by  0,  r,  +  1,  ...  ,  rn-,  +  1,  we  have  the  equations 


/ 
V 


dP\  dP\ 


.  .  +  =  - 

1     (dx),  yi      \dx)n        x-x,  x- 


(-} 

\dx/i 


where  r\,  ... ,  r'7l_]  are  positive  integers  not  greater  than  Tlf ... ,  TW_I  respectively. 

Let  these  equations  be  solved  for  (-5-)  :  then  in  accordance  with  equa- 

\dxj-i 

tions  (G)  on  page  63  we  have,  after  removal  of  the  suffix, 


45]  THE   THIRD   AND    FIRST   KIND.  67 

f  (y)          =  (x,  IV''-1  <f>,  +  (x.  1)T'*~J  <k  +  . . .  +  (x,  IVVi"1  <f»rt_i 

dx 

+ 

vU   ^^   *^\ 


where  </>i  stands  for  <£;  (a;,  y). 

This,  by  the  method  of  deduction,  is  the  most  general  form  which  dP/dx 
can  have ;  the  coefficients  in  the  polynomials  (x,  I)1"'*"1  are  in  number,  at  most, 

T!  +  T2  +  ...  +TH_!, 

or  p ;  and  no  other  element  of  the  expression  is  undetermined.     Now  the 
most  general  form  of  dP/dx  is  known  to  be 


1  dx  p  dx      \dx  J  ' 

wherein  f  ~^-  1  is  any  special  form  of  -y-   having  the  necessary  character,  and 

\i ,  ...,  \p  are  arbitrary  constants.     Hence,  by  comparison  of  these  forms,  we 
can  infer  the  two  results — 

(i)     The  most  general  form  of  integral  of  the  first  kind  is 
f   dx  ,_j 

J  f(y}  X''J  '  0n-i(^,  y)J, 

wherein  r'i  <  T;  and  the  coefficients  in  (x,  I)7'"1  are  arbitrary : 

(ii)  A  special  and  actual  form  of  integral  of  the  third  kind  logarithmically 
infinite  at  the  two  finite,  ordinary,  places  (xly  y^,  (x»,  7/2),  namely  like 
log  [(x  —  x1)/(x  —  x2)],  and  elsewhere  finite,  is 

f     i  77  I  I  nr o" 

J          I        \y  J    I  tv  t*/j 

0o  (iC>  y}  +  0i  (x,  y}  gl  (x2,  y2)  +  . . .  +  0n_a  (x,  y)  gn-\  (&-2>  2/2)! 

r  _  y 

A      ^2  J 

or 

fx    dx     /"*•  ,    d  r^>0 (x,  y)  +  0! (x,  y) gl (£,  tj)  +  ...  +  0n_i (x,  y) gn-\ (j£,  ri}~\ 


In  the  actual  way  in  which  we  have  arranged  the  algebraic  proof  of  this 
result  we  have  only  considered  values  of  the  current  variable  x  for  which  the 
n  sheets  of  the  surface  are  distinct :  the  reader  may  verify  that  the  result 
is  valid  for  all  values  of  x,  and  can  be  deduced  by  means  of  the  definitions 
of  the  forms  </>„,  ...,  <£n_j,  which  have  been  given,  other  than  the  equation 
(G). 

Ex.     Apply  the  method  to  obtain  the  form  of  the  general  integral  of  the  first  kind  only. 

5—2 


68  DEDUCTION    OF    INTEGRAL   OF   SECOND    KIND.  [45 

We  shall  find  it  convenient  sometimes  to  use  a  single  symbol  for  the 
expression 

<f>0  (as,  y)  +  (/>!  (x, 


and  may  denote  it  by  (#,  £).     Then  the  result  proved  is  that  an  elementary 
integral  of  the  third  kind  is  given  by 


em 

Px'       =  \    dx  \(x,  #1)  —  (x,  a?.,)"]. 

xltx.2       Jc         LV    ' 


This  integral  can  be  rendered  normal,  that  is,  chosen  so  that  its  periods  at 
the  p  period  loops  of  the  first  kind  are  zero,  by  the  addition  of  a  suitable 
linear  aggregate  of  the  p  integrals  of  the  first  kind. 

Now  it  can  be  shewn,  as  in  Chapter  II.  §  19,  that  if  Ex'  c  denote  an  elemen 
tary  integral  of  the  second  kind,  the  function  of  (x,  y)  given  by  the  differ 
ence 

,„.  .....  «(,dj:  ^n;-*?'.  M**pt«        --••.!« 

wherein  D%  denotes  a  differentiation,  is  not  infinite  at  (£,  •»?).  It  follows  from 
the  form  of  P*'  °x  ,  here,  that  this  function  does  not  depend  upon  (x2,  y«). 
Hence  it  is  nowhere  infinite,  as  a  function  of  (x,  y}.  Therefore,  if  not  inde 
pendent  of  (x,  y),  it  is  an  aggregate  of  integrals  of  the  first  kind.  Thus  we 
infer  that  one  form  of  an  elementary  integral  of  the  second  kind,  which  is 
once  algebraically  infinite  at  an  ordinary  place  (£,  •»;),  like  —  (as  —  ^)~1,  is 
given  by 

dx_   d^     ftp  (x,  y)  +  0!  (as,  y)  gl  (  £  ??)+...  +  <f>n-i  ( 


The  direct  deduction  of  the  integral  of  the  second  kind  when  the  infinity 
is  at  a  branch  place,  which  is  given  below,  §  47,  will  furnish  another  proof  of 
this  result. 

46.  We  proceed  to  obtain  the  form  of  an  integral  of  the  third  kind  when 
one  or  both  of  its  infinities  (xly  yj,  (<KZ,  y»)  are  at  finite  branch  places  ;  and 
when  there  may  be  other  branch  places  for  x  =  xl  or  x  =  x2. 

As  before,  let  a  be  the  integral  polynomial  vanishing  at  all  the  finite 
branch  places.  The  function 

ga  (x  —  ajj)  (x  —  #2)  dP[dx 

will  vanish  at  all  the  places  x  =  xl  :  and  though  it  may  vanish  at  some  of 
these  to  more  than  the  first  order,  it  will  vanish  at  (x1}  y^)  only  to  as  high 
order  as  (x  —  x^}.  Hence  the  sum  of  the  values  of  this  function  in  the  several 
sheets  for  the  same  value  of  x  is  of  the  form  aJ,  where  J  is  a  polynomial  in  x 
which  does  not  vanish,  in  general,  for  x  =  x±  or  x  =  x.^. 


46]     INTEGRAL   OF   THIRD    KIND    WHEN    INFINITIES   ARE   BRANCH    PLACES.      69 

Hence  as  before  (§  45)  we  can  write 

/    dP\  I    dP\  Xx  X., 

Iff  T-  1+  •••  +  U7  j  ~  1=  -  +(x,iyt-1. 

\    ax  /i  \    tW  /n     x  —  xl     x  —  x» 

Multiply  this  equation  by  x  —  xl  and  consider  the  limiting  form  of  the 
resulting  equation  as  (x,  y)  approaches  to  (x1,  y^)  :  let  w  +  1  be  the  number  of 
sheets  which  wind  at  this  place.  Recalling  that  the  limiting  value  of 
(x  —  x^dPjdx  is  l/(w+l),  we  see  that  w+I  terms  of  the  left  hand,  corre 
sponding  to  the  w+  1  sheets  at  the  discontinuity  of  the  integral,  will  take  a 
form 


where  e  is  a  (?y  +  l)th  root  of  unity.  The  limit  of  this  when  t  =  0  is 
9(xi>  y\)l(w  +  1);  the  corresponding  terms  of  the  left  will  therefore  have 
9(xi>y\)  as  limit.  The  other  terms  of  the  left  hand  will  vanish. 

Hence  Xj  =  g(xlt  y^),  X2  =  ^(^2,  y2).  The  determination  of  the  upper  limit 
for  p  and  the  rest  of  the  deduction  proceed  exactly  as  before.  Thus, 

The  expression  already  given  for  an  integral  of  the  third  kind  holds  ivhether 
(%i>  yi),  (#2,  y-)  be  branch  places  or  ordinary  places. 

If  we  denote  the  form  of  integral  of  the  third  kind  thus  determined  by 
•P^  *  >  the  zero  c  being  assigned  arbitrarily,  it  follows,  as  in  §  45,  above,  that 
an  elementary  integral  of  the  second  kind,  which  is  infinite  at  a  branch 
place  #!,  is  given  by 


Now  if  we  write  t  for  tXl  and  #/  =xl  +  tw+1,  the  coefficient  of  dxff'(y)  in  the 
integrand  of  the  form  here  given  for  Px'fc    is 

Xi  ,  Xi 

<t>«  +  01  •  (ffi  +  tg,'  +...)+...  +  (/>n-i  •  (gn-i  +  tg'n-i  +  •  •  •) 


x  -  a?  - 


wherein  ^>0,  ...,  </>„_,  are  functions  of  a-,  y,  and  ^,  ....  r/,^,  #/,  f//,  ...  are 
written  for  5r](^1)  y,),  ...  ,  gn_,  (Xl,  y,),  Dg^x,,  y}),  Dg,(xl}  y,),  ...  ,  respectively, 
D  denoting  a  differentiation  in  regard  to  t.  Hence  the  ultimate  form  is 


70  EXAMPLES.  [46 

That  is,  introducing  £,  tj,  instead  of  xly  ylt  an  elementary  integral  of  the 
second  kind,  infinite  at  a  finite  branch  place  (f,  rj),  is  given  by 

da;    0!  (as,  y)  g(  (£,  rf)  +  . . .  +  <£n_!  (x,  y)  #'„_,  (£,  77) 


/'(y)  f-f 

where  </i  (£,  77),  ...  are  the  differential  coefficients  in  regard  to  the  infini 
tesimal  at  the  place.  It  has  been  shewn  in  (6)  §  43  that  these  differential 
coefficients  cannot  be  all  zero. 

Sufficient  indications  for  forming  the  integrals  when  the  infinities  are  at 
infinite  places  of  the  surface  are  given  in  the  examples  below  (1,  2,  3,  ...);  in 
fact,  by  a  linear  transformation  of  the  independent  variable  of  the  surface  we 
are  able  to  treat  places  at  infinity  as  finite  places. 

Ex.  1.     Shew  that  an  integral  of  the  third  kind  with  infinities  at  (xly  y^,  (x.2t  #2)  can 
also  be  written  in  the  form 


(a?,  y)  ffr  (xl  ,  ?/i)     X2  -  *  00  (x,  y  )  +  2X2T»-  <ftr  (x, 


_ 

./'(y)  #-#1  ^-^2 

wherein  X1  =  (^-a)/(*'1-a),  \2  =  (x-a)/(x.2-a},  T,.  +  I  is  the  dimension  of  gr,  and  a  is  any 
arbitrary  finite  quantity. 

It  can  in  fact  be  immediately  verified  that  the  difference  between  this  form  and  that 
previously  given  is  an  integral  of  the  first  kind.  Or  the  result  may  be  obtained  by  con 
sidering  the  surface  with  an  independent  variable  £  =  (x  —  a)~l  and  using  the  forms  of  §  39 
of  this  chapter  for  the  fundamental  set  for  functions  infinite  only  at  places  x  —  a.  The 
corresponding  forms  of  the  functions  <j>  are  then  obtainable  by  equations  (H)  §  44. 

Ex.  2.  Obtain,  as  in  the  previous  and  present  Articles,  corresponding  forms  for  inte 
grals  of  the  second  kind. 

Ex.  3.  Obtain  the  forms  for  integrals  of  the  third  and  second  kinds  which  have  an 
infinity  at  a  place  x=  QO  . 

It  is  only  necessary  to  find  the  limits  of  the  results  in  Examples  1  and  2  as  (x1,  y-^) 
approaches  the  prescribed  place  at  infinity.  It  is  clearly  convenient  to  take  a  =  0. 

Ex.  4.     For  a  surface  of  the  form 

y*  =  x(x-a1)  ......  (#-02P  +  i), 

wherein  a1}  ...,  a2p  +  1  are  finite  and  different  from  zero  and  from  each  other,  we  may*  take 
the  fundamental  set  (1,  g^)  to  be  (1,  y\  and  so  obtain  (00,  </>1)=:(fy,  1).  Assuming  this, 
obtain  the  forms  of  all  the  integrals,  for  infinite  and  for  finite  positions  of  the  infinities. 

Ex.  5.  In  the  case  of  Example  4  for  which  />  =  !,  the  integral  of  Example  1,  when  a 
is  taken  0,  is 

fdx  r^  y+aft^-'yt  _  ^  y  +  *?Xj~*yi\ 
]  y  \-x        x  —  xv  x        x  —  x2      J" 

Putting  xl  =  QO  and  yl  —  tnx^  +  nxt  +  A  +  Bxv  ~  1  +  .  .  .,  this  takes  the  form 


_^  fdx 
^  J  y 

,    [ 
-4| 

J 


|          z 


y   _     x 

dx  F 
Imz  + 

V  L         x-Xz     x 


Chap.  V.  §  56. 


47]  DIRECT    PROOF   FOR   INTEGRAL    OF    SECOND    KIND.  71 

Prove  that  this  integral  is  infinite  at  one  place  x  =  cc   like  logf-J  and  is  otherwise 
infinite  only  at  (.vz,  y.2),  namely  like  —  log  (x  —  .>;2),  if  (.i'2,  yz)  be  not  a  branch  place. 
Ex.  6.     Prove  in  Example  5  that  the  limit  of 

2  /  ~  \~        ~     ~         I        ~ 

j  y  L'*       •*    **i  •*     j 

as  (,i\,  yj)  approaches  that  place  (ao  ,  oo  )  where  y  =  mx*  +  njc+A  +  B/jc  +  ...,  is 


y 

and  that  the  expansion  of  this  integral  in  the  neighbourhood  of  this  place  is 

A    1 


and  that  it  is  otherwise  finite.  It  is  therefore  an  integral  of  the  second  kind  with  this 
place  as  its  infinity.  The  process  by  which  the  integral  is  obtained  is  an  example  of  the 
method  followed  in  the  present  and  the  last  Articles,  for  obtaining  an  elementary  integral 
of  the  second  kind  from  an  elementary  integral  of  the  third  kind. 

47.  We  give  now  a  direct  deduction  of  the  integral  of  the  second  kind 
whose  infinity  is  at  a  finite  place  (£,  77)  :  we  suppose  that  (w  +  1)  sheets  of 
the  surface  wind  at  this  place,  and  find  the  integral  which  is  there  infinite 
like  an  expression  of  the  form 

<"•!  ,  -4.J  .         .  Aw     Aw+1 

T"T4        h>+^£' 

t  being  the  infinitesimal  at  the  place. 

Firstly,  let  F  be  an  integral  which  is  infinite  like  the  single  term  (x  —  ^)~l> 
so  that  in  the  neighbourhood  of  the  infinity  its  expansion  has  a  form 

F=    ± 


Forming  as  before  the  sum  of  the  values  of  the  functions  g  .  (x  —  £)2  dFJdx  in 
the  n  sheets  of  the  surface,  g  being  any  integral  function,  we  obtain  an 
expression 


Putting  x  =  %  we  infer,  since  all  terms  on  the  left  except  those  belonging  to 
the  place  (£,  77)  vanish,  that 


Differentiating,  and  then  putting  a;  =  f,  we  obtain,  from  the  terms  on  the  left 
belonging  to  the  infinity, 


the  summation  extending  to  (w  +  1)  terms. 


72  DIRECT   INVESTIGATION  [47 

Now 

r  rl  ~l  1  (J 

•-  ; — T^-^T:.  -r.  \V+*  (B+2Ct +  ...)'} 


dos 
vanishes  when  t  is  zero  :  hence 


Hence  we  can  prove  as  before  that,  save  for  additive  terms  which  are 
integrals  of  the  first  kind,  the  integral  which  is  infinite  like  (as  —  £)~J  is 
given  by 

ix    Dw+l  [<£0  +  </>!#!  (f, 


This  result  is  true  whether  (^,  ?;)  be  a  branch  place  or  an  ordinary  place. 

Consider  now  the  integral,  say  E,  which  is  infinite  at  (f,  77)  like  t~m,  m 
being  a  positive  integer  less  than  w  +  1.   At  this  place,  therefore,  (x  —  £)  dEjdx 

171 

is  infinite  like  ---  —  y  .  —  .     If,  as  before,  we  consider  the  sum  of  the  n  values 

of  the  expression  a  .  g  .  (x  —  £)  dE/dx,  wherein  </  is  any  integral  function  and 
a  is  the  integral  polynomial  before  used,  which  vanishes  at  all  the  finite 
branch  points  of  the  surface,  we  shall  obtain 


To  find  X,  let  x  approach  to  £.  Then  all  the  terms  on  the  left,  except 
those  for  the  w+1  sheets  which  wind  at  the  infinity  of  E,  vanish  :  for  such  a 
non-vanishing  term  we  have  an  expansion  of  the  form 


where  D  denotes,  as  usual,  a  differentiation  in  regard  to  the  infinitesimal  of 
the  surface  at  (|,  77),  and  g  is  written  for  g  (£,  77).  The  sum  of  these  w+1 
expansions  is 


Now  in  fact  every  summation  ^tr,  being  a  sum  of  terms  of  the  form 


wherein  e  is  a  primitive  (w  +  l)th  root  of  unity,  will  be  zero  unless  r  be  a 
multiple  of  w+1.     Thus  the  terms  involving  negative  powers  of  t  in  the 


48] 


OF  INTEGRAL  OK  SECOND  KIND. 


73 


sum  will  vanish :  those  involving  positive  powers  of  t  will  vanish  ultimately 
when  t  —  0 ;  and  in  fact  A  is  zero,  otherwise  E  would  contain  the  logarithmic 
term  A  log  (x  —  £)  when  (x,  y)  is  near  to  (£,  77).  Hence  on  the  whole 


A.  —  — 


m  —  1 


Then,  proceeding  as  before,  we  obtain  an  expression  of  the  integral  in  the 
form, 

1       fx   dx  1 

~  ^  i  J 


Thus,  denoting  the  expression 


n-\ 


<£„  0,  y)  +  2  <f>r  (x,  y)  gr  (£,  77) 

i 

by  <t>,  an  integral  which  is  infinite  like  an  expression 

A 

•"•  i/i-i-i 


is  given  by 


t 


,          , 
h 


x    dx 


<t> 


*^^         I     >P. 


Of  course  the  differentiations  at  the  place  (£,  77)  must  be  understood  in 
the  sense  in  which  they  arise  in  the  work.  If  <£  (£,  77)  be  any  function  of 
£,  77,  D<f>  (£,  77)  means  that  we  substitute  in  <f>  (x,  y),  for  x,  %  +  tw+1,  and  for  y, 
an  expression  of  the  form  77  +  P(t\  that  we  then  differentiate  this  function  of 
t  in  regard  to  t,  and  afterwards  regard  t  as  evanescent. 

Ex.  1.     Obtain  this  result  by  repeated  differentiation  of  the  integral  pf'e . 

Ex.  2.  Obtain  by  the  formula  the  integral  which  is  infinite  like  A/t  +  JB/t'2  in  the 
neighbourhood  of  (0,  0),  the  surface  being  f  =  x(x,  1)3.  Verify  that  the  integral  obtained 
actually  has  the  property  required. 

48.     The  determinant  A  (1,  glt  ... ,  gn_^,  of  which  the  general  element  is 


can  be  written  in  the  form 


,     x~ri~1sl 


,     x~Ti 


X~Tn-i 


-1 


.,    orTn-r 


In  this  form  the  determinant  factor  is  finite  at  every  place  x  =  oo :  hence 
also  ar <*-*+»»>  A (1,  ffl,  ... ,  #„_,)  is  finite  (including  zero)  at  infinity.     Thus 


8  h 

OF     i 

TJNIVERSII 


74  THE    ESSENTIAL   FACTOR   OF   THE    DISCRIMINANT.  [48 

A  (1,  glt  ...  ,  gn-i},  which  is  an  integral  polynomial  in  x,  is  of  not  higher  order 
than  2?i  —  2  +  2p  in  x. 

But  when  the  sheets  of  the  surface  for  x  =  oc  are  separate,  it  is  not  of  less 
order  ;  it  is  in  fact  easy  to  shew  that  if  for  any  value  of  x,  x  =  a,  there  be 
several  branch  places,  at  which  respectively  w1  +  1,  w2+  1,  ...  sheets  wind,  then 
A  (1,  g1}  ...,  gn_j)  contains  the  factor  (x—  a)wi+w*+-. 

For,  writing,  in  the  neighbourhood  of  these  places  respectively, 

x-a  =  t1w'+l,  a?  —  a  =  «2W»+1,  ..., 
the  determinant  (§  43) 

(1)  ^ 


.   or,   .    •    ,   gzii  , 

of  which  A(l,  glt ...,  gn-i)  is  the  square,  can,  for  values  of  x  very  near  to 
x  =  a,  be  written  in  a  form  in  which  one  row  divides  by  tlt  another  row  by 
ti2. ...,  another  row  by  t^1,  in  which  also  another  row  divides  by  t2,  another 
row  by  t.?,...,  and  another  row  by  t.2w>,  and  so  on. 

Thus  this  determinant  has  the  factor  ^wi(«'i+1)  t£w*(w*+l) . . . ,  and  hence 
the  square  of  this  determinant  has  the  factor  (x  —  a)Wl  (x  —  a)w<i 

Therefore,  when  there  are  no  branch  places  at  infinity,  A  (1,  glt  ...,gn-i) 
has  at  least  an  order  2w,  =  2n+.2p  —  2  (§  6). 

In  that  case  then  A  (1,  gly  ...,  gn-\)  is  exactly  of  order  2n  +  2p  —  2:  and, 
when  all  the  branch  places  occur  for  different  values  of  x,  its  zeros  are  the 
branch  places  of  the  surface,  each  entering  to  its  appropriate  order. 

When  the  surface  is  branched  at  infinity,  choose  a  value  x  =  a  where 
all  the  sheets  are  separate:  and  let  gi  =  (x  —  a)Ti+IA;.  Then  by  putting 
£  =  (#  —  a)"1  we  can  similarly  prove  that  A(l,  Aa,  ...,/fn_[)  is  an  integral 
polynomial  in  £  of  precisely  the  order  2n  +  2p—2.  But  it  is  immediately 
obvious  that 


Hence  if  the  lowest  power  of  £  in  A  (1,  h1}  ...  ,  An_i)  be  f",  A  (1,  g1}  ...  ,  gn~i) 
is  an  integral  polynomial  of  order  2n  +  2p  —  2  —  s.  In  this  case  the  zeros  of 
A  (1,  gly  ...  ,  gn-i),  which  arise  for  finite  values  of  x,  are  the  branch  places, 
each  occurring  to  its  appropriate  order,  provided  all  the  branch  places  occur 
for  different  values  of  x:  and  A  (1,  hi,  ...  ,  hn-i)  vanishes  for  x=<x>  to  an 
order  expressing  the  number  of  branch  places  there. 

Ex.  1.     For  the  surface  y*=3?(x-  !)(#-«)  there  are  two  branch  places  at  x=0,  and 
a  branch  place  at  each  of  the  places  #=1,  x=a,  where  all  the  sheets  wind.     Thus 

-2  =  w=2.  1  +  3  +  3  =  8. 
Chap.  II.  §  21. 


49]  RATIONAL    FUNCTION    WITH  p  +  I    POLES.  75 

For  thi.s  surface  fundamental  integral  functions  are  given  by  ffl=y,  9<i=y^lx,  ff3=y3/x- 
With  these  values,  prove  that  A  (1,  fflt  g^  #3)=  -256.1'2  (.>;-  I)3  (x-aj\  there  being  a  factor 
.i-'2  corresponding  to  the  superimposed  branch  places  at  .r  =  0,  while  the  other  factors  are  of 
the  same  orders  as  the  branch  places  corresponding  to  them. 

Ex.  2.  The  surface  y^  =  x^(x—  1)  is  similar  to  that  in  the  last  example,  but  there  is  a 
branch  place  at  infinity  at  which  the  four  sheets  wind,  so  that,  in  the  notation  of  thi.s 
Article,  s  =  3.  As  in  the  last  example  2n  +  2p  —  2  =  8,  and  1,  y,  y^lx^flx  are  a  fundamental 
system  of  integral  functions.  Prove  that,  now,  &(1,  <Ji,  g2,  y3)  is  equal  to  -25tu>2(x--l):{, 
its  order  in  x  being  2/i  +  2p  —  2  —  s  =  8  —  3  =  5. 


49.  In  accordance  with  the  previous  Chapter*  the  most  general  rational 
function  having  poles  at  p  +  1  independent  places,  is  of  the  form  AF+B, 
where  F  is  a  special  function  of  this  kind  and  A,  B  are  arbitrary  constants. 
The  function  will  therefore  become  quite  definite  if  we  prescribe  the 
coefficient  of  the  infinite  term  at  one  of  the  p  +  1  poles  —  the  so-called  residue 
there  —  and  also  prescribe  a  zero  of  the  function. 

Limiting  ourselves  to  the  case  where  the  p  +  1  poles  are  finite  ordinary 
places  of  the  surface,  we  proceed,  now,  to  shew  that  the  unique  function  thus 
determined  can  be  completely  expressed  in  terms  of  the  functions  introduced 
in  this  chapter.  It  will  then  be  seen  that  we  are  in  a  position  to  express 
any  rational  function  whatever. 

If  the  general  integral  of  the  third  kind  here  obtained  with  unassigned 
zero  be  denoted  by  P^  a  ,  the  current  variables  being  now  (z,  s),  instead  of 
(x,  y),  the  infinities  of  the  function  being  at  x  and  a,  the  function 


«  =  </>•>  (z,  s)  +  fa  (z,  s}gl(x,y}  +  ......  +  </>„_,  (z,  s)  gn^  (x,  y) 

dz  z-  x 

<fto  (z,  s)  +  fa  (z,  s)  g,  +  ......  +  ftn~i  (z,  s)    «_! 


(z,  s)  (z,  IX'-1^- +  fal_1  (z,  s)  (z,  l)\-rl, 

wherein  glt  ...,  gnr_l  are  written  for  the  values  of  the  functions  gl  (z,s),  ..., 
f/n-i  (z,  s)  at  the  place  denoted  by  a,  contains  p  disposeable  coefficients, 
namely,  those  in  the  polynomials  (z,  \}^~l, ,  (z,  l)Tn-i~l. 

Let  now  cl} ,  cp  denote  p  finite,  ordinary  places  of  the  surface,  the 

values  of  z  at  these  places  being  actually  clf  ...,  cpt  which  are  so  situated  that 
the  determinant 


wherein  fa(r}  is  the  value  of  fa  (z,  s)  at  the  place  cr,  does  not  vanish.     That  it 

is  always  possible  to  choose  such  p  places  is  clear  :  for  if  vlt ,  vp  denote  a 

*  Chap.  III.  §  37. 


76  ACTUAL   EXPRESSION   OF   RATIONAL  [49 

set  of  independent  integrals  of  the  first  kind,  the  vanishing  of  A  expresses 
the  condition  that  a  rational  function  of  the  form 


involving  only  p  —  1  disposeable  ratios  \l:\2:  ......  :  \p,  vanishes  at  each  of 

the  places  C1}  ......  ,  cp. 

Choose  the  p  coefficients  in  the  function  f'(s)dP/dz,  so  that  this  function 
vanishes  at  clt  ......  ,  cp  :  and  denote  the  function  dP/dz,  with  these  coeffi 

cients,  by  ty  (a,  a;  z,^,  ......  ,  cp),  so  that  A/'(s)  \Jr  (a,  a  ;  z,  cx  ......  cp)  is  equal 

to  the  determinant 

[z,  x\  -  [z,  a],     $!  (z,  s\  £</>!  (z,  s),  ...,  z*-1  ^  (z,  s),  ...,  zTn-rl  fa^  (z,  s) 


where  [^,  *•]  denotes  the  expression 

<£o  (z,  s)  +  <fti  (z,  s)  g1(a:,y)  +  ...+  $n-i  (z,  s)  g!  (a,  y) 

Z  —  X 

Suppose  now  that  (z,  s)  is  a  finite  place,  not  a  branch  place,  such  that 
none  of  the  minors  of  the   elements  of  the  first  row  of  this   determinant 
vanish.     Consider   -v|r  (x,  a  ;   z,  Cj  ,  ......  ,  cp)   as   a  function  of  (x,  y).     It   is 

clearly  a  rational  function  ;  and  is  in  fact  rationally  expressed  in  terms  of  all 
the  quantities  involved.     It  is  infinite  at  each  of  the  places  z,  cu  c2,  ......  ,  cp  — 

and  in  fact  as  x  approaches  z,  the  limit  of  (z  —  x)  ty  (x,  a  ;  z,  cl}  ......  ,  c^,)  is 

the  same  as  that  of 

0o  (z,  s}  +  ^<j)r  (z,  s)  gr  (ay/) 

/'(*) 

namely,  unity  (§  44,  F)  :  so  that  at  x  =  z,  ty  is  infinite  like  —  (x  —  z}~1.     And 
at  GI,  .  ..,  Cp  it  is  similarly  seen  to  be  infinite  to  the  first  order. 

To  obtain   its  behaviour  when  x  is  at  infinity,  we  notice  that,  by  the 
definition  of  the  dimension  of  gi  (x,  y),  the  expression 

(x,  y)          .       .[I      z  zri~l  1 

-     -•+  -r~  ' 

xri  J 


z  —  x  \_x     x 

which  is  of  the  form 

Zri 


T.+Z        ~\ 

V+... 

x2 


is  finite  for  infinite  values  of  x.  If  then  we  add  to  the  first  column  of  the 
determinant  which  expresses  the  value  of  A/'  (s)  -\Jr  (x,  a  ;  z,  clf  ...,  cp),  the 
following  multiples  of  the  succeeding  p  columns 

g^y)     ffi  (a,  6)    frfoy)     9-2  (a,  b)  ,_  ,_,   „  , 

~~      --- 


49]  FUNCTION   WITH  p  -f  1    ARBITRARY    POLES.  77 

the  determinant  will  contain  only  quantities  which  remain  finite  for  infinite 
values  of  x. 

On  the  whole  then,  as  the  reader   can    now  immediately  see,  we  can 
summarise  the  result  as  follows. 

•ty  (x,  a  ;  z,clt  ......  ,  cp)  is  a  rational  function  of  x,  having  only  p  +  1  poles, 

each  of  the  first  order,  namely  z,  cl  ,  ......  ,  cp.     It  is  infinite  at  z  like  —  (x  —  z)~l 

and  it  vanishes  at  x  =  a. 

It  is  immediately  seen  that  if  a  function  of  x  of  the  form 


.. 

which  is  so  chosen  that  it  is  zero  at  all  of  ct,  ...,  cp  except  Cj  and  is  unity  at 

Ci,  be  denoted  by  wi  (x),  then  -Jr  (x,  a;  z,  cl  ...  c«)  is  infinite  at  CL  like  ***  ^  . 

x  -  Ci 

Let  now  R  (x,  y)  be  a  rational  function  of  (x,  y)  with  poles  at  the  finite 
ordinary  places  z1}  z2,  ...,  ZQ:  let  its  manner  of  infinity  at  z.-t  be  the  same  as 
that  of  —  \i{x  —  Zi)~\  Then  the  function 

R  (x,  y)-\l^(x,a:  zlt  clt  ...,cp)-...-\Q^(x,  a;  zv,  clt  ...,  cp) 

is  a  rational  function  of  (x,  y)  which  is  only  infinite  at  clf  ...,  cp.  Since 
however  these  latter  places  are  independent*,  no  such  function  exists  —  nor 
does  there  exist  a  rational  function  infinite  only  in  places  falling  among 
c1}  ...,  cp.  Hence  the  function  just  formed  is  a  constant;  thus 

R(x,  y)  =  \l^(x,  a;  zl}  c,,  ...,  cp)  +...+  \Q^(x,  a;  ZQ,  c,,  ...,cp)  +  \. 
Conversely  an  expression  such  as  that  on  the  right  hand  here  will  represent 
a  rational  function  having  zlt  ...,  ZQ  for  poles,  for  all  values  of  the  coefficients 
\i,  ...,  \Q,  \,  which  satisfy  the  conditions  necessary  that  this  expression  be 
finite  at  each  of  cl}  ...,  cp;  these  conditions  are  expressed  by  the  p  equations 

*i  *>i  (z,)  +  \,a>i  (z2)  +.  ..+  Xy  a)i  (ZQ)  =  0, 
where  i  =  1,  2,  ...,  p. 

When  these  conditions  are  independent  the  function  contains  therefore 

Q-p+l 

arbitrary  constants—  in  accordance  with  the  result  previously  enunciated 
(Chapter  III.  §  37).  The  excess  arising  when  these  conditions  are  not  inde 
pendent  is  immediately  seen  to  be  also  expressible  in  the  same  way  as  before. 

We  thus  obtain  the  Riemann-Roch  Theorem  for  the  case  under  con 
sideration. 

The  function  -^  (x,  a  ;  z,  c,,  ...,  cp)  will  sometimes  be  called  Weierstrass's 
function.     The  modification  in  the  expression  of  it  which  is  necessary  when 
*  In  the  sense  employed  Chapter  III.  §  23, 


78  ALGEBRAICAL    DEDUCTION   OF   THE   RESULTS  [49 

some  of  its  poles  are  branch  points,  will  appear  in  a  subsequent  utilization 
of  the  function  (Chapter  VII.*).  The  modification  necessary  when  some  of 
these  poles  are  at  infinity  is  to  be  obtained,  conformably  with  §  39  of  the 
present  chapter  by  means  of  the  transformation  x  =  (%  —  m)~l,  whereby  the 
place  a;  =  oo  becomes  a  finite  place  £  =  m. 

50.  The  theory  contained  in  this  Chapter  can  be  developed  in  a  different 
order,  on  an  algebraical  basis. 

Let  the  equation  of  the  surface  be  put  into  such  a  form  as 

wherein  alt  ...,  an  are  integral  polynomials  in  x:  so  that  y  is  an  integral 
function  of  x. 

By  algebraical  methods  only  it  can  be  shewn  that  a  set  of  integral 
functions  glt  ...,  gn_^  exists  having  the  property  that  every  integral  function 
can  be  expressed  by  them  in  a  form 

(x,  l)A  +  (#,  1)A[  #i+...+  (#,  I)A»-I  gn-i, 

in  such  a  way  that  no  term  occurs  in  the  expression  which  is  of  higher 
dimension  than  the  function  to  be  expressed;  and  that  the  sum  of  the 
dimensions  of  gl}  ...,  gn-i  is  not  less  than  n—l  but  is  less  than  that  of  any 
other  set  (1,  hlt  ...,  hn-i),  in  terms  of  which  all  integral  functions  can  be 
expressed  in  such  a  form  as 

If  the  sum  of  the  dimensions  of  gl}  ...,  gn_^  be  then  written  in  the  form 
p  +  n  —  1,  p  is  called  the  deficiency  of  the  fundamental  algebraic  equation. 

The  expressions  of  the  functions  gl}  g2,  ...,  gn-l  being  once  obtained, 
and  the  forms  <£0,  ^>15  ...,<£„_!  thence  deduced  as  in  this  Chapter,  the  integrals 
of  the  first  kind  can  be  shewn,  as  in  this  Chapter  or  otherwise^,  to  have  the 
form 

d®      17       i  w  -i    •  \  ,       _ 


/'(y) 

wherein  r\  <  rlt  etc.,  T;  +  1  being  the  dimension  of  g{.     Thus  the  number 

of  terms  which  enter  is  at  most  TJ  + +  rn_i  or  p.     But  it  can  in  fact  be 

shewn  algebraically  that  every  one  of  these  terms  is  an  integral  of  the  first 
kind,  namely,  that  an  integral  of  the  form 


is  everywhere  finite^  provided  0  ^r  ^Tt-  —  1. 

*  The  reader  may,  with  advantage,  consult  the  early  parts  (e.g.  §§  122,  130)  of  that  chapter  at 
the  present  stage. 

t  Hensel,  Crelle,  109. 

+  For  this  we  may  use  the  definition  (G)  or  the  definition  (H)  (§  44).  The  reader  may 
refer  to  Hensel,  Crelle,  105,  p.  336. 


50]  OF   THIS   CHAPTER.  79 

Then  the  forms  of  the  integrals  of  the  second  and  third  kind  will  follow 
as  in  this  Chapter:  and  an  algebraic  theory  of  the  expression  of  rational 
functions  of  given  poles  can  be  built  up  on  the  lines  indicated  in  the 
previous  article  (§  49)  of  this  Chapter.  In  this  respect  Chapter  VII.  may  be 
regarded  as  a  continuation  of  the  present  Chapter. 

A  method  for  realising  the  expressions  of  glt  ...,  <7n_j  for  a  given  form  of 
fundamental  equation  is  explained  in  Chapter  V.  (§  73). 

For  Kronecker's  determination  of  a  fundamental  set  of  integral  functions, 
for  which  however  the  sum  of  the  dimensions  is  not  necessarily  so  small  as 
p  +  n  —  1,  the  reader  may  refer  to  the  account  given  in  Harkness  and 
Morley,  Theory  of  Functions,  p.  262.  It  is  one  of  the  points  of  interest  of  the 
system  here  adopted  that  the  method  of  obtaining  them  furnishes  an  algebraic 
determination  of  the  deficiency  of  the  surface. 


CHAPTER  V. 

ON  CERTAIN  FORMS  OF  THE  FUNDAMENTAL  EQUATION  OF  THE  RlEMANN 

SURFACE. 

51.  WE  have  already  noticed  that  the  Riemarm  surface  can  be  expressed 
in  many  different  ways,  according  to  the  rational  functions  used  as  variables. 
In  the  present  chapter  we  deal  with  three  cases  :  the  first,  the  hyperelliptic 
case  (§§  51 — 59),  is  a  special  case,  and  is  characterised  by  the  existence  of  a 
rational    function  of  the  second  order ;   the   second,   which  we  shall  often 
describe  as  that  of  Weierstrass's  canonical  surface  (§§  60 — 68),  is  a  general 
case  obtained  by  choosing,  as  independent  variables,  two  rational  functions 
whose    poles  are  at  one  place  of  the  surface  :    the  third  case   referred  to 
(§§  69 — 71)  is  also  a  general  case,  which  may  be  regarded  as  a  generalization 
of  the  second  case.     It  will  be  seen  that  both  the  second  and  third  cases 
involve  ideas  which  are  in  close  connexion  with  those  of  the  previous  chapter. 
The  chapter  concludes  with  an  account  of  a  method  for  obtaining  the  funda 
mental  integral  functions  for  any  fundamental  algebraic  equation  whatever 
($|  73—79). 

It  may  be  stated  for  the  guidance  of  the  reader  that  the  results  obtained  for  the 
second  and  third  cases  (§§  60 — 71)  are  not  a  necessary  preliminary  to  the  theory  of  the 
remainder  of  the  book  ;  but  they  will  be  found  to  furnish  useful  examples  of  the  actual 
application  of  the  theory. 

52.  We  have  seen  that  when  p  is  greater  than  zero,  no  rational  function 
of  the  first  order  exists.     We  consider  now  the  consequences  of  the  hypothesis 
of  the  existence  of  a  rational  function  of  the  second  order.     Let  £  denote 
such  a  function  ;  let  c  be  any  constant  and  a,  ft  denote  the  two  places  where 
£=c,  so  that  (f  —  c)'1  is  a  rational  function  of  the  second  order  with  poles 
at  a,  /3.     The  places  a,  /3  cannot  coincide  for  all  values  of  c,  because  the 
rational  function  d^/dx  has  only  a  finite  number  of  zeros.     We  may  therefore 
regard  a,  /3  as  distinct  places,  in  general.     The  most  general  rational  function 
which  has  simple  poles  at  a,  J3  cannot  contain  more  than  two  linearly  entering 
arbitrary  constants.     For  if  such  a  function  be  \  +  \ifi  +  X.2/2  +  •  •  •  >  ^->  ^-i> 
being  arbitrary  constants,   each  of  the  functions  f1}  f.2, ...    must  be  of  the 
second  order  at  most  and  therefore  actually  of  the  second  order :  by  choosing 
the  constants  so  that  the  sum  of  the  residues  at  a  is  zero,  we  can  therefore 


53]  THE    HYPERELLIPTIC   CASE.  81 

obtain  a  function  infinite  only  at  ft,  which  is  impossible*.  Thus  the  most 
general  rational  function  having  simple  poles  at  a,  ft  is  of  the  form 
-^  (£  -  c)"1  +  B.  Therefore,  from  the  Riemann-Roch  Theorem  (Chapter  III., 
§  37),  Q-q=p-(r  +  I),  putting  Q  =  2,  q  =  1,  we  obtain  £>-(T  +  !)  =  !; 
namely,  the  number  of  linearly  independent  linear  aggregates 

ft  (x)  =  Xxfl,  («)+...+  Xpftp  («), 

which  vanish  in  the  two  places  a,  /?  is  p  -  1.  Since  a  may  be  taken  arbitrarily 
and  c  determined  from  it,  and  p  —  I  is  the  number  of  these  linear  aggregates 
which  vanish  in  an  arbitrary  place,  we  have  therefore  the  result  —  When  there 
exists  a  function  of  the  second  order,  every  place  a  of  the  surface  determines 
another  place  ft:  and  the  determination  may  be  expressed  by  the  statement 
that  every  linearly  independent  linear  aggregate  ft  (x)  which  vanishes  in 
one  of  these  places  vanishes  necessarily  in  the  other. 

53.  Conversely  when  there  are  two  places  a,  ft  in  which  p  —  1  linearly 
independent  ft  (x)  aggregates  vanish,  there  exists  a  rational  function  having 
these  two  places  for  simple  poles.  To  see  this  we  may  employ  the  formula 
of  §  37,  putting  Q  =  2,  r  +  l=p-l,  and  obtaining  q=l.  Or  we  may 
repeat  the  argument  upon  which  that  result  is  founded,  thus  —  Not  every 
one  of  ftj  (x),  .  .  .  ,  ftp  (x)  can  vanish  at  a  ;  let  ft,  (a)  be  other  than  zero.  Since 
p  -  1  linearly  independent  ft  (x)  aggregates  vanish  in  a,  and,  by  hypothesis, 
p  -  1  linearly  independent  ft  (x)  aggregates  vanish  in  both  a  and  ft,  it 
follows  that  every  ft  (x)  aggregate  which  vanishes  in  a  vanishes  also  in  ft. 
Hence  each  of  the  p  —  1  aggregates 

ft2  (a)  ft,  (x)  -  ft,  (a)  ft2  (x),  ......  ,  flp  (a)  flx  (x)  -  ftx  (a)  ftp  (a), 

vanishes  in  ft,  namely,  we  have  the  p  —  1  equations 

fti(«)ft1(^)-ft1(a)fti(/3)  =  0,     (i  =  2,  3,...,p). 
Therefore  the  function 


has  each  of  its  periods  zero.  Thus  it  is  a  rational  function  whose  poles  are  at 
a  and  ft  :  and  ft,  (/3)  cannot  be  zero  since  otherwise  the  function  would  be  of 
the  first  order. 

Hence  when  there  are  two  places  at  which  p  —  1  linearly  independent 
ft(#)  aggregates  vanish,  there  is  an  infinite  number  of  pairs  of  places  having 
the  same  character.  For  any  pair  of  places  the  relation  is  reciprocal,  namely, 
if  the  place  a  determine  the  place  ft,  a.  is  the  place  which  is  similarly 
determined  by  ft  :  in  other  words,  the  surface  has  a  reciprocal  (1,  1)  corre 
spondence  with  itself.  It  can  be  shewn  by  such  reasoning  as  is  employed  in 

*  By  the  equation  Q  -  q  =p  -(T  +  1),  if  q  were  2,  r  +  1  would  be  p,  or  all  linear  aggregates  Q(x) 
would  vanish  in  the  same  places,  which  is  impossible  (Chap.  II.  §  21). 

B.  C 


82  THE   HYPERELLIPTIC   CASE.  [53 

Chap.  I.  (p.  5),  that  if  (xl}  y^),  (x2,  y2)  be  the  values  of  the  fundamental 
variables  of  the  surface  at  such  a  pair  of  places,  each  of  #j  ,  ^  is  a  rational 
function  of  xz  and  ?/2,  and  that  conversely  x2,  y2  are  the  same  rational 
functions  of  xl  and  y^ 

54.  We  proceed  to  obtain  other  consequences  of  the  existence  of  a  rational 
function,  g,  of  the  second  order.  If  the  poles  of  £  do  not  fall  at  finite  distinct 
ordinary  places  of  the  surface,  choose  a  function  of  the  form  (£  —  c)"1,  in 
accordance  with  the  explanation  given,  for  which  the  poles  are  so  situated. 
Denote  this  function  by  2.  Then*  the  function  dz/dx  has  2.2  +  2p—  2  =  2p  +  2 
zeros  at  each  of  which  z  is  finite.  Denote  their  positions  by  xly  x2,  ...,  ^+2- 
If  these  are  not  all  finite  places  we  may,  if  we  wish,  suppose  that,  instead  of 
x,  such  a  linear  function  of  x  is  taken  that  each  of  xl}  ...  ,  x2p+2  becomes 
a  finite  place.  They  are  distinct  places.  For  if  the  value  of  z  at  X{  be  Cf, 
z  —  d  is  there  zero  to  the  second  order  :  that  another  place  x-}  should  fall  at 
Xi  would  mean  that  z  —  c;  is  there  zero  to  higher  than  the  second  order, 
which  is  impossible  because  z  is  only  of  the  second  order.  By  the  expla 
nations  previously  given  it  follows  that  a  linear  aggregate  H  (#),  which 
vanishes  at  any  one  of  these  places  x1}  ...  ,  xw+2,  vanishes  to  the  second  order 
there.  Hence  there  is  no  linear  aggregate  II  (x)  vanishing  at  p  or  any 
greater  number  of  these  places,  for  H  (x)  has  only  2p  —  2  zeros.  The  general 
rational  function  which  has  infinities  of  the  first  order  at  the  places  xl,...t  xp+r 
will  therefore  f  contain  a  number  of  q  +  1  of  constants  given  by  p  +  r  —  q  =  p, 
namely,  will  contain  r  +  1  constants.  Such  a  function  will  therefore  not 
exist  when  r  =  0.  In  order  to  prove  that  a  function  actually  infinite  in  the 
prescribed  way  does  exist  for  all  values  of  r  greater  than  zero,  it  is  sufficient, 
in  accordance  with  §§  23  —  27  (Chap.  III.),  to  shew  that  there  exists  no 
rational  function  having  xly  x2,  ...  ,  #f  for  poles  of  the  first  order  for  any 
value  of  i  less  than  p  +  1.  Without  stopping  to  prove  this  fact,  which  will 
appear  a  posteriori,  we  shall  suppose  r  chosen  so  that  a  function  of  the 
prescribed  character  actually  exists.  For  this  it  is  certainly  sufficient  that  r 
be  as  great  as  p  j.  Denote  the  function  by  h,  so  that  h  has  the  form 


\,\lt...,\r  being  arbitrary  constants. 

Let  h,  h'  denote  the  values  of  h  at  the  two  places  (x,  y),  (xr,  y'\  where 
z  has  the  same  value.  Then  to  each  value  of  z  corresponds  one  and  only  one 
value  of  h  +  h',  or  h  +  h'  may  be  regarded  as  an  uniform  function  of  z  :  the 
infinities  of  h  +  h'  are  clearly  of  finite  order,  so  that  h  +  ti  is  a  rational 
function  of  z.  Consider  now  the  function  (z  -  Cj)  (z  -  C2)  .  .  .  (z  -  cp+r)  (h  +  h'). 


*  Chap.  I.  §  6. 
t  Chap.  III.  §  37. 

£  Chap.  III.  §  27.    For  the  need  of  the  considerations  here  introduced  compare  §  37  of 
Chap.  III. 


55]  DEDUCTION    OF   CANONICAL   EQUATION.  83 

Since  h  and  h'  are  only  infinite  at  places  of  the  original  surface  at  which 
z  is  equal  to  one  or  other  of  c1(  ...,  cp+r,  this  function  is  only  infinite  for 
infinite  values  of  z.  As  it  is  a  rational  function  of  z,  it  must  therefore  be  a 
polynomial  in  z  of  order  not  greater  than  p  +  r.  Hence  we  may  write 

h  +  k'=  (Z,    \}p+rl(z  -  Cj)  ...  (Z  -  Cp+r). 

But  here  the  left  hand  is  only  infinite  to  the  first  order,  at  most,  at  any 
one  of  d,  ...,  Cp+r  —  and  the  denominator  of  the  right  hand  is  zero  to  the 
second  order  at  such  a  place.  Hence  the  numerator  of  the  right  hand  must 
be  zero  at  each  of  these  places,  and  must  therefore  be  divisible  by  the 
denominator.  Thus  h  +  h'  is  an  absolute  constant,  =  20  say.  From  the 
equations 

h  = 


we  infer  then  that  S;  +  S'f  is  also  a  constant,  =  2(7;  say  :  for  h  was  chosen  to 
be  the  most  general  function  of  its  assigned  character  and  the  coefficients 
X,  ....  \r  are  arbitrary.  Thence  we  obtain 

G  =  \  +  \C1  +  ...  +\Cr. 
We  can  therefore  put 


so  that  s  will  be  a  function  of  the  same  general  character  as  h,  such  however 
that  s  +  s'  =  0  :  in  its  expression  the  constants  \i  ,  .  .  .  ,  \r  are  arbitrary,  while 
the  constants  Clf  ...,  Cr  depend  on  the  choice  made  for  the  functions 
S  ? 

•^l»  •••>  ^r- 

55.  Consider  now  the  two  places  a,  a?  at  which  z  is  infinite.  Choose  the 
ratios  \  :  X2  :  ...  :  \r  so  that  s  is  zero  to  the  (r  —  l)th  order  at  a.  This  can 
always  be  done,  and  will  define  s  precisely  save  for  a  constant  multiplier, 
unless  it  is  the  case  that  when  s  is  made  to  vanish  to  the  (r  —  l)th  order 
at  a,  it  vanishes,  of  itself,  to  a  higher  order.  In  order  to  provide  for  this 
possibility,  let  us  assume  that  s  vanishes  to  the  (r  —  I  +  &)th  order  at  a. 
Since  s'  =  —  s,  s  will  also  vanish  to  the  (r  —  l+  &)th  order  at  «'.  There  will 
then  be  other  p  +  r  -  2  (r  -  1  +  k),  or  p  -  r  +  2  -  k,  zeros  of  s.  From  the 
manner  of  formation  this  number  is  certainly  not  negative.  Consider  now 
the  function 

f=(z-cj)...(z-cp+r)s?. 

At  the  places  where  z  is  infinite  /  is  infinite  of  order  p  +  r  —  2  (r  —  1  +  k), 
or  p  -  r  +  2  -  2k  times.  At  the  places,  xlt  ...,  xp+r  where  s  is  infinite,  it  is 
finite;  each  of  the  factors  z  -  clt  ...,  z  -  cp+r  is  zero  to  the  second  order  at 
the  place  where  it  vanishes.  Since  s2  =  -  ss',  f  is  a  symmetrical  function  of 
the  values  which  s  takes  at  the  places  where  z  has  any  prescribed  value. 
Hence,  by  such  reasoning  as  is  previously  employed,  it  follows  that  the  func- 

6—2 


84  CANONICAL   EQUATION.  [oo 

tion  f  is  a  rational  integral  polynomial  in  z  of  order  p  —  r  +  2  —  2k.  Denote 
this  polynomial  by  H.  By  consideration  of  the  zeros  of/  it  follows  that  the 
2  (p  —  r  +  2  —  2k)  zeros  of  the  polynomial  H  are  the  zeros  of  s2  which  do  not 
fall  at  a  or  a'.  But  since  the  sum  of  the  values  of  s  at  the  two  places  where 
z  has  any  prescribed  value  is  zero,  it  follows  that  s  is  zero  at  each  of  the 
places  Xp+r+i,  '••,  #2p+2-  For  each  of  these  is  formed  by  a  coalescence  of  two 
places  where  z  has  the  same  value,  and  at  each  of  them  s  is  not  infinite. 
Hence  the  polynomial  H  must  be  divisible  by  (z  —  cp+r+1)  ...  (z  —  0^+2). 
Thus,  as  H  is  a  polynomial  of  order  p  —  r  +  2  —  2k  in  z,  p  —  r  +  2  —  2k  must 
be  at  least  equal  to  2p  +  2  —  (p  +  ?•)  or  to  p  —  r  +  2.  Hence  k  is  zero,  and 
the  value  of  H  is  determinate  save  for  a  constant  multiplier.  Supposing 
this  multiplier  absorbed  in  s  we  may  therefore  write 

(z-c1)...(z-  cp+r)  s*  =  (2-  cp+r+1)  ...(z-  Cop+2)  (A) ; 

and  s  is  determined  uniquely  by  the  conditions,  (1)  of  being  once  infinite  at 
xly  ...,  xpJfr,  (2)  of  being  (?•  —  1)  times  zero  at  each  of  the  places  a,  a'  where  z 
is  infinite.  Denote  s,  now,  by  sp+r,  and  denote  the  function  h  from  which  we 
started,  which  was  defined  by  the  condition  of  being  once  infinite  at  each  of 
a?!,  ...,  Xp+r,  by  hp+r,  and  consider  the  function  (z  —  cp+r)sp+r.  This  function 
is  once  infinite  at  each  of  x1}  ...,  xp+r_l}  it  is  zero  to  the  first  order  at  xp+r, 
and  it  is  r—  1  —  1,  =  r  -  2  times  zero  at  each  of  the  places  a,  a'  where  z  is 
infinite.  Hence  the  function 

(z  -  cp+r)  sp+r  (A  +  AjZ  +  ...+  Ar_2 2r~2)  +  B, 

wherein  B,  A,  Aly  ...,  Ar_2  are  arbitrary  constants,  has  the  property  of  being 
once  infinite  at  each  of  xl}  ...,  xp+r_lt  and  not  elsewhere.  It  is  then  exactly 
such  a  function  as  would  be  denoted,  in  the  notation  suggested,  by  hp+r-1} 
and  it  contains  the  appropriate  number  of  arbitrary  constants — and  we  can 
from  it  obtain  a  function  sp+r_lt  having  the  property  of  being  once  infinite  at 
each  of  x1}  ...,  xpJrr_^  and  vanishing  (r  —  2)  times  at  each  of  the  places  a,  a' 
where  z  is  infinite. 

Ex.  1.     Determine  sp  +  r_1  in  accordance  with  this  suggestion. 

Ex.  2.     Prove  that  hp  +  r  is  of  the  form  sp  +  r  (A  +  A ^  + . . .  +  A r  _  ^  ~ !)  +  B. 

Ex.*.     Prove  that  Ap  +  ,  +  4  is  of  the  form   s^r(A+A,z+     +Ar  +  t_l2^^^  +  R 

(*-Vtr+i)*»(*-Vfcr+t) 

Ex.  4.     Shew  that  the  square  root       /(*-cj>+r  +  1)...(s-c2p  +  2)  ^  ^  interpreted  as  an 

V          (z~ci)-"(z~cp  +  r) 

one-valued  function  on  the  original  surface. 

56.  The  functions,  z,  sp+r  are  defined  as  rational  functions  of  the  x,  y 
of  the  original  surface.  Conversely  x,  y  are  rational  functions  of  z,  sp+r. 
For*  we  have  found  a  rational  irreducible  equation  (A)  connecting  z  and 

*  See  Chap.  I.  §  4. 


56]  FUNDAMENTAL   INTEGRAL   FUNCTIONS.  85 

sp+r  wherein  the  highest  power  of  sp+r  is  the  same  as  the  order  of  z.  Hence 
this  equation  (A  )  gives  rise  to  a  new  surface,  of  two  sheets,  with  branch  places 
at  z  =  c1>...,  Czp+2,  whereon  the  original  surface  is  rationally  and  reversibly 
represented. 

It  is  therefore  of  interest  to  obtain  the  forms  of  the  fundamental  integral 
functions  and  the  forms  of  the  various  Riemann  integrals  for  this  new  surface. 
It  is  clear  that  the  function 

(Z  -  C,)  .  .  .  (Z  -  Cp+r)  Sp+r  0,    l)*_i  , 

where  k  is  a  positive  integer,  and  (z,  \)k-\  denotes  any  polynomial  of  order 
k—l,  is  infinite  only  at  the  places  a,  a'  where  z  is  infinite,  and  in  fact 
to  order  p  +  r  —  (r—  l)  +  k  —  l,  =  p  +  k:  and  that,  therefore,  by  suitable  choice 
of  the  coefficients  in  another  polynomial  (z,  l)p+fc,  we  can  find  a  rational 
function 

(z  -  d)  ...  (z  -  cp+r)  Sp+r  (z,  !)*_!  +  (z,  l)p+k, 

which  is  not  infinite  at  a',  and  is  infinite  at  a  to  any  order,  p  +  k,  greater 
than  p.  Now,  of  rational  functions  which  are  infinite  only  at  a,  there  are  p 
orders  for  which  the  function  does  not  exist*.  Hence  these  must  be  the 
orders  1,  2,  ...  ,  p. 

Hence,  of  functions  infinite  only  in  one  sheet  at  z  =  oo  ,  on  the  surface 

(Z  -  d)  ...  (Z  -  Cp+r)  Szp+r  =  (z  -  Cp+r+i)  ...(z-  C^+a), 

that  of  lowest  order  is  a  function  of  the  form 


which  becomes  infinite  to  the  (p  +  l)th  order.  Hence  by  Chapter  IV.  §  39, 
every  rational  function  which  becomes  infinite  only  at  the  places  z  =  oo  ,  can 
be  expressed  in  the  form 

(z,  1)X-K*,  1V*7, 

and  if  the  dimension  of  the  function,  namely,  the  number  which  is  the  order 
of  its  higher  infinity  at  these  places,  be  p  +  1,  X  and  fi  are  such  that 

p  +  1  >  X,  p  +  l>  ft  +p  +  1. 

Therefore  also,  if  er  =  (z  —  cx)  .  .  .  (z  —  cp+r)  sp+r  =  t)  —  (z,  1  )p+1  ,  in  which  case 
equation  (A)  may  be  replaced  by  the  equation 

<f*=(z-  d)  (z  -  c,)  ...(z-  c2p+2), 
we  have  the  result  that  all  such  functions  can  be  also  expressed  in  the  form 

(z,  l)v  +  (.s,  I),  <r, 
with 


Chap.  III.  §  28. 


86  EXAMPLES.  [56 

By  means  of  this  result,  hitherto  assumed,  the  forms  for  the  various 
integrals  given  Chapter  II.,  §  17,  Chapter  IV.,  §  46,  are  immediately 
obtainable  by  the  methods  of  Chapter  IV. 

57.  Or  we  can  obtain  the  forms  of  the  integrals  of  the  first  kind  thus — 
Let  v  be  such  an  integral.  Consider  the  rational  function 

,          .       ,  .dv 

8p+r(z-c1)...(z-cp+r)fa. 

It  can  only  be  infinite  (1)  where  z  is  infinite  (2)  where  dz  =  0,  that  is  at 
the  branch  places  of  the  (sp+r,  z)  surface.  It  is  immediately  seen  that  the 
latter  possibility  does  not  arise.  Where  z  is  infinite  the  function  is  infinite 
to  the  order  p  +  1  —  2,  or  p—  1.  Hence  it  is  an  integral  polynomial  in  z  of 
order  p  —  l.  Namely,  the  general  integral  of  the  first  kind*  is 

/•  (z,  \)p-ldz 

58.  Ex.  1.  A  rational  function  hp_k,  infinite  only  at  the  places  where  z  =  cl,  ...,  cp_t, 
contains  p-k-p  +  r  +  l  +l  =  r+2-£  arbitrary  constants,  where  T  +  !  is  the  number  of 
coefficients  in  a  general  polynomial  (z,  l)p-i  which  remain  arbitrary  after  the  prescription 
that  (z,  !)„_!  shall  vanish  at  c1}  ...,  cp_t.  Prove  this:  and  infer  that  Ap,  Ap_1,...do  not 
exist. 

Ex.  2.     It  can  be  shewn  as  in  §  57  that  at  any  ordinary  place  of  the  surface 


rational  functions  exist,  infinite  only  there,  of  orders  p  +  l,  p  +  2,  ...:  the  gaps  indicated  by 
Weierstrass's  theorem  (Chapter  III.  §  28)  come  therefore  at  the  orders  1,  2,  ...,p.  At  a 
branch  place,  say  at  z  =  c,  the  gaps  occur  for  the  orders  1,  3,  5,  ...,  (2p-  1).  For,  all  other 
possible  orders,  which  a  rational  function,  infinite  only  there,  can  have,  are  expressible  in 
one  of  the  forms  2(p-k),  2p  +  2r+l,  2p  +  2r,  where  k  is  a  positive  integer  less  than  p,  or 
zero,  and  r  is  a  positive  integer:  and  we  can  immediately  put  down  rational  functions 
infinite  to  these  orders  at  the  branch  place  z=c  and  nowhere  else  infinite.  Prove  in  fact 
that  the  following  functions  have  the  respective  characters 

fe  *)?-*     fa  l)ro-  +  (g-c)fo  l)p  +  r     (z,  l)p  +  r 


wherein  (z,  !),,_*,  (z,  l)r,  (z,  l)p  +  r  are  polynomials  of  the  orders  indicated  by  their  suffixes 
with  arbitrary  coefficients. 

Shew  further  that  the  most  general  Q(:c)  aggregate  which  vanishes  2p-2k  times  at  the 
branch  place  contains  k  arbitrary  coefficients:  and  infer  that  the  expressions  given 
represent  the  most  general  functions  of  the  prescribed  character  (see  Chapter  III.  §  37). 

Ex.  3.     Prove  for  the  surface 

Ax*  +  Rvy  +  Cy*  +  Pa?  +  Qtfy+Rxy* 
that  the  function 


Cf.  the  forms  quoted  from  Weierstrass.     Forsyth,  Theory  of  Functions,  p.  456, 


59]  IRREMOVEABLE   CONSTANTS   OF  THE  SURFACE.  87 

wherein  X  and  /*  are  arbitrary  constants,  is  of  the  second  order.  And  that  there  are  six 
values  of  z  for  which  the  pairs  of  places  at  which  z  takes  the  same  value,  coincide,  these 
places  of  coincidence  being  zeros  of  the  function 

2  (A  x*  +  Bxy  +  Cf)  +  Px3  +  Q^y  +  Rxy*  +  Sy3. 
Prove  further  that  a  rational  function  which  is  infinite  at  these  six  places  is  given  by 

_  2  (  Ax*  +  Bxy  +  Cy*)  +  P'x3  +  QWy  +  R'xy*  +  S'y3 

~ 


for  arbitrary  values  of  the  constants  P',  Q',  R',  S'. 

This  function  is,  therefore,  such  a  function  as  has  been  here  called  hp  +  r  :  and  since  there 
are  six  places  at  which  dz  is  zero,  p  is  equal  to  2  and  r  equal  to  4. 

Prove  that  the  sum  of  the  values  of  h  at  the  two  places  other  than  (0,  0)  at  which  z  has 
the  same  value  is  constant  and  equal  to  2. 

We  may  then  proceed  as  in  the  text  and  obtain  the  transformed  surface  in  the  simple 
hyperelliptic  form.  But  a  simpler  process  in  practice  is  to  form  the  equation  connecting 
z  and  h.  Writing  k  =  h—\  and  Z=xjy,  prove  that 

P  {(PZ3  +  QZ*  +  RZ+  ,S02  -  4  (  AZ*  +  BZ+  C)  (a^  +  a^Z3  +  a^  +  a3Z+  a4)} 

=  {(P  -  P)  Z3  +  ((?  -  Q)  Z*  +  (R'-  R)  Z+  (S1  -  £)}*. 

Hence,  if  the  coefficient  of  k2  on  the  left  be  written  (Z,  1)6,  and  we  write 
Y=  [(P'  -  P)  Z3  +  (Q'-Q)Z*  +  (R'  -  R)  Z+  (S'  - 

=  [2  (A  x*  +  Bxy  +  Cy*}  +  Px3  +  Qa?y  +  Rxy* 
we  have 

Y*  =  (Z,  l)e, 

which  is  the  equation  of  the  transformed  surface.  And,  as  remarked  in  the  text,  the 
transformation  is  reversible  ;  verify  in  fact  that  #,  y  are  given  by 

x=2Z(AZ2  +  BZ+  C)/[  r-  (PZ3  +  QZ*  +  RZ+  £)], 
y  =  2  (AZ*  +  BZ+  <7)/[  Y-  (PZ3  +  QZ*  +  RZ+  S)]. 

Hence  any  theorem  referred  to  one  form  of  equation  can  be  immediately  transformed  so 
as  to  refer  to  the  other  form. 

59.     The  equation 

o-2  =  (z  -  d)  (z  -  c2)  .  .  .  (z  -  c2p+2) 

by  which,  as  we  have  shewn,  any  hyperelliptic  surface  can  be  represented, 
contains  2^-1-2  constants,  namely  clt  C2,  .  .  .  ,  c^+2.  If  we  write  z  —  (ox  +  b)/(x  +  c) 
we  introduce  three  new  disposable  constants  ;  by  suitable  choice  of  these 
the  equation  of  the  surface  can  be  reduced  to  a  form  in  which  there  are  only 
2p  —  1  parametric  constants.  For  instance  if  we  put 

(Z  -  C,)  (C8  -  C2)/(>  -  C2)  (Ca  -  d)  =  XJ(x  -  1) 

and  then,  further, 

s=A<r(z-  c3)-P-\ 
where  the  constant  A  is  given  by 

A  =  (c,  -  c,)*  (c,  -  c,YI(c,  -  c2)*"H  (c,  -  c4)»  (GS  -  c5)i  .  .  .  (c3  -  (Vw)1, 


88  EXAMPLES.  [59 

the  equation  becomes 

s2  =  x  (x  -  1)  (oc  -  a,)  (x  -  as)  .  .  .  (x  -  o^+j). 
wherein 

ar  =  (cz  -  c3)  (cr  -  c^Kc,  -  c2)  (c3  -  cr\ 

and  the  right-hand  side  of  the  equation  is  now  a  polynomial  of  order  2p  +  1 
only.  Of  its  branch  places  three  are  now  at  x=0,  x=l,  #=oo,  and  the 
values  of  x  for  the  others  are  the  parametric  constants  upon  which  the 
equation  depends.  It  is  quite  clear  that  the  transformation  used  gives  s,  x 
as  rational  function  of  or,  z.  Thus 

The  hyperelliptic  su?face  depends  on  2p  —  1  moduli  only.  Among  the 
positions  of  the  3p  —  3  branch  places  upon  which  a  general  surface  depends 
(Chapter  I.  §  7),  there  are,  in  this  case,  3p  -3-(2p  -l)=p  -2  relations. 

Thus  a  surface  for  which  p  =  2  is  hyperelliptic  in  all  cases.  There  are  in 
fact  (p—l)p(p  +  l)  =  Q  places*  for  which  we  can  construct  a  rational 
function  of  order  2  infinite  only  at  the  place. 

A  surface  for  which  p  =  I  is  also  hyperelliptic  —  but  it  is  more  than  this 
(Chapter  I.  §  8),  being  susceptible  of  a  reversible  transformation  into  itself  in 
which  an  arbitrary  parameter  enters. 

Ex.  1.     On  the  surface  of  six  sheets  associated  with  the  equation 

y6  =  x  (  x  —  a)  (x  -  6)4 

there  are  four  branch  places,  one  at  (0,  0)  where  six  sheets  wind,  and  at  (a,  0)  where  six 
sheets  wind,  two  at  (b,  0)  at  each  of  which  three  sheets  wind.  These  count  f  in  all  as 

w  =  6 
Hence,  by  the  formula 

putting  n  =  6,  we  obtain  p  =  2. 

Thus  there  exists  a  rational  function  £  of  the  second  order,  and  the  surface  can  be 
reversibly  transformed  into  the  form  »?2  =  (£,  l)(i.     In  fact  the  function 


is  infinite  to  the  first  order  at  each  of  the  branch  places  (b,  0),  (a,  0)  and  is  not  elsewhere 
infinite. 

To  obtain  the  values  of  £  at  the  branch  places  of  the  new  surface,  we  may  express  either 
x  or  y  in  terms  of  £.  Since  there  are  two  places  at  which  £  takes  any  value,  each  of  x  and 
y  will  be  determined  from  £  by  a  quadratic  equation—  which  may  reduce  to  a  simple 
equation  in  particular  cases.  When  £  has  a  value  such  that  the  corresponding  two  places 
coincide,  each  of  these  quadratic  equations  will  have  a  repeated  root. 
Now  we  have 

(x-bf 
- 


Chap.  III.  §  31.  f  Forsyth,  Theory  of  Functions,  p.  349, 


59]  EXAMPLES  OF   HYPERELLIPTIC   EQUATIONS.  89 

Hence 

y2(£G_1)_y£5(a_  2&)  _&(«-&)  £4  =  0. 

The  condition  then  is 

P(«-26)2  +  46(«-6)£4(|«-l)  =  0,  or   |*  [a2  (£«  -  1  )  +  («  -  26)2]  =  0. 

The  factor 


is  equal  to 

[a2  {(x  -Vf-x  (x  -  a)}  +  (a  -  26)2  x  (x  -  a)]/#  (#  -  a), 

which  is  immediately  seen  to  be  the  same  as 

[x  (a  -  26)  +  ab]/x  (x  -  a) 

or 

{[x  (a  -  26)  +  ab]  [x  -  6]2/y3}2. 

Thus  this  factor  gives  rise  to  the  six  places  at  which  x=  -  ab/(a  -  26).     And  if  we  put 

T,  =  [x  (a  -  26)  +  ab]  [a?  - 
we  obtain 


which  is  then  the  equation  associated  with  the  transformed  surface. 

Then,  from  the  equation 

^  -  s  =  \x  (a  -  26)  +  ab]/[x  -  6], 
we  obtain 


which  give  the  reverse  transformation. 

Ex.  2.    Prove  for  the  surface 

y3=x  (x-a)  (#  -  6)2  (x-cf 
that  jo  =  2  and  that  the  function 

£=(x-b}(x-c)ly 

is  of  the  second  order.     Prove  further  that 

[a£3  _  6  _  cp  +  4fa  (£3  _  !)  =  {[a  _  b  _  c)  y&  +  Mcx  -  abc]/x  (x  -  a)}2 

Hence  shew  that  the  surface  can  be  transformed  to 


and  that 

#  =  [a2|3  +  ai;  +  26c  -  ab  -  ac]/[a|3  +  r)  +  6  +  c  -  2a], 

y  =  2£2  [be  +  a2  -  a6  -  ac]  [a2^3  +  a^  +  26c  -  ab  -  ac]  /  [«|3  +  rj  +  b  +  c  -  2a]2. 

Ex.  3.  In  the  following  five  cases  shew  that  j»  =  2,  that  £  is  a  function  of  the  second 
order,  that  in  each  case  »/2  is  either  a  quintic  or  a  sextic  polynomial  in  £,  and  obtain  each 
of  x  and  y  as  rational  functions  of  £  and  17  ; 

(a)  yw=x(x-aY(x-bf,  £  =  (x-a)  (x  -  6)//,               r)  =  Ja.(x-aji(x-bY 

08)  f  =  x(x-a)*(x-b)\  £  =  (*-a)(.*-6)//,              r,  =  Ja  .  (x  -  a)*  (x  -  b)*!y*> 

(y)  ?/>  =  x(x-a}(x-b}\  £  =  C*-6)/y,                           ,,  =  [>(a-26)  +  a6][.r-&]2/y:J 

(8)  y»  =  .r2  (.r  -  a)3  (#  -  6)3(.r  -  c)4,  £  =  A-(.r  -  a)  (x  -  6)  (#  -  c)/y2,  T,  =  c.v  (x  -  a)2  (a?  -  6)2  (x  -  c)/y3 

(c)  y4=a?(^-a)2(^-6)2(.r-  c)3,  £  =  (x-d)(x-b)(x-cy*/ft  r,  =  c(x-a)(x-b)(x-c)/xy. 


90  WEIERSTRASS'S   CANONICAL   EQUATION.  [59 

Ex.  4.    Shew  that  the  surface 

yn=(x-ai}n\..(x-ar}nr 

can  always  be  transformed  to  such  form  that  nly  ...,  nr  are  positive  integers  whose  sum  is 
divisible  by  n  :  and  in  that  form  determine  the  deficiency  of  the  surface.  Shew  also  that, 
in  that  form,  the  only  cases  in  which  the  deficiency  is  2  are  those  given  in  Exs.  1,  2,  3. 
Prove  that  the  cases  in  which  p  =  l  are* 

y6=x(x  —  af(x  —  b}3t  y*=x(x-a)(x—b\ 
y*=*x(x-a)(x-  6)2,    yz=x(x-a}(x-  6)  (x  -  c). 

The  results  here  given  have  been  derived,  with  alterations,   from  the  dissertation, 
E.  Netto,  De  Transformatione  Aequationis  yn  =  R(x}  (Berlin,  1870,  G.  Schade). 

The  equation 

yn  =  (x-ai}ni...(x-ar}nr 

is  considered  by  Abel,  (Eitvres  Completes  (Christiania,  1881),  vol.  i.,  pp.  188,  etc. 

It  is  to  be  noticed  that  in  virtue  of  Chapter  IV.  we  are  now  in  a  position,  immediately 
to  put  down  the  fundamental  integrals  for  the  surfaces  considered  in  Examples  1,  2,  3. 

60.  Passing  from  the  hyperelliptic  case  we  resume  now  the  considera 
tion  of  the  circumstances  considered  in  Chapter  III.  §§  28,  31  —  36. 

Consider  any  place,  c,  of  a  Riemann  surface  :  and  consider  rational 
functions  which  are  infinite  only  at  this  place  :  all  such  functions  will  be 
denoted  by  symbols  of  the  form  gN,  the  suffix  N  denoting  the  order  of  infinity 
of  the  function  at  the  place. 

Let  ga  be  the  function  of  the  lowest  existing  order.  The  suffixes  of  all 
other  existing  functions  gN  can  be  written  in  the  form  N  =  pa  +  i,  where 
i  <  a.  Since  there  are  only  p  orders  for  which  functions  of  the  prescribed 
character  do  not  exist,  all  the  values  i  =  0,  1  ,  ...,(«—!)  will  arise.  Let  /^a  +  i 
be  the  suffix  of  the  function  of  lowest  order  whose  order  is  congruent  to  i  for 
modulus  a.  We  obtain  thus  a  functions 


ffa>> 

Then,  if  gma+i  be  any  other  function  that  occurs,  m  cannot  be  less  than  /*,-, 
and  a  constant  A,  can  be  chosen  so  that  g-ma+i  —  ty        SW+fi  which  is  clearly 

a  rational  function  infinite  only  at  c,  is  not  infinite  to  the  order  ^a  +  i. 
Thus  we  have  an  equation  of  the  form 


wherein  pa  +j  is  less  than  ma  +  i.     Proceeding  then  similarly  with  g^+j,  we 
clearly  reach  an  equation  of  the  form 


wherein  the  coefficients  A,  B,  ...,  K,  whose  number  is  a,  are  rational  integral 
polynomials  in  ga. 

*  Cf.  Forsyth,  p.  486.     Briot  and  Bouquet,  ThSorie  des  Fonct.  Ellipt.  (Paris,  1875),  p.  390, 


62]  WEIERSTRASS'S    CANONICAL    EQUATION.  91 

In  particular,  if  gr  be  any  rational  function  whatever  of  the  gN  functions, 
we  have  equations 

g,     =  Al     +  Btf^a^    + +  K$*a  _  !«+«-i 

_  a+a_1  (ii). 


61.  If  these  equations,  regarded  as  equations  for  obtaining  #Mia+1,..., 
g^  _  a+a-i  in  terms  of  ga  and  gr,  be  linearly  independent,  we  can  obtain,  by 
solving,  such  results  as 

g».a+i  =  Qi,i  (ffr  -  AJ  +  Qifl  (9r2  -  A,)  +  .  .  .  +  Qf>  «_,  (g"'1  -  A^), 

wherein  Q{il}  ...,  Qi,a-i  are  rational  functions  of  ga,  which  are  not  necessarily 
of  integral  form. 

If  however  the  equations  be  not  linearly  independent,  there  exist  equations 
of  the  form 


or  say 


wherein  Plf  P2,  ...,  Pa_l5  P  are  integral  rational  polynomials  in  ga.  Denote 
the  orders  of  these  in  ga  by  X1}  X^,  ...,  Xrt-i>  ^  respectively;  here  P  denotes 
the  expression 

P^  +  P2A2  +...+  Pa-^a-!  . 

Then  Pk  gk  is  of  order  aX^  +  rk  at  the  place  c  of  the  surface.  In  order 
that  such  an  equation  as  (iii)  may  exist,  the  terms  of  highest  infinity  at 
the  place  c  must  destroy  one  another:  hence  there  must  be  such  an 
equation  as 

a\jc  +rJc  =  a\K  +  rk', 
and  therefore 

rfa  =  (Xjf  —  Xjfc)/(&  —  k'). 

Now  k  and  k'  are  both  less  than  a  :  this  equation  requires  therefore  that 
r  and  a  have  a  common  divisor. 

62.  Take  now  r  prime  to  a  ;  then  it  follows  that  the  equations  (ii)  must 
be  linearly  independent.  And  in  that  case  each  of  g^a+i,  •••>  g*  _  a+<i-i  can 
be  expressed  rationally  in  terms  of  ga  and  gr,  the  expression  being  integral 
in  gr  but  not  necessarily  so  in  ga. 

Also  by  equation  (i)  it  follows  that  every  function  infinite  only  at  c  is 
rationally  expressible  by  ga  and  gr:  and  in  particular  that  there  is  an 
equation  of  the  form 

Lfr  +  Ll9a-1  +  ...  +  L^g,  +  La  =  0  (iv), 


92  ALL  THE  SHEETS   WIND   AT   INFINITY.  [62 

wherein  L,  L1}  ...,  La  are   integral   rational   polynomials   in   ga,  of  which 
however,  since  gr  is   only  infinite  when  ga  is   infinite,  L   is   an   absolute 
constant.     It  follows   from  the   reasoning  given  that  the  equation  (iv)  is 
irreducible,  and  therefore  belongs  to  a  new  Riemann  surface,  wherein  ga  and 
gr  are  independent  and  dependent  variables.     Further,  any  rational  function 
whatever  on  the  original  surface  can  be  modified  into  a  rational  function 
which   is   infinite    only   at   the   place   c,  by  multiplication   by  an   integral 
polynomial  in  ga  of  the  form  (ga  -  Etf*  (ga  -  Etf*  .......     Hence  any  rational 

function  on  the  surface  is  expressible  rationally  by  ga  and  gr.  Hence  the 
surface  represented  by  (iv)  is  a  surface  upon  which  the  original  surface  can 
be  rationally  and  reversibly  represented. 

Since  g~l  is  zero  to  order  a  at  the  place  where  ga  is  infinite,  it  is  clear  that 
the  new  surface  is  one  for  which  there  is  a  branch  place  at  infinity  at  which  all 
the  sheets  wind. 

To  every  value  of  gr  there  belong  r  places  of  the  old  surface,  at  which  gr 
takes  this  value,  and  therefore  also,  in  general*,  r  values  of  ga.  Hence  the 
highest  power  of  ga  in  equation  (iv)  is  the  rth,  and  this  term  does  actually 
enter.  While,  because  ga  only  becomes  infinite  when  gf  is  infinite,  the 
coefficient  of  the  term  gra  is  a  constant  (and  not  an  integral  polynomial  in  gr). 

The  equation  (iv)  is  the  generalization  of  that  which  is  used  in  introducing  what  are 
called  Weierstrass's  elliptic  functions,  namely  of  the  equation 


This  equation  is  satisfied  by  writing  g.i~^(u\  g^  =  ^(u}:  it  is  a  known  fact  that  the 
poles  of  jp(«)  are  at  one  place  (where  w  =  0).  This  is  not  true  of  the  Jacobian  function 
snu. 

63.     It  follows  from  equation  (i)  that  the  functions 


form  a  fundamental  set  for  the  expression  of  rational  functions  infinite  only 
at  the  place  c  of  the  surface,  that  is,  a  fundamental  set  for  the  expression 
of  the  integral  rational  functions  of  the  surface  (iv).  And,  defining  the 
dimension  D  of  such  an  integral  function  F  as  the  lowest  positive  integer 
such  that  g~  F  is  finite  at  infinity  on  the  surface  (iv),  in  accordance  with 
Chap.  IV.,  §  39,  it  is  clear  that  in  the  expression  of  an  integral  function  by 
this  fundamental  system  there  arise  no  terms  of  higher  dimension  than  the 
function  to  be  expressed  :  this  fundamental  set  is  therefore  entirely  such 
an  one  as  that  used  in  Chapter  IV.  If  k  be  the  order  of  infinity  of  an 
integral  function  F,  at  the  single  infinite  place  of  the  surface  (iv),  it  is  obvious 

k 
that  the  dimension  of  F  is  the  least  integer  equal  to  or  greater  than  -  . 

*  That  is,  for  an  infinite  number  of  values  of  gr. 


64]  POSSIBLE   POSITION   OF  THE   GAPS   OF   A   RATIONAL    FUNCTION.  93 

64.  We  shall  generally  call  the  equation  (iv)  Weierstrass's  canonical  form; 
a  certain  interest  attaches  to  the  tabulation  of  the  possible  forms  which  the 
equation  can  have  for  different  values  of  the  deficiency  p.  It  will  be  sufficient 
here  to  obtain  these  forms  for  some  of  the  lowest  values  of  p ;  it  will  be  seen 
that  the  method  is  an  interesting  application  of  Weierstrass's  gap  theorem. 

Take  the  case  p=4>,  and  consider  rational  functions  which  are  only  infinite 
at  a  single  place  c  of  a  surface  which  is  of  deficiency  4.  Such  functions  do 
not  exist  of  all  orders — there  are  four  orders  for  which  such  functions  do  not 
exist ;  these  four  orders  may  be  1,  2,  3,  4,  and  this  is  the  commonest  case*, 
or  they  may  fall  otherwise.  We  desire  to  specify  all  the  possibilities  :  their 
number  is  limited  by  the  considerations — 

(i)  If  functions  of  orders  kl}  kz,  ...  exist,  say  Fl,  F*, ... ,  then  there  exists 
a  function  of  order  n^  +  n2k.2  +  ...  ,  where  n1}  n2, ...  are  any  positive  integers. 
In  fact  F^F^...  is  such  a  function. 

(ii)     The  number  of  non-existent  functions  must  be  4. 

(iii)  The  highest  order  of  non-existent  function  cannot  bef  greater  than 
2p  -  1  or  7. 

It  follows  that  a  function  of  order  1  does  not  exist,  and  if  a  function  of 
order  2  exists  then  a  function  of  order  3  does  not  exist ;  for  every  positive 
integer  can  be  written  as  a  sum  of  integral  multiples  of  2  and  3. 

Consider  then  first  the  case  when  a  function  of  order  2  exists.  Write 
down  all  positive  integers  up  to  2p  or  8.  Draw|  a  bar  at  the  top  of  the 
numbers  2,  4,  6,  8  to  indicate  that  all  functions  of  these  orders  exist — 

12345678  (a). 

If  then  the  functions  of  orders  5  or  7  existed  there  would  need  to  be 
a  gap  beyond  8,  which  is  contrary  to  the  consideration  (iii)  above.  Hence 
the  non-existent  orders  are  1,  3,  5,  7.  We  have  thus  a  verification  of  the 
results  obtained  earlier  in  this  chapter  (§  58,  Ex.  2). 

Consider  next  the  possibility  that  a  function  of  order  3  exists,  there  being 
no  function  of  order  2.  If  then  a  function  of  order  4  exists,  the  symbol 
will  be 

12345678, 

a  function  of  order  6  being  formed  by  the  square  of  the  function  of  order  3, 
that  of  order  7  by  the  product  of  the  functions  of  orders  3  and  4,  and  the 
function  of  order  8  by  the  square  of  the  function  of  order  4.  Thus  there 
would  need  to  be  a  gap  beyond  8.  Hence  when  a  function  of  order  3  exists 

*  Chap.  III.  31. 

t  Chap.  III.  §  34.     Also  Chap.  III.  §  27. 

+  Cf.  Chap.  III.  §  2G. 


94 


POSSIBLE   POSITION   OF   THE   GAPS   OF   A   RATIONAL   FUNCTION  [64 


there  cannot  be  one  of  order  4.  If  however  functions  of  orders  3  and  5 
exist  the  symbol  would  be 

12345678  (£), 

the  function  of  order  8  being  formed  by  the  product  of  the  functions  of  orders 
3  and  5.  So  far  then  as  our  conditions  are  concerned  this  symbol  represents 
a  possibility.  Another  is  represented  by  the  symbol 


12345678  (7). 

In  this  case  however  the  existent  integral  function  of  order  8  is  not  expressible 
as  an  integral  polynomial  in  the  existent  functions  of  orders  3  and  7. 

When  a  function  of  order  3  exists  there  are  no  other  possibilities  ;  other 
wise  more  than  4  gaps  would  arise. 

Consider  next  the  possibility  that  the  lowest  order  of  existent  function 
is  4.     Then  possibilities  are  expressed  by 

1  2  3  4~5  "6  7  8  (S), 

1  2  3  477  6  7~8  (e), 


12345  6T~8  (£), 

as  is  to  be  seen  just  as  before. 

Finally,  there  is  the  ordinary  case  when  no  function  of  order  less  than 
5  exists,  given  by 


1234  5~6  7  8 


(77). 


For  these  various  cases  let  a  denote  the  lowest  order  of  existent  function 
and  r  the  lowest  next  existent  order  prime  to  a.  Then  the  results  can  be 
summarised  in  the  table 


p=4           a 

r 

Gaps  at 
orders 

Fundamental 
system  of  orders 

Dimensions  of 
functions  of 
fundamental 
system 

Sum  of 
these  di 
mensions 

P+rt-i 

\(n-\)(r-\)-p 

a             2 

9 

1,  3,  5,  7 

0,  9 

0,  5 

5 

5 

0 

/3           3 

5 

1,  2,  4,  7 

0,  5,  10 

0,  2,  4 

6 

6 

0 

y       3 

7 

1,  2,  4,  5 

0,7,8 

0,  3,  3 

6 

6 

2 

8          4 

5 

1,  2,  3,  7 

0,  5,  6,  11 

0,  2,  2,  3 

7 

7 

2 

e            4 

5 

1,  2,  3,  6 

0,  5,  7,  10 

0,  2,  2,  3 

7 

7 

2 

f           4 

7 

1,  2,  3,  5 

0,  6,  7,  9 

0,  2,  2,  3 

7 

7 

5 

f,            5 

6 

1,  2,  3,  4 

0,  6,  7,  8,  9 

0,  2,  2,  2 

8 

8 

6 

65] 


FOE   THE   CASES  p  =  3,  p  =  4. 


95 


That  the  seventh  and  eighth  columns  of  this  table  should  agree  is  in 
accordance  with  Chapter  IV.,  §  41.  The  significance  of  the  last  column  is 
explained  in  §  68  of  this  Chapter. 

Similar  tables  can  easily  be  constructed  in  the  same  way  for  the  cases 
p=l,  2,  3. 

Ex.  1.     Prove  that  for  p  =  3  the  results  are  given  by 


p  =  3 

a 

r 

Gaps  at 
orders 

Fundamental 
system  of  orders 

Dimensions  of 
functions  of 
fundamental 
system 

Sum  of 
these  di 
mensions 

P+a-l 

«i 

•2 

1 

i,  3,  r> 

0,7 

0,4 

4 

4 

IB 

3 

4 

1,2,5 

0,4,8 

0,  2,  3 

5 

5 

7 

3 

5 

1,2,4 

0,5,7 

0,2,3 

5 

5 

8 

4 

5 

1,2,3 

0,  5,  6.  7 

0,  2,  2,  2 

6 

6 

Ex.  2.     Prove  that  for  />  =  5,  6,  7,  8,  the  possible  cases  in  which  the  lowest  existing 
function  is  of  the  third  order  are  those  denoted  by  the  symbols 


p  —  5 


123456789  10 
1  2  3  4  5  6~7  8  JTlO 

12345678  9~10  11~12 


1  2  3  4  5  6  7  8  9  10  11  12 


1  2  3  4  5  6  7  8  9  10  11  12  13  14 


=  7  J 1  2  3  4  5  6  7  8  9  10  11  12  13  14 


.1  2  3  4  5  6  7  8  9  10  11  12  13  14 


a  2  3  4  5  6  7  8  9  10  11  12  13  14  15  16 

p  =  8  ,123456789  10  TTT2  13  14  15  16 

ll  2345678  916  11  12~  13  14  HTT6 

65.  We  have  already  stated  (Chap.  IV.  §  38)  that  when  the  fundamental 
set  of  integral  functions  are  so  far  given  that  we  know  the  relations  expressing 
their  products  in  terms  of  themselves,  the  form  of  an  equation  to  represent 
the  surface  can  be  deduced.  We  give  now  two  examples  of  how  this  may  be 
done :  these  examples  will  be  sufficient  to  explain  the  general  method. 

Take  first  the  case  p  =  4,  a  =  3,  r  =  7.  Denote  the  corresponding  func 
tions  by  g3,  g7.  In  accordance  with  §  60  preceding,  all  integral  functions  can 
be  expressed  by  means  of  g3  and  two  functions  g7,  g8  whose  orders  are  respec 
tively  =  1  and  2  for  modulus  3 :  in  particular  there  are  equations  of  the  form 

9?  =  9s  (03,  1)2  +  g7  (0s,  1)2  +  (03,  1)4 
9rf*  =  9*  (ff*.  1)8  +  9i  (ff»  l\  +  (ft,  1)5 

#82  =08  (</3>    1).  +07  (03,    1)3  +  (03,    1)S 


96  FORMATION   OF   THE   EQUATION.  [65 

wherein  (g3,  1)2  denotes  an  integral  polynomial  in  y3  of  order  2  at  most,  the 
upper  limit  for  the  suffix  being  determined  by  the  condition  that  no  terms 
shall  occur  on  the  right  of  higher  dimension  than  those  on  the  left.  Similarly 
for  the  other  polynomials  occurring  here  on  the  right. 

Instead  of  g7,  g8  we  may  clearly  use  any  functions  g7  -  (g3,  1),,  gs  -  (g3y  1)2. 
Choosing  these  polynomials  to  be  those  occurring  on  the  right  in  the  value  of 
ffrffs)  we  may  write  our  equations 

9*  =  «2#8  +  &07  +   Q4  ,    #82  =  7S08  +  a$7  +  «5  ,    9$*  =  &  (A), 

where  the  Greek  letters  denote  polynomials  in  g3  of  the  orders  given  by 
their  suffixes. 

Multiplying  the  first  and  last  equations  by  gs  and  g7  respectively,  and 
subtracting,  we  obtain 

g7&  =  gs  (0^8+  &#7  +  o4) 


and  thence,  since*  1,  g7,  g8  cannot  be  connected  by  an  integral  equation  of 
such  form, 

0272  +  «4  =  0,  fifeo,  -  /33  =  0,  ar2<*5  +  /3o/35  =  0, 

from  which,  as  0.3  is  not  identically  zero,  —  for  then  g7  would  satisfy  a  quadratic 
equation  with  rational  functions  of  g3  as  coefficients  —  we  infer 

«5  +  &«3  =  0  (B). 

Similarly  from  the  last  two  equations  (A)  we  have 

7  +  oB) 


and  thence 

/8B-  05,03  =  0,  0^  +  05  =  0,  72^3  +  oa«4  =  0, 

so  that,  since  «3  cannot  be  zero  —  as  follows  from  the  second  of  equations  (A)  — 

we  have 

VM  +  a4  =  0  (C). 

The  equations  (B)  and  (C)  have  been  formed  by  the  condition  that  the 
equations  (A)  should  lead  to  the  same  values  for  gfa  and  gfg1t  however  these 
latter  products  be  formed  from  equations  (A).  We  desire  to  shew  that,  con 
versely,  these  equations  (B)  and  (C)  are  sufficient  to  ensure  that  any  integral 
polynomial  in  g7  and  gs  should  have  an  unique  value  however  it  be  formed 
from  the  equations  (A).  Now  any  product  of  powers  of  g1  and  g8  is  of  one  of 
the  three  forms  g7,  gf  ,  g7g*K.  In  the  first  two  cases  it  can  be  formed  from 
equations  (A)  in  one  way  only.  In  the  third  case  let  us  suppose  it  proved 
that  K  has  an  unique  value  however  it  be  derived  from  the  equations  (A); 

*  Chap.  IV.  §  43. 


66]  FORMATION   OF  THE   EQUATION.  97 

then  to  prove  that  g7g8  K  has  an  unique  value  we  require  only  to  prove  that 
g7  .  ge  K  =  gs  .  g7  K.  Let  K  be  written  in  the  form  ggL  +  g7M  +  N.  Then  the 
condition  is  that  g7  (LgJ  +  Mg7g8  +  Ngs)  shall  be  equal  to  g8  (Lg7g%  +  Mgf  +  Ng7). 
This  requires  only  #7  •  #82  =  #»  •  #7#8  and  g7  .  g7ga  =  ga  .  g?  :  and  it  is  by  these 
conditions  that  we  have  derived  equations  (B)  and  (C).  Hence  also  g^^K 
has  an  unique  value. 

Thus  every  rational  integral  polynomial  in  g7  and  gs  will,  when  the  con 
ditions  (B),  (C)  are  satisfied,  have  an  unique  value  however  it  be  formed  from 
equations  (A). 

The  equations  (B)  and  (C)  are  equivalent  to  a4=-a272,  As  =  a2«s, 
a5  =  —  a3/32,  and  lead  to 


Thence 


or  g73  -  P2gf  +  cr2  y2g7  -  a22«3  =  0, 

which  is  the  form  of  equation  (iv)  which  belongs  to  the  possibility  under 
consideration. 

The  expression  of  the  fundamental  set  of  integral  functions  1,  gr,  g%  in  terms  of  g3  and 
-  is  therefore 


66.  Take  as  another  example  the  possibility  e,  §  64  above,  where 
a  =  4,  r  =  5,  the  orders  of  non-existent  functions  being  1,  2,  3,  6.  For  a 
fundamental  system  of  integral  functions  we  may  take  1,  gs,  g*,  g7. 

We  have  then  such  an  equation  as 

9*9-1  =  g?  (04,  l)i  +  c#52  +  <75(<74,  l)i  +  (&,  l)s 
where  c  is  a  constant  :  let  this  be  written  in  the  form 

gsg?  =  «i#7  +  g*  +  frgs  +  «s, 

the  constant  c  being  supposed  absorbed  in  gf. 

Write  hs  for  g^  —  ^  and  h7  for  g7  —  Ji5  —  A  ~  %ai- 
Then 


Replacing  now  /*5,  h7  by  the  notation  gs,  g1  and  a3  +  fliA  +  <*i2  by  «3  we  may 
write 


9*97  =  «s,    i/72  =  ^3  +  aa^s  +  a,  (7S2  +  frg,  ,    g,3  = 
B. 


98  EXAMPLES.  [66 

Hence  the  condition  g5 .  gf  =  g5g7 .  g7  requires 

from  which 

and  thence 

0^3=  —  ^a^a,  or  if  0^  is  not  zero,  y3=—(3-iy.2. 

Substituting  this  value   for  ys  and  the  value  g7=  a3lg5=  ^yz/ga  in  the 
expression  for  g&s  we  obtain 


or 

9*  ~  Jiffs*  ~  P*9*  +  Piytfs  -  *i722  =  0, 

which  is  then  a  form  of  the  equation  (iv)  corresponding  to  the  possibility  (e). 
In  this  case  the  fundamental  integral  functions  may  be  taken  to  be 


It  is  true  in  general,  as  in  these  examples,  that  the  terms  of  highest  order 

of  infinity  in  the  equation  (iv)  are  the  terms  ga,  gr.     For  there  must  be  two 
terms  (at  least)  of  the  highest  order  of  infinity  which  occurs  ;  and  since  r  is 

prime  to  a,  two  such  terms  as  gag*,  9a9r   cannot  be  of  the  same  order  of 
infinity. 

Ex.  1.     Prove  that  for  p  =  3  the  form  of  the  equation  of  the  surface  in  the  case  where 


and  shew  that  this  is  reducible  to  the  form 

yz  +yx  (x  +  a)  +  x*  +  c^-r3  +  a.^  +  a^c  +  a4  =  0, 

x  being  of  the  form  Ag3  +  B,  y  of  the  form  Cg^  +  Dg3  +  E,  A,  B,  C,  D,  E  being  constants. 
Thus  the  surface  depends  on  3p  -  4  or  5  constants,  at  most. 

Ex.  2.  The  reader  who  is  acquainted  with  the  theory  of  plane  curves  may  prove  that 
the  homogeneous  equation  of  a  quartic  curve  which  has  a  point  of  osculation,  can  be  put 
into  the  form 


By  putting  #  =  »;/£,  #  =  «/£>  tnis  takes  the  form  of  the  final  equation  of  Example  1.     Com 
pare  Chapter  III.  §  32. 

Ex.  3.     Prove  that  for  jt)  =  3,  the  form  of  the  equation  of  the  surface  in  the  case  where 


Ex.  4.     Denoting  the  left  hand  of  equation  (iv)  by  f(gr,  ga],  df/dgr  by  f'(ffr)  and  the 
operator 


67]  RATIONAL    FUNCTIONS   NOT   EXPRESSIBLE   INTEGRALLY.  99 

by  Z>,  prove  that  if  gm  be  any  rational  function  which  is  infinite  only  where  gu  and  gr  are 
infinite,  there  exists  an  equation 

X<>J»-igm  +  XlD*-*gm  + +  Xa_l9m  =  0, 

where  X0, ,  J^-i  are  polynomials  in  ga. 

67.  We  have  already  in  Chapter  IV.  referred  to  the  fact  that  an  integral 
function  is  not  necessarily  expressible  integrally  in  terms  of  the  coordinates 
x,  y  by  which  the  equation  of  the  surface  is  expressed,  even  though  y  be  an 
integral  function.  The  consideration  of  the  Weierstrass  canonical  surface 
suggests  interesting  examples  of  integral  functions  which  are  not  expressible 
integrally. 

In  order  that  an  integral  function  g  whose  order  is  p  should  be  expressible 
as  an  integral  polynomial  in  the  coordinates  ga,  gr  of  the  surface,  in  the  form 


it  is  necessary  that  there  should  be  a  term  on  the  right  hand  whose  order  of 
infinity  is  the  same  as  that  of  the  function  ;  we  must  therefore  have  an 
equation  of  the  form 

fj,  =  ma  +  nr 

wherein  m,  n  are  positive  integers.  Since  a  polynomial  in  ga  and  gr  can  be 
reduced  by  the  equation  of  the  surface  until  the  highest  power  of  gr  which 
enters  is  less  than  a,  we  may  suppose  n  less  than  a. 

This  equation  is  impossible  for  any  value  of  //,  of  the  form  nr  —  ka.  And 
since  herein  k  may  be  taken  equal  to  any  positive  integer  less  than  nr/a,  the 
number  of  integers  of  this  form,  with  any  value  of  n,  is  E(nr/a),  or  the 
greatest  integer  contained  in  the  fraction  nr/a.  Hence  on  the  whole  there 
are 

°2  E(nr/a) 

n=l 

orders  of  integral  functions  which  are  not  expressible  integrally  by  ga  and  gr. 

Corresponding  to  any  order  which  is  not  expressible  in  the  form  nr  —  ka, 
which  is  therefore  of  the  form  nr  +  ma,  we  can  assign  an  integrally  expressible 

integral  function  *  namely  gnrg™  :  hence  the  p  orders  corresponding  to  which, 
according  to  Weierstrass's  gap  theorem,  no  integral  functions  whatever  exist, 
must  be  among  the  excepted  orders  whose  number  we  have  proved  to  be 

"Z  E  (nr/a)  orf  £  (a  -  1)  (r  -  1). 

n  =  l 

Though  it  does  not  follow  that  every  integral  function  whose  order  is  of  the  form  nr  +  ma 
can  be  expressed  wholly  in  integral  form. 

t  If  a   right-angled   triangle  be  constructed   whose   sides   containing  the   right   angle   are 
respectively  a  and  ?•,  and  the  interior  of  the  triangle  be  ruled  by  lines  parallel  to  the  sides 

7—2 


100  NUMBER   OF   ORDERS   OF   RATIONAL   FUNCTIONS  [67 

Hence  the  number  of  orders  of  actually  existing  integral  functions  which  are 
not  expressible  integrally  is 


In  the  table  which  we  have  given  for  p  =  4  (§  G4)  the  existing  integral 
functions  which  are  not  expressible  integrally  are,  for  the  case  (7),  of  orders  8 
and  11  ;  for  the  case  (8}  of  orders  6  and  11  ;  for  the  case  (e)  of  orders  7  and 
11  ;  for  the  case  (f)  of  orders  6,  9,  10,  13,  17  ;  for  case  (77)  of  orders  7,  8,  9,  13, 
14,  19.  The  reader  can  easily  assign  the  numbers  for  the  cases  in  which 
^  =  3. 

Ex.  1.     Prove  that  for  the  surface 

9*+9*(9*-c)+9f,9s(9v  l\+9*(9*>  Va  =  °> 
the  function 

ffj=ff&(ff&-c')/ff3 
is  an  integral  function  which  is  not  expressible  as  an  integral  polynomial  in  g3  and  <75. 

Ex.  2.     Prove  that  for  the  surface 


where  a2  =  o  (gs  -  kj  (g3  -  £2), 

82  =  (ff3-ki)fi  +  l>i, 

/!  being  of  the  first  order  in  g3,  and  c,  blt  k±,  k^  being  constants,  the  two  following  functions 
are  integral  functions  not  integrally  expressible  —  • 

#8  =g^  (9i  +  As)/a2  1  ffu  ='9i  (ffr  +  bi)l(ffa  ~  *i)- 

68.  The  number  ^  (a  —  l)(r-l)—p  is  susceptible  of  another  interpre 
tation  which  is  in  close  connexion  with  the  last.  Let  the  set  of  fundamental 
integral  functions  for  the  Weierstrass  canonical  surface  be  denoted  by 
1,  Glt  G2,...,  6ra_!.  From  the  equations  whereby  1,  gr,  gr,...,  gar  are 
expressed  in  terms  of  them  we  are  able  (Chapter  IV.,  §  43)  to  deduce  an 
equation 


wherein  A(l,  gr,  ...,  gv"1)  is  formed  as  a  determinant  whose  (i,  j)th  element 
is  the  sum  of  the  values  of  g*r+J~2  at  the  a  places  of  the  surface  where  ga  has 
the  same  value,  and  is  therefore  an  integral  polynomial  in  ga,  A(l,  GI,  .  .  .  ,  Ga-^) 
is  formed  as  a  determinant  whose  (i,  j)th  element  is  the  sum  of  the  values  of 
Gi^Gj-!  for  the  same  value  of  ga,  which  also  is  an  integral  polynomial  in 

containing  the  right  angle,  and  at  unit  distances  from  these  sides  and  each  other,  so  describing 
squares  interior  to  the  triangle,  the  number  of  angular  points  interior  to  the  triangle  is  easily 

seen  to  be    S   E  (nr/a).     On  the  other  hand  if  the  right-angled  triangle  be  regarded  as  the  half  of 

n=l 

a  rectangle  whose  diagonal  is  the  hypotenuse  of  the  right-angled  triangle,  and  the  ruled  lines  be 
continued  into  the  other  half,  it  is  easily  seen  that  the  total  number  of  angular  points  of  the 
squares  interior  to  the  whole  rectangle  is  (a-  1)  (r-  1). 


69]  NOT    EXPRESSIBLE    INTEGRALLY.  101 

ga,  and  V  is  a  determinant  whose  elements  are  those  integral  polynomials  in 
ga  which  arise  in  the  expressions  of  1,  gr,  ...,  g"~l  in  terms  of  1,  GI,  ...  ,  (ra_i. 

The  determinant  A  (1,  gr,  ...  ,g"~l)  is  the  square  of  the  product  of  all  the 
differences  of  the  values  of  gr  which  correspond  to  any  value  of  ga.  It 
therefore  vanishes,  for  finite  values  of  ga,  when  and  only  when  two  of  these  are 
equal.  If  the  form  of  the  equation  of  the  surface  be  denoted  by  f(gr,  ga)  =  0, 
this  happens  when,  and  only  when,  df/dgr=0.  Now  df/dgr  is  an  integral 
polynomial  in  ga  and  gr,  of  order  a—  1  in  the  latter.  Regarded  as  a  rational 
function  on  the  surface  it  is  only  infinite  when  ga  and  gr  are  infinite.  It 
follows  from  the  fact  (§  66),  that  gar  is  a  term  of  the  highest  order  of  infinity 
which  enters  in  the  polynomial  f(gr,  ga\  that  df/dgr  is  infinite,  at  ga  =  oc  , 
to  an  order  r(a—  1).  This  is  therefore  the  number  of  finite  places  on  the 
surface  at  which  df/dgr  vanishes.  Hence  we  infer  that  the  polynomial 
A(l,$.,—»$£-1j  is  of  degree  r(a-l)  in  ga. 

Since  there  is  a  branch  place  at  infinity  counting  for  (a  —  I)  branch 
places,  the  polynomial  A(l,  Glt...,Ga-i)  is  of  order  2a  +  2p  -  2-  (a  -  1) 
=  a-l  +  2pin0fl(§§48,  61). 

Thus  V  is  of  order 

i[r(a-l)-(a- 
that  is,  of  order 


This  interpretation  of  the  degree  of  v  is  of  interest  when  taken  in  connexion  with  the 
theorem  —  Every  integral  function  can  be  written  in  the  form 

(ffa,  gr)l(ffa,  1), 

the  numerator  being  an  integral  polynomial  in  ga  and  gr,  and  the  denominator  being  an 
integral  polynomial  in  ga.  All  the  polynomials  (ga,  1)  thus  occurring  are  divisors  of  the 
polynomial  y.  See  §  48  and  §  88  Exx.  ii,  iii*. 

When  the  factors  of  v  are  all  simple  we  may  therefore  expect  to  be  able  to  associate 
each  of  them,  as  denominator,  with  an  integral  function  which  is  not  integrally  expressible. 
In  this  connexion  some  indications  are  given  in  a  paper,  Camb.  Phil.  Trans,  xv.  pp.  430,  436. 
For  Weierstrass's  canonical  surface  see  also  a  dissertation,  De  aequatione  algebraica...in 
quandam  formam  canonicam  transformata.  G.  Valentin.  Berlin,  1879.  (A.  Haack.) 
Also  Schottky,  Crelle,  83.  Conforme  Abbildung.  .  .ebener  Flachen. 

69.  The  method  which  has  been  exemplified  in  §§  65,  66  for  the  formation 
of  the  general  form  of  the  equation  of  a  surface  when  the  fundamental  set 
of  integral  functions  is  given,  is  not  limited  to  Weierstrass's  canonical  surface. 

Take  for  instance  any  surface  of  three  sheets,  and  let  1,  g1}  g^  be  any  set 
*  Cf.  Harkness  and  Morley,  Theory  of  Functions,  p.  268,  §  186. 


102  INDICATION   OF    GENERALIZATION    OF  [69 

of  fundamental  integral  functions  with  the  properties  assigned  in  Chapter  IV. 
§  42.     Then  there  exist  equations  of  the  form 

£i#2  =  7  +  ft  $1  +  a  9* 


wherein  the  Greek  letters  denote  polynomials  in  the  independent  variable 
of  the  surface,  x,  whose  degrees  are  limited  by  the  condition  that  no  terms 
occur  on  the  right  of  higher  dimensions  than  those  on  the  left. 

Thus  the  dimension  of  ft  is  not  greater  than  that  of  g2  and  the  dimension 
of  a  is  not  greater  than  that  of  g^  Hence  we  may  use  #1  —  a,  g2  —  (3  instead 
of  g1  and  g2  respectively,  and  so  take  the  first  equation  in  the  form  glg3  =  y> 
the  form  of  the  other  equations  being  unaltered.  As  before,  there  are  con 
ditions  that  these  equations  should  lead  to  unique  values  for  every  integral 
polynomial  in  gl  and  </2,  namely 

#2  (71  +  &9i  +  *i9*)  =  9iV>    9i  (72  +  «2<7i  +  &SO  =  #27- 
These  lead  to  the  equations 


7=a1a2,     71  =- 
and  thence  to 


(v) 


Since  every  rational  function  can  be  represented  rationally  by  x  and 
gl  and  g2  =  &\&>tlgi  ,  it  follows  that  every  rational  function  can  be  represented 
rationally  by  x  and  glt  Hence  the  surface  represented  by  the  first  of  these 
two  final  equations  is  one  upon  which  the  original  surface  is  rationally  and 
reversibly  represented.  So  also  is  the  surface  represented  by  the  second  of 
these  equations. 

The  fundamental  integral  functions  are  derived  immediately  from  the 
equation,  being 


Ex.  1.     Prove  that  the  integrals  of  the  first  kind  for  the  surface 

f(ffi>  x)=ffi3-Piffi2+aiP2ffi  -0^02  =  0 
are  given  by 


where  rj  +  1,  r2  +  l  are  the  dimensions  of  g±  and  gz  and  /'  (g^  = 

Ex.  2.     Prove  that  for  the  case  quoted  in  Ex.  i,  §  40,  Chapter  IV,  the  form  of  the 
equation  is,  (i)  when  p  is  odd  =  2n-  1,  say, 

Sfn3-angn2  +  an_1an  +  lffn-ain-lan  +  2  =  0, 


70]  WEIERSTRASS'S   CANONICAL   EQUATION.  103 

where  an_l,  an,  an+1,  n,l  +  2  are  polynomials  in  x  of  the  orders  indicated  by  their  suffixes, 
(ii)  when  j9  is  even  =  2?i  —  2,  say, 

ffn3  -  «nffn*  +  Pn*ngn  ~  /3»27n  =  0, 
where  on,  /3tt,  yn,  8n  are  polynomials  in  x  of  the  nth  order. 

Ex.  3.     Writing  ffi  =  nly,  the  first  of  the  equations  (v)  becomes 

Q2=0.  (A) 


If  the  dimensions  of  gl  and  gz  be  rl  +  l,  T2-|-l,  find  the  degrees  of  the  polynomials 
GI}  /31}  a2,  /32.  And  prove  that  if  the  positive  quadrant  of  a  plane  of  rectangular  co 
ordinates  (x,  y)  be  divided  into  squares  whose  sides  are  each  1  unit  in  length,  and  a  convex 
polygon  be  constructed  whose  angular  points  are  determined  from  this  equation  (A),  by 
the  rule  that  a  term  xry"  in  the  equation  determines  the  point  (r,  s)  of  the  plane,  then  the 
number  of  angular  points  of  the  squares  which  lie  within  this  polygon  is  p. 

70.     In  obtaining  the  equation 

9?  ~  &#!2  +  «!&#!  -  «!2«2  -  0  (E) 


we  have  spoken  as  if  the  original  surface  were  of  three  sheets.     It  is  im 
portant  to  notice  that  this  is  not  necessary. 

Suppose  our  given  surface  to  be  any  surface  for  which  a  rational  function 
of  the  third  order,  £,  exists.  Take  c  so  that  the  poles  of  the  function  (£  —  c)~l, 
which  is  also  a  function  of  the  third  order,  are  distinct  ordinary  places  of  the 
surface.  So  determined  denote  the  function  by  x.  Let  alf  cr2,  «s  denote  these 
poles.  Then  just  as  in  §  39  of  Chapter  IV.  it  can  be  shewn  that  there  exist 
two  rational  functions  g^  and  g2,  only  infinite  in  ax  and  a.2,  such  that  every 
rational  function  which  is  infinite  only  in  Oj,  a2,  a3  can  be  expressed  in  the 
form 


wherein  y,  a,  /3  are  integral  polynomials  in  x  whose  degrees  have  certain 
upper  limits  determined  by  the  condition  of  dimensions. 

And  as  before  we  can  obtain  the  equation  (E).  Further,  if  F  be  any 
rational  function  whatever  and  Alf  A2,  ...  be  the  values  of  x  at  the  places 
other  than  ax,  a2,  a3  at  which  F  becomes  infinite,  it  is  clearly  possible  to  find 
a  polynomial  K  of  the  form  (x  -  A^  (x  -  A^)n*  .  .  .  such  that  .KTonly  becomes 
infinite  at  al}  a2,  a3.  Hence  every  rational  function  of  the  original  surface 
can  be  expressed  rationally  by  x  and  glt 

Thus  as  x,  g^  are  rational  functions  on  the  original  surface,  (E)  represents 
a  new  surface  upon  which  our  canonical  surface  is  rationally  and  reversibly 
represented.  And  it  is  as  much  the  proper  normal  form  for  surfaces  upon 
which  a  rational  function  of  the  third  order  exists  as  is  the  equation 


104  SURFACE  OF  FOUR  SHEETS.  [70 

o-2  =  (z,  l)2p+2,  previously  derived,  for  the  hyperelliptic  surfaces  upon  which  a 
function  of  the  second  order  exists. 

Ex.     Obtain  the  hyperelliptic  equation  in  this  way. 

71.  In  the  same  way  we  can  obtain  a  canonical  form  for  surfaces  upon 
which  a  function  of  the  fourth  order  exists.  We  can  shew  that  there  exist 
three  functions  glt  gz,  g3  satisfying  such  equations  as 


+  k, 


wherein  the  nine  coefficients  are  integral  polynomials  in  a  rational  function  x, 
which  is  of  the  fourth  order;  and  that  the  surface  is  rationally  and  reversibly 
representable  upon  a  surface  given  by  the  equation 


+  aj)sk2  +  a-jbjcz  +  aj)3ki  =  0. 

Ex.  These  coefficients  alt  ...,  fc3  satisfy  certain  relations;  prove  that  the  conditions 
that  Sra.ff3*=ffzffa.g3,  gl  .  g32=ffiff3  •  9v  ffiffs-  ffa=ffaffa-ffi  are  that  the  following  nine 
polynomials  should  be  divisible  by  a  polynomial  A,  whose  value  is  a]2b3—  a3a161-ot2^i2  > 


Herein  ?i1  =  a3  —  c1?  ^1  =  a263  —  ^x. 
In  fact  if 


the  results  of  the  division  of  these  nine  polynomials  by  A  are  respectively 

«o>    &5>    C5>    a4>    64>    C4>    f/(i>    ^0»    C6> 

while 


72.  When  the  order  of  the  independent  function,  denoted  in  §§  69—71  by  x,  is  known, 
and  the  dimensions  of  the  fundamental  integral  functions  in  regard  thereto,  the  general 
forms  of  the  polynomial  coefficients  in  the  equations,  whereby  the  products  of  pairs  of 
these  integral  functions  are  expressed  as  linear  functions  of  themselves,  can  be  written 
down.  And  thence,  if  the  necessary  algebra  (such  as  that  indicated  in  the  example  of 
§  71),  which  serves  to  limit  the  forms  of  these  polynomial  coefficients,  can  be  carried  out,  a 
canonical  form  of  the  equation  of  the  surface  can  be  deduced. 

But  the  converse  process  may  arise  :  when  we  are  given  a  form  of  the  fundamental 
equation  associated  with  the  surface,  we  may  require  to  replace  the  given  equation  by  one 
in  which  the  dependent  variable  is  one  of  the  set  of  fundamental  integral  functions.  More 
generally  we  may  replace  it  by  an  equation  in  which  the  dependent  variable  is  an  integral 
function  of  the  form 


OF   1 

UNIVEI 


V1 

OF   Till 


_  CAl 


74]  DETERMINATION    OF    FUNDAMENTAL    INTEGRAL    FUNCTIONS.  105 

This  replacement  possesses  a  high  degree  of  interest  (§  88.  Ex.  iii).  In  either  case 
it  is  necessary  to  be  able  to  calculate  the  fundamental  integral  functions. 

73.  We  give  now  sufficient  explanation  to  enable  the  reader  to  calculate  the  expression 
of  the  fundamental  integral  functions  for  any  given  form  of  the  fundamental  equation 
associated  with  the  Riemann  surface.  This  equation  may*  be  taken  in  the  form 

#*+y"~lai  +  ~-+ytt»-i  +  a»  =  0>  (A) 

«15  ...,  an  being  integral  polynomials  in  x  ;  thus  y  is  an  integral  function  of  x  (§  38). 

The  n  values  of  any  rational  function,  17,  which  arise  for  the  same  value  of  x,  will  be 
denoted  by  i^1),  ...  ,  ij(")  and  called  conjugate  values  ;  their  sum  will  be  denoted  by  2^.  If 
any  of  the  possible  rational  expressions  of  17  be  $  (x,  y)/^  (#,  y\  $  and  ty  being  integral 
polynomials  in  x  and  y,  and  if  in  the  expression  of  >j('), 


we  multiply  numerator  and  denominator  by  the  product  of  the  n  —  l  values  conjugate  to 
^(.r,^1)),  the  denominator  will  become  an  integral  symmetric  function  of  y(l\  ...,y(n\  and 
can  therefore  be  expressed  by  means  of  the  equation  (A),  as  an  integral  polynomial  in  x  ; 
and  the  numerator  will  take  a  form  which  can  be  expressed  as  an  integral  polynomial  in 
x  and  yW.  Hence  the  value  of  any  rational  function,  on  the  surface  associated  with  the 
equation  (A),  can  be  expressed  in  the  form 


_ 
1= 

A,  ...,  An_ly  D  denoting  integral  polynomials  in  x,  with  no  common  divisor. 

Thus,  to  determine  the  expression  of  the  fundamental  integral  functions,  we  may 
enquire  what  modification  this  general  form  undergoes  when  TJ  is  an  integral  function. 

74.  In  the  first  place  the  denominator  D  must  be  such  that  Dz  is  a  factor  of  the 
integral  polynomial  f  A  (1,  ?/,  ...,yn~1)  ;  so  that  D  is  capable  only  of  a  limited  number  of 
forms.  For  let  x  —  a  be  a  factor  of  Z),  repeated  r  times,  and  write 

Ai  =  (x-aYBi^Ci,        (t  =  0,l,...  ,(n-l)) 

wherein  d  is  a  polynomial  of  order  less  than  r  ;  since  J,  ...,  An_l  have  no  common  divisor 
which  divides  D,  not  all  of  C,  Clt  ...  ,  Cn_l  can  be  divisible  by  x-a.     Then  the  function 


is  an  integral  function,  when  17  is  an  integral  function,  as  appears  from  its  first  form  of 
expression.     Denote  it  by  f. 

Suppose  Ci  not  divisible  by  x-a.     From  the  equation  f 

Mi^-.^-U^+S..^-'^^!,^,...,^^, 

recalling  the  form  of  the  determinant  which  is  the  square  root  of  the  left  hand  side,  we 
infer 

(^VA(1'<y'><M'yi~1'^)y<+1'-"'/l~1)=Vi2A(1'5ri'>>i'5r»-i)- 

Hence,  save  for  sign, 

*/?!-(*-  aX/Ct, 

so  that  (x  —  aY  divides  v- 

Thus  the  first  step  in  the  determination  of  the  integral  functions  is  to  put  A  (!,_>/, 
....y"-1)  into  the  form  MI*»  ...u**,  wherein  MI(  ...  ,  ur  are  polynomials  having  only  simple 

*  Chap.  IV.  §  38.  f  Chap.  IV.  §  43. 


106  ACTUAL   ALGEBRAICAL   DETERMINATION   OF  [74 

factors.  This  can  always  be  done  by  the  rational  process  of  finding  the  highest  divisor 
common  to  A(l,y,  ...,yn~1)  and  its  differential  coefficients  in  regard  to  x.  It  will  include 
most  cases  of  practical  application  if  we  further  suppose  all  the  linear  factors  of 
A(l>ty,  ...,yn~1)  to  be  known*. 

75.  Suppose  then  that  x  —  a  is  a  factor  which  occurs  to  at  least  the  second  order  in 
A(l,y,  ...,<yn"1).  Denote  x-a  by  u.  By  the  solution  of  a  system  of  linear  equations, 
we  can  (below,  §  78)  find  all  the  existing  linearly  independent  expressions  of  the  form 

(a  +  a1y+...+an_lyn-1)lu, 

wherein  a,  at  ,  .  .  .  ,  a,t  _  1  are  constants,  which  represent  integral  functions.  If  the  highest 
power  of  y  actually  entering  be  the  same  in  two  of  these  integral  functions,  say  in  f  and  f  ', 
we  can  use  instead  of  f  a  function  of  the  form  f  —  /if,  where  /i  is  a  certain  constant.  By 
continued  application  of  this  method  of  reduction  we  obtain,  suppose,  k  integral  functions, 
of  the  form 

£r  =  (a'  +  a\y+...+a'ryr)/U,  (C) 

wherein,  since  these  functions  are  linearly  independent,  k  is  less  than  n,  and  the  vahies  of 
r  that  occur  are  all  different.  These  values  of  r  that  occur  are  among  the  sequence 
1,  2,  ...,  (n—  1)  ;  let  s  denote  in  turn  all  the  n—  1  —  k  other  integers  in  this  sequence.  Put 
£,  for  y*.  Consider  now  the  set  of  integral  functions 

*»  lit  •••>£*-!• 

As  before  we  can  determine  by  the  solution  of  a  system  of  linear  equations  all  the 
linearly  independent  functions  of  the  form 


wherein  /3,#i,  ...,  /3n_x  are  constants,  which  are  integral  functions  ;  and,  as  before,  we  can 
choose  them  so  that  the  f  's  of  highest  suffix  which  occur  shall  not  be  the  same  in  any  two 
of  these  integral  functions.  Then  in  place  of  1,  f1}  ...,  fn_1  we  obtain  a  set  1,  £15  ...,£„_!, 
wherein  gr  is  fr  unless  there  be  an  integral  function  of  the  form 

O'  +  /3'lCl  +  ...+/3'rtr)/«,  (D) 

wherein  the  f  of  highest  suffix  occurring  is  £r,  in  which  case  £r  denotes  this  function. 
Then  we  enquire  whether  there  are  any  integral  functions  of  the  form 


•y,  ...,yn-i  being  constants.  If  there  are,  the  process  is  to  be  continued  t-  If  there  are 
none,  let  v  denote  any  other  linear  factor  occurring  in  A  (1,  y,...,  yn~1}  to  at  least  the 
second  order.  Then,  as  for  the  set  1,  y,  ...,  y""1,  we  investigate  what  linearly  independent 
integral  functions  exist  of  the  form 


and  continue  the  process  for  v  as  for  u  :  and  afterwards  for  all  other  repeated  factors  of 

Aa,^...,^-1)- 

76.     When  these  processes  are  completed,  we  shall  obtain  a  set  of  integral  functions 

!>  »?]>  •••)  '/n-l) 

such  that  there  exists  no  integral  function  of  the  form 


*  In  the  work  below,  if  u  be  a  polynomial  of  order  r,  it  is  necessary  to  suppose  a,  a5  ,  ...,  a*  to 
be  polynomials  of  order  ?•—  1. 

+  The  number  of  steps  is  finite,  by  §  74. 


77]  FUNDAMENTAL   INTEGRAL    FUNCTIONS.  107 

wherein  a,  ...,  an_t  are  constants,  for  any  value  of  c.  It  is  obvious  now  from  the  successive 
definitions  (C),  (D),  ...  of  the  sets  (1,  ft,  ...,  fn-i)»  (1,  £1,  ...,£n-i),  ...,  (1,  ijlt  ...,  •;»_,),  that 
every  power  of  y  can  be  represented  in  the  form 


wherein  v,  vv,  ...,  vn_l  are  integral  polynomials  in  x.     Hence  every  integral  function  can 
be  written  in  the  form 

r,  =  (  A'+  El  r,,  +  .  .  .  +  En  _  l  r,n  _  J/F, 

wherein  E,  ...,  £!n-u  F  are  integral  polynomials  in  x  without  common  divisor.     If  now 
x—  c  be  a  factor  of  F  and  we  write 

Ei  =  (x-c)  (fi  +  ai,     i=0,  1,  2,  ...,  (n-  1), 
at  being  a  constant,  the  function 


is  an  integral  function,  as  appears  from  the  form  of  the  left-hand  side.  By  the  property 
of  the  set  1,  Vn  •••>  'Jn-i  there  is  no  integral  function  having  the  form  of  the  right-hand 
side,  unless  each  of  a,  alt  ...,  an_T  be  zero. 

Hence  each  of  E,  ...,En  _l  are  divisible  by  x  —  c.     By  successive  steps  of  this  kind  it 
can  be  shewn  that  every  integral  function  can  be  written  in  the  form 


1Tln-l,  (E) 

wherein  H,  fll,  ...,  Hn-i  are  integral  polynomials  in  x. 

77.  But  in  order  that  the  set  1,  rjl,  ...,  r}n_l  should  be  such  a  fundamental  set  as 
I>ffi>  •••>.9rn-i>  used  in  Chap.  IV.,  there  must  be  no  terms  occurring  on  the  right-hand  side 
here,  which  are  of  higher  dimension  than  rj.  We  prove  now  that  this  requires  a  further 
reduction  in  the  forms  of  1,  ^  ...,  rjn_l,  which  is  of  a  kind  precisely  analogous  to  the 
reductions  already  described. 

Let  a  +  1  be  the  dimension  of  17,  pf  the  order,  and  therefore  also  the  dimension  of  the 
polynomial  ZT(  (§  76)  and  a-i  +  l  the  dimension  of  ^;  we  suppose  o^  ^>  o-2  ;j>  ...  :j>  o-n_1  ; 
then 


Putting  #=!/£,  h=rtlx<T    ,  hi  =  rnlxT     ,  Hix~Pi=(\^)pit  an  integral  polynomial  in  £, 
this  equation  is 


If  now  in  equation  (E)  a  term  arises  of  higher  dimension  than  rj,  one  of  the  integers 

p  —  (o-  +  l),    ...,  pi  +  <Ti  —  O-,... 

is  greater  than  zero.     In  that  case  let  r+l  be  the  greatest  of  these  integers.     Then  we  can 
write 

^=(...+  (i,£Mi+.  ..)/£, 

wherein  the  symbols  (1,  £)mi  denote  integral  polynomials  in  £.     Putting 

(liflm^A'i  +  Oi,      (1  =  0,  1,  2,  ...,  w-1), 

wherein  a;  is  a  constant,  we  have 


Herein  the  left  hand  is  a  function  which  is  not  infinite  when  x  is  infinite.     Hence, 


108  ACTUAL  ALGEBRAICAL  DETERMINATION  OF  [77 

when  the  set  1,  r)l,  ...,rjn^l  are  such  that  the  condition  of  dimensions*  is  not  satisfied, 
there  exist  functions  of  the  form 

i.e.  of  the  form 


wherein  a,  ...,  an_!  are  constants  which  are  not  infinite  when  £  is  zero  or  x  is  infinite. 

In  virtue  of  their  definition  the  functions  hlt  ...,/;„_!  are  not  infinite  when  x  is  infinite, 
and  are  therefore  infinite  only  when  x  is  zero  or  £  infinite.  We  may  therefore  regard  them 
as  integral  functions  of  £.  And  since  there  exists  no  integral  function  of  the  form  rjifx,  the 
dimensions  of  klt  ...,hn_l  as  functions  of  £  are  o-j  +  1,  ...,  o-n_1  +  l. 

As  before  determine  a  set  of  linearly  independent  functions  of  the  form 


a,  ...,  an_j  being  constants,  which  are  not  infinite  when  £  =  0,  choosing  them  so  that  the  h 
of  highest  suffix  which  occurs  is  not  the  same  in  any  two  of  the  functions.  Let  the 
function  wherein  the  h  of  highest  suffix  is  hr  be  denoted  by  &,.,  so  that  kr  is  of  the  form 

kr  = 
Then 

^  =  ^+ 

is  a  function  which  is  not  infinite  when  #=0,  as  appears  from  the  form  of  the  right-hand 
side  ;  it  is  therefore  an  integral  function  of  x,  and  since  kr  is  not  infinite  when  x  is  infinite 
it  is  an  integral  function  of  x  whose  dimension  is  only  o>.  Denote  it  by  Qr.  Then  r)r  can 
be  expressed  in  the  form 

r          OY~f~l     i  OV  —  O"i     ,  (Tf  —  OV-  1          /-v   -\  /Tl\ 

T)r=  --  [fl*  +Wl*  l  +  ...+fi.r-^r-l«  ~  Gr],  (*) 

P-r 

and  in  the  right  hand  no  term  occurs  of  higher  dimension  than  that  of  i;r,  while  Gr  is  of 
less  dimension  than  r)r.  If  then  there  be  m  functions  such  as  kr,  m  of  the  functions 
i7u  ...,  ijn-i  can  be  expressed  in  the  form  (F)  in  terms  of  the  remaining  n  —  l  —  m  functions 
of  ijj,  ...,»;„_!  and  m  functions  Gr  ;  the  sum  of  the  dimensions  of  these  m  functions  Gr  is 
less  by  m  than  that  of  the  dimensions  of  the  functions  rjr  which  they  replace.  Denoting 
the  functions  among  i^,  ...,  tjn_l  which  are  not  thus  replaced  by  functions  G,  also  by  the 
symbol  G,  for  the  sake  of  uniformity,  every  integral  function  is  expressible  in  the  form 

(x,  l)A  +  (.r,  l)^Gl  +  ...  +  (x,  l^ffn-i, 

and  the  sum  of  the  dimensions  of  Gl,  ...,  Gn^l  is  less  by  m  than  the  sum  of  the  dimensions 
°f  »?i,  •••j'Jn-i- 

If  now  in  this  expression  of  integral  functions  by  Gly  ...,  Gn_1  any  terms  can  arise 
which  are  of  higher  dimension  than  the  functions  to  be  expressed,  we  can  similarly  replace 
the  set  G!,  ...,  Gn_l  by  another  set  whose  dimensions  have  a  still  less  sum. 

Since  no  integral  function  can  have  a  less  dimension  than  1,  the  sum  of  the  dimensions 
of  the  functions  whereby  integral  functions  are  expressed,  cannot  be  diminished  below  n  —  1. 
We  shall  therefore  arrive  at  length  at  a  set  glt  ...,^B_1  of  integral  functions,  in  terms  of 
which  all  integral  functions  can  be  expressed  so  that  the  condition  of  dimensions  is 
satisfied. 

It  is  this  system  which  it  was  our  aim  to  deduce. 

*  Chap.  IV.  §  39. 


78]  FUNDAMENTAL   INTEGRAL   FUNCTIONS.  109 

Ex.  For  the  surface  associated  with  the  equation  yz  =  (x,  l)2/>  +  2  a^  integral  functions 
can  in  fact  be  represented  in  the  form  (x,  l}^  +  (x,  l)AjVn  where  rjl=y->f-xm.  If  m>p  +  l 
the  dimension  of  ^  is  m.  In  order  to  ascertain  whether  the  condition  of  dimensions  is 
satisfied  we  enquire  whether  there  exist  any  functions  of  the  form  x  [a  +  a±  (y  +  .vm)/xm], 
wherein  a,  at  are  constants,  which  are  finite  for  >r  =  oo,  namely  whether  [a  +  a1(3/£m  +  !)]/£ 
can  be  an  integral  function  of  £. 

Shew  that  this  can  only  be  the  case  when  a  +  0^  =  0.  Putting  kr  =  [-a-lt-al(y^m  +  l)]l^ 
it  is  clear  that  kr.rm~l  =  aly.  Thus  all  integral  functions  can  be  represented  in  the  form 
(x,  !).+(#,  1).  y.  Shew  that  the  condition  of  dimensions  is  now  satisfied. 

78.  There  is  one  part  of  the  process  given  here  which  has  not  been  explained.  Let 
?;!,  ...,  r/n-!  be  integral  functions,  and  let  u  denote  a  linear  function  of  the  form  x  —  c.  It 
is  required  to  find  all  possible  functions  of  the  form 


wherein  a,  ...,  an_l  are  constants,  which  are  not  infinite  when  w  =  0.  We  suppose 
ij!,  ...,  »?„_!  to  be  such  that  the  product  of  every  two  of  them  is  expressible  in  the  form 
•v  +  vlrjl  +  ...  +  vn_lr)n_l,  v,  ...,  yn_!  being  integral  polynomials  in  x  ;  this  condition  is 
always  satisfied  in  the  actual  case  under  consideration. 

The  integral  function  //=  a  +  a17?1-|-...+an  _i»7»-i  will  satisfy  an  equation  of  the  form 
(H  -  HW]  ...(#-  fl»)  =  Hn  +  A\Hn   l  +  ...+  Kn  _  ,H+  Kn  =  0, 

wherein  A"i  is  an  integral  polynomial  in  a,  ...,  an_!  of  the  ith  order  ;  Ki  is  also  an  integral 
polynomial  in  x.  In  order  that  H/u  be  an  integral  function  it  is  sufficient  that  Kt  be 
divisible  by  u\  and  when  H/u  is  an  integral  function  these  n  conditions  will  always  be 
satisfied.  And  it  is  easy  to  see  that  if  Si  denote  the  sum  of  the  {th  powers  of  the  n  values 
of  H  which  arise  for  any  value  of  x,  these  conditions  may  be  replaced  by  the  conditions 
that  Si  be  divisible  by  u^  It  is  clear  that  it  may  not  be  an  easy  matter  to  obtain  the 
values  of  a,  ...,  an_!,  which  satisfy  the  conditions  thus  expressed. 

But  in  fact  these  conditions  can  be  reduced  to  a  set  of  linear  congruences,  and  event 
ually  to  a  set  of  linear  equations  for  a,  ...,  an_i.  We  shall  not  give  here  the  proof  of  this 
reduction*,  but  give  the  resulting  equations.  For  in  many  practical  cases  we  can  obtain 
the  results,  geometrically  or  otherwise,  in  a  much  shorter  way. 

Let 

/ 


denote  in  order  of  magnitude  all  the  positive  rational  numerical  fractions  not  greater  than 
unity,  whose  denominators  are  not  greater  than  n  ;  each  being  in  its  lowest  terms.  Let 
Tj!,  ...,  77,.  denote  any  linearly  independent  integral  functions.  Let  2  denote  the  sum  of  the 
n  values  of  a  function  which  arise  for  any  value  of  x.  Determine  all  the  possible  sets  of 
values  of  the  constants  a,  a1}  ...,  ar  such  that  the  congruence 

2(a  +  a1771  +  ...  +  ar77r)(c  +  c1771  +  ...  +  cr77r)  =  0     (mod.  u) 

is  satisfied  for  all  values  of  the  quantities  c,  clt  ...,  cr.  Substituting  in  the  left  hand  the 
value  of  x  for  which  u  =  0  and  equating  separately  to  zero  the  coefficients  of  c,  clt  ...,  cr,  we 
obtain  r-\-l  linear  equations  for  the  constants  a,  «j,  ...,  ar.  By  these  equations  we  can 

*  Which  is  given  by  Hensel,  Acta  Math.  18,  pp.  284  —  292.     His  use  of  homogeneous  variables 
is  explained  below  Chap.  VI.  §  85.    But  it  is  unessential  to  the  theory  of  the  reduction  referred  to. 


110  ACTUAL   ALGEBRAICAL   DETERMINATION  OF  [78 

express  a  certain  number*  of  a,  alf  ...,  ar  in  terms  of  the  others  ;  denoting  these  others  by 
ft,  ...,  ft  the  function  a  +  a^  +  .-.-fa,.^  takes  the  form  ftd  +  .-.+ftf*,  wherein  £lt  ...,  £, 
are  definite  linear  functions  of  1,  i^,  ...,  r)r  with  constant  coefficients,  and  the  equations  in 
question  are  then  satisfied  for  all  constant  values  of  ft, ...,  ft.  We  associate f  the  functions 

CD  •••)  f«  with  the  first  term  -  of  the  series  of  fractions  specified  above.   We  proceed  thence 

7i 

to  deduce  a  set  of  integral  functions  associated  with  the  next  term  of  the  series,  —     . 

?i  ~—    1 

But  in  order  to  be  able  to  describe  the  successive  processes  in  as  few  words  as  possible,  let 
us  assume  we  have  obtained  a  set  of  integral  functions  £j,  ...,  £m  which  in  the  sense 
employed  are  associated  with\  the  fraction  e  of  the  series,  and  wish  to  deduce  a  set  of 
functions  associated  with  the  next  following  fraction  of  the  series,  «'.  Put  down  the  con 
gruence 

2  (yi&  +  . ..+*»&»)  («i£i  +  .» +e,B&»)i-isO    (mod.  w^i). 

Herein  ylt  ...,  ym  denote  constants,  {denotes  in  turn  all  positive  integers  not  greater 
than  n  which  are  exact  multiples  of  the  denominator  of  the  fraction  e,  so  that  if  is  an 
integer,  \it'  denotes  the  least  integer  which  is  not  less  than  ie',  and,  for  any  proper  value 
of  ij  the  congruence  is  to  be  satisfied  for  all  values  of  the  quantities  ex,  ...,  em.  It  will  be 
found  in  practice  that  the  left-hand  side  divides  by  u]if' :~1  for  all  values  of  y15  ...,ym, 
%,...,  em.  If  we  carry  out  the  division,  then,  in  the  result,  substitute  the  value  of  x 

which  makes  u=0,  and  equate  separately  to  zero  the  coefficients  of  the  (  .       )  products  of 

\i—  l/ 

e1,  ...,  em  which  enter  on  the  left,  we  shall  have  this  number  of  linear  equations  for 
7u  •••>  ym-  Solving  these,  and  thereby  expressing  as  many  as  possible  of  yx,  ...,  ym  in 
terms  of  the  remaining,  which  we  may  denote  by  y/,  ...,  y'm>,  yi£i  +  ...  +  ym£m  will  take  a 
form  yi£i'  +  ...+y'm'gm',  wherein  y/,  ...,  y'm'  are  arbitrary  constants,  and  £/,  ...,  gm>  are 
definite  linear  functions  of  £ls  ...,  £m.  We  say  that  £/,  ...,  %m>  are  associated  with  the 
fraction  e'. 

This  process  is  to  be  continued  beginning  with  the  case  when  e--  and  ending  with  the 

Yi 

case  when  e'  =  l.  The  functions  associated  with  the  last  term,  1,  of  the  series  of  frac 
tions,  say  G!,  ...,  Gk,  are  all  the  functions  of  the  form  a  +  alr)l  +  ...  +  an ^lrjn_l,  wherein 
a,  als  ...,  an^l  are  constants,  which  are  such  that  GJu,  ...,  Gk/u  are  finite  when  u=0. 

For  the  case  »  =  3,  of  a  surface  of  three  sheets,  the  series  is  J,  |,  |,  1.  The  successive 
congruences  may  therefore  be  denoted  by 

(S2)  =  0  (mod.  it),  (S3)  =  0  (mod.  w2),  (>S'2)  =  0  (mod.  w2),  (S3)  =  0  (mod.  «3), 
wherein  (S^  denotes  such  an  expression  as  2  (yili  +  ...+y,»|m)  (^i^i  +  '-'+^n^mY'1- 

In  fact  3  is  the  only  integer  not  greater  than  3  such  that  3.  ^  is  integral  and  |3 .  £|  =  2. 
And  2  is  the  only  integer  not  greater  than  3  such  that  2 .  £  is  integral  and  1 2 .  §  |  =•  2  ; 
finally  3  is  the  only  integer  such  that  3 .  §  is  integral,  and  1 3 .  1 1  =  3. 

For  a  surface  of  four  sheets  the  fractions  are 

i,  J,  i,  §,  I,  i. 

*  At  most,  and  in  general,  equal  to  r. 

\_ 
t  In  a  certain  sense  the  functions  f1?  ...,  £,  are  all  divisible  by  u«. 

+  Divisible  by  xf,  in  a  sense. 


79]  FUNDAMENTAL    INTEGRAL   FUNCTIONS. 

We  therefore  have 


111 


1 

<' 

t  such  that  it  =  integral 

M 

congruence 

0 

i 

t  =  2 

i 

(^sO  (mod.  %) 

i 

ft 

?:=4 

1^1  =  2 

(*S4)  =  0  (mod.  «2) 

1 

i 

t  =  3 

If  =2 

(£3)  =  0  (mod.  M2) 

i 

1 

{=4 

I!!-. 

(52)  =  0(mod.  w2) 

§ 

1 

M 

l!l  =  3 

(*S"3)  =  0  (mod.  u3) 

1 

1 

;=4 

141=4 

(*S"4)  =  0  (mod.  w4) 

It  must  be  borne  in  mind  that  the  results  of  the  solution  of  each  of  the  seven  con 
gruences  of  the  sequence  in  the  right-hand  column,  are  here  supposed  to  be  substituted  in 
the  next  one  :  so  that,  for  instance,  the  fourth  congruence  here  may  be  quite  other  than  a 
slightly  harder  case  of  the  first  congruence. 

Ex.     Prove  that  for  a  surface  of  five  sheets  the  congruences  are,  in  order, 

(I)  (S2)  =  0  (,  «);    (2)  (S5)  =  0  (,  O;    (3)  (S4)  =  0  (,  «2)  ;  (4)  (S3)  =  0  (,  «**)  ;  (5)  (S5)  =  0  (,  w3); 
(6)(S2)  =  0(,«2);  (7)(S4)  =  0(,«3);  (8)(^5)  =  0(,^;  (9)  (S3)  =  0  (,*»);  (10)  (S4)  =  0  (,  ««); 

(II)  (^  =  0  (,M6). 

79.     Ex.  i.     Prove  for  the  equation  y*=xz  (x—  1)  that  A  (1,  y,  y2,  y3)  =  —  256  a6  (.r  —  I)3. 
Shew  that  the  equations 

2  (a  +  a^y  +  azf  +  atf3)*  =  0  (mod.  (x  -  1  )«), 

where  a,  an  a2,  a3  are  constants,  and  i  is  in  turn  equal  to  1,  2,  3,  4,  are  only  satisfied  by 
a  =  aj  =  o2  =  a3  =  0. 

Shew  that  the  equations 

2  O  +  fty  +  ft^  +  flsy^O  (mod.  a*), 

where  0,  ft,  ft,  ft  are  constants,  and  i  is  in  turn  equal  to  1,  2,  3,  4,  require  0=ft  =  0  and 
leave  ft  and  ft  arbitrary.     Hence  y-  ,  ^  are  the  only  integral  functions  of  the  form 


Shew  that  the  equations 

2  (-y+yi3/+72  ^+y3  7)*  =  *)  (mod.  **) 

\  &          x  j 

require  y=y1  =  y2=y3=o. 

Prove  that  the  dimensions  of  1,  y,  y-  ,  y-  are  0,  1,  1,  2.     Prove  then  that  there  is  no 

X          X 

function  of  the  form 


which  is  finite  for  x  infinite. 


112  EXAMPLES.  [79 

Hence  1,  y,  —  ,   —  are  a  fundamental  system  such  as  1,  gv,  #2,  9z  m  Chap.  IV.  ;  and 

(C          X 

the  deficiency  of  the  surface  is  1  +  1  +  2  •-  (4  -  1  )  =  1  . 

Ex.  ii.     In  partial  illustration  of  Hensel's  method  of  reduction  consider  the  case  of  the 
equation 

f  -  3^/2  +  3y.v  (x  -  1  )  +  x*  (x  -  1  )2  (O.^3  +  7.v2  +  5.r  +  3)  =  0, 

for  which  the  sums  of  the  powers  of  y  are  given  by 
s  =  3.r     s  =  3#2  +  fix     s  =  - 


The  determinant  A  (1,  y,  j/2)  is  divisible  by  .r3  and  by  (x  —  I)2,  as  appears  on  calculation. 
By  forming  the  equation  satisfied  by  yl\x  it  appears  that  y^jx  is  an  integral  function. 
Denote  it  by  r).  We  consider  now  what  functions  exist  of  the  form 

(a  +  atf  +  a2  rf)l(x  -1), 
wherein  a,  a1?  a2  are  constants,  which  are  integral  functions. 

The  congruence   (S2)  =  2  (a  +  a^  +  a^)  (c  +  clty  +  e2^)  =  0  (mod.  .r-1)  leads,   considering 
the  coefficients  of  c,  cn  c2  separately,  to  the  congruences 


s1  +  a2-0(  ,.r-  1),  a^ 
and  therefore  to  the  equations 


which  give  a  =  0,  ax=  —  3a2,  and  shew  that  the  only  function  of  the  kind  required  is,  save 
for  a  constant  multiplier, 

(,-%)/(*-  1). 

The  other  three  congruences  reduce  then  to  conditions  for  this  function  ;  for  example, 
the  congruence  (£3)  =  0(  ,  ^2)  becomes 


_x(x  —  1)      x—  1 

But  in  fact,  if  we  write  g  =  (y^-Zxy}jx  (x-\\   A  =  dx3  +  7.£2  +  5.v  +  3,  we  immediately 
find  from  the  original  equation  that 

g3  +  §gi _ fy  (A.x -$)  +  Azx(x-l)  +  9 Ax  =  0, 
so  that  g  is  an  integral  function. 

Apply  the  method  to  shew  that  y*jx  is  the  only  integral  function   of  the   form 


Prove  that  the  dimensions  of  the  functions 


are  respectively  0,  3,  3. 

Putting  a?  =  1/|,  y/.r3  =  A,  examine  whether  there  exists  any  integral  function  of  £  of 
the  form 

[a  +  aiA  +  3a2  (A2-3£%)/£  (! 

and  deduce  the  fundamental  integral  functions. 
The  deficiency  of  the  surface-  is  3  +  3  -(3-1)  =  4. 


81] 


CHAPTER  VI. 

GEOMETRICAL  INVESTIGATIONS. 

80.  IT  has  already  been  pointed  out  (§  9)  that  the  algebraical  equation, 
associated  with  a  Riemann  surface,  may  be  regarded  as  the  equation  of  a 
plane  curve ;  for  the  sake  of  distinctness  we  may  call  this  curve  the  funda 
mental  curve.     The  most  general  form  of  a  rational  function  on  the  Riemann 
surface  is  a  quotient  of  two  expressions  which  are  integral  polynomials  in 
the  variables  (x,  y)  in  terms  of  which  the  equation  associated  with  the  surface 
is  expressed.     Either  of  these  polynomials,  equated  to  zero,  may  be  regarded 
as  representing  a  curve  intersecting  the  fundamental  curve.     Thus  we  may 
expect  that  a  comparison  of  the  theory  of  rational  functions  on  the  Riemann 
surface  with  the  theory  of  the  intersection  of  a  fundamental  curve  with  other 
variable  curves,  will  give  greater  clearness  to  both  theories. 

In  the  present  chapter  we  shall  make  full  use  of  the  results  obtainable 
from  Riemann's  theory  and  seek  to  deduce  the  geometrical  results  as  con 
sequences  of  that  theory. 

81.  The   converse  order  of  development,  though   of  more   elementary 
character,  requires  much  detailed  preliminary  investigation,  if  it  is  to  be 
quite  complete,  especially  in  regard  to  the  theory  of  the  multiple  points 
of  curves.     But  the  following  account  of  this  order  of  development  may  be 
given  here  with  advantage  (§§  81 — 83).     Let  the  term  of  highest  aggregate 
degree  in  the  equation  of  the  fundamental  curve f(y,  #)  =  0  be  of  degree  n; 
and,  in  the  usual  way,  regard  the  equation  as  having  its  most  general  form 
when  it  consists  of  all  terms  whose  aggregate  degree,  in  x  and  y,  is  not 
greater  than  n;   this  general  form  contains  therefore  £(7i+l)(w  +  2)  terms. 
Suppose,  further,  that  the  curve  has  no  multiple  points  other  than  ordinary 
double  points  and  cusps,  8  being  the  number  of  double  points  and  K  of  cusps. 
Consider  now  another  curve,  ty  (x,  y)  =  0,  of  order  m,  whose  coefficients  are 
at  our  disposal.     By  proper  choice  of  these  coefficients  in  -v/r  we  can  determine 
xp-  to  pass  through  any  given  points  of  y,  whose  number  is  not  greater  than 
the  number  of  disposeable  coefficients  in  -v|r.     Let  k  be  the  number  of  the 
prescribed  points,  and  interpret  the  infinite  intersections  of /and  >/r,  in  the 
usual  way,  so  that  their  total  number  of  intersections  is  raw.     Then  there 

B.  8 


114  INTRODUCTORY  SKETCH.  [81 

remain  mn  —  k  intersections  of  /  and  i/r  which  are  determined  by  the  others 
already  prescribed.  We  proceed  to  prove  that  if  m  >  n  —  3,  and  if  we  utilise 
all  the  coefficients  of  -fy  to  prescribe  as  many  of  the  intersections  of  -^  andy 
as  possible,  and  introduce  further  the  condition  that  i/r  shall  pass  once  through 
each  cusp  and  double  point  off,  then  the  number  of  remaining  intersections 
which  are  determined  by  the  others  will  be  p  =  ^  (n  —  1)  (n  —  2)  —  B  —  K*,  for 
all  values  of  m.  For,  if  m  ^  n,  the  intersections  of  ty  with  f  are  the  same  as 
those  of  a  curve 

^  +  Um_nf=  0, 

wherein  Um_n  is  any  integral  polynomial  in  the  coordinates  a;  and  y,  in  which 
no  term  of  higher  aggregate  dimension  than  m  —  n  occurs.  By  suitable 
choice  of  the  ^  (m  —  n  +  1)  (m  —  n  +  2)  coefficients  which  occur  in  the  general 
form  of  Um-n  we  can  reduce  ^  (m—n  +  l)(m  —  n  4-  2)  coefficients  in  \jr+  Um-nf 
to  zero-f".  It  will  therefore  contain,  in  its  new  form, 

M  +  I  =  1  +  \m  (m  +  3)  -  £  (m  -  n  +  1)  (m  -  n  +  2) 

arbitrary  coefficients.  M  is  therefore  the  number  of  the  intersections  of  ^r 
with  f  which  we  can  dispose  of  at  will,  by  choosing  the  coefficients  in  >/r 
suitably.  Of  these  intersections,  by  hypothesis,  2  (8  +  K)  are  to  be  taken 
at  the  double  points  and  cusps  of  the  curve  /.  This  can  be  effected  by  the 
disposal  of  £  +  K  of  the  arbitrary  coefficients.  There  remain  then 

1  +  \m  (m  +  3)  -  \(m  -  n  +  1)  (m  -  n  +  2)  -  8  -  tc 

disposeable  coefficients  and  mn  —  2  (8  +  K)  intersections.     Of  these,  therefore, 
mn  -  2  (8  +  K)  -  [|  m  (in  +  3)  -  \(m  -  n  +  1)  (m  -  n  +  2)  -  B  -  K] 

is  the  number  of  intersections  determined  by  the  others  which  are  at  our 
disposal ;  and  this  number  is 

£(n-l)(n-2)-(S  +  *). 

In  case  m  <  n,  of  the  mn  —  2  (8  +  K)  intersections  of  ty  with  f,  which  are 
not  at  the  double  points  or  cusps  of  y,  we  can,  by  means  of  the  ^w(m+3)— 8— K 
coefficients  of  ^r  which  remain  arbitrary  when  ty  is  prescribed  to  vanish  at 
each  double  point  and  cusp,  dispose  of  all  except 

mn  -  2  (S  +  K)  -  [|ra  (m  +  3)  -  (8  +  K)]  ; 
when  m  =  n  —  1  or  n  —  2  it  is  easily  seen  that  this  is  the  same  as  before. 

82.  Let  us  assume  now  that  the  polynomials  which  occur,  as  the  nume 
rator  and  denominator,  in  the  expression  of  a  rational  function,  have  the 

*  Reasons  are  given,  Forsyth,  Theoi-y  of  Functions,  p.  356,  §  182,  for  the  conclusion  that  this 
number  is  the  deficiency  of  the  Riemann  surface  having  /  (y,  x)  =  Q  as  an  associated  equation. 
We  shall  assume  this  result. 

t  As,  for  instance,  the  coefficients  of  ym,  ijm~\  ym^x,  ...,  yn,  ynx,  ...,  ynxm'n,  in  which  case 
the  highest  power  of  y,  in  ^+  */„,_„/,  that  remains,  is  yn~l. 


83]  INTRODUCTORY  SKETCH.  115 

property  here  assigned  to  ty,  of  vanishing  once  at  each  double  point  and 
cusp  of/  Without  attempting  to  justify  this  assumption  completely,  we 
remark  that  if  it  is  not  verified  at  any  particular  double  point,  the  rational 
function  will  clearly  take  the  same  value  at  the  double  point  by  whichever  of 
the  two  branches  of  the  curve  /  the  double  point  be  approached.  As  a 
matter  of  fact  this  is  not  generally  the  case.  Suppose  then  we  wish  to  obtain 
a  general  form  of  rational  function  which  has  Q  given  finite  points  of 
/,  A  !,...,  AQ,  as  poles  of  the  first  order.  Draw  through  these  poles, 
Alt  ...,  AQ,  any  curve  ty  whatever,  of  degree  greater  than  n  —  3,  which  passes 
once  through  each  double  point  and  cusp  off.  Then  ty  will  intersect  /  in 

mn  -  2  (8  +  *)  -  Q 

other  points  Blt  B2,  ....  Through  these  other  points  Blt  _B2>  •••  off,  and 
through  the  double  points,  draw  another  curve,  S-,  of  the  same  degree  as  ty. 
The  curve  ^  will  in  general  not  be  entirely  determined  by  the  prescription 
of  the  mn  —  2  (8  +  K)  —  Q  points  B1}  -B2,  ____  Let  the  number  of  its  coefficients 
which  still  remain  arbitrary  be  denoted  by  q  +  1.  Then  it  would  be  possible 
by  the  prescription  of,  in  all, 

mn  -  2  (S  +  K)  -  Q  +  q 

points  of  ^,  to  determine  ^  completely.  But  by  what  has  just  been  proved, 
S-  is  determined  completely  when  all  but  p  of  its  intersections  are  prescribed. 

Wherefore 

mn  -  2  (8  +  K)  -  Q  +  q  =  mn  -  2  (S  +  «)  -  p. 

Hence  Q  —  q  =  p,  and  ^  has  the  form 


where  X,  \lt  .  .  .  ,  X^  are  arbitrary  constants  and  -v/r,  S-1}  .  .  .  ,  ^9  are  q  +  1  linearly 
independent  curves,  all  passing  through  the  mn  —  2  (8  +  K)  —  Q  points 
BI,  B.2,  ...,  as  well  as  through  the  double  points  and  cusps;  and  the  general 
rational  function  with  the  Q  prescribed  poles  will  have  the  form 

X  +  Xj  .Rj  +  .  .  .  +  ^qRq  , 

where  Ri  =  ^/i|r  ;  and  this  function  contains  q  +  1  arbitrary  coefficients. 


83.  In  this  investigation,  which  is  given  only  for  purposes  of  illustration,  we  have 
assumed  that  the  prescription  of  a  point  of  a  curve  determines  one  of  its  coefficients  in 
terms  of  the  remaining  coefficients,  and  that  the  prescription  of  this  one  point  does  not  of 
itself  necessitate  that  the  curve  pass  through  other  points  ;  and  we  have  obtained  not 
the  exact  form  of  the  Riemann-Roch  Theorem  (Chap.  III.  §  37),  but  the  first  approxima 
tion  to  that  theorem  which  is  expressed  by  Q  —  q=p;  this  result  is  true  for  all  cases  only 
when  Q>n(n-3)-2(8  +  ic). 

We  may  illustrate  the  need  of  the  hypothesis  that  the  curves  x//-  and  ^  pass  through  the 
double  points  and  cusps,  by  considering  the  more  particular  case  when  the  fundamental 
curve 

/=(#»  y)2  +  (a»  y\  +  fa  y)4  =  °> 

8—2 


116  INTRODUCTORY.  [83 

wherein  (x,  y\  is  an  integral  homogeneous  polynomial  in  x  and  y  of  the  second  degree,  etc., 
is  a  quartic  with  a  double  point  at  the  origin  #=0,  y  =  0.  Since  here  «=4  and  8  +  K  =  l, 

we  have 

j»-$(»-l)(n-2)—&-*-i.3.2-l-«, 

and  therefore  (in  accordance  with  Chap.  III.  §§  23,  24,  etc.)  there  exists  a  rational  function 
having  any  three  prescribed  points  as  poles  of  the  first  order.  Let  us  attempt  to  express 
this  function  in  the  form  ^/\/^,  wherein  ^,  ^  are  curves,  of  degree  m,  (m>l),  which  do  not 
vanish  at  the  double  point.  Beside  the  three  prescribed  poles  A^  A2,  A3  of  the  function, 
^  will  intersect/  in  4m  —  3  points  Bv,  JB2,  ....  The  intersections  with  /  of  the  general 
curve  ^  of  degree  TO,  are  the  same  as  those  of  a  curve 


provided  TO  <•:  4,  and  are  therefore  determined  by  ^TO(m  +  3)—  £'(m  —  4  +  1)  (m  —  4  +  2),  or 
4m  —  3  of  them.  And  it  is  easily  seen  that  the  same  result  follows  when  m=3  or  2. 
Hence  no  curve  ^  can  be  drawn  through  the  points  Slt  B2,  ...  other  than  the  curve  \//-, 
which  already  passes  through  them  ;  and  the  rational  function  cannot  be  determined  in 
the  way  desired.  It  will  be  found  moreover  that  this  is  still  true  when  the  hypothesis, 
here  made,  that  ^  and  ^-  shall  be  of  the  same  degree,  is  allowed  to  lapse.  As  in  the 
general  case,  this  hypothesis  is  made  in  order  that  the  function  obtained  may  be  finite  for 
infinite  values  of  x  and  y. 

A  curve  which  passes  through  each  double  point  and  cusp  of  the  fundamental  curve  / 
is  said  to  be  adjoint.  When  /  has  singularities  of  more  complicated  kind  there  is  a  corre 
sponding  condition,  of  greater  complexity.  For  example  in  the  case  of  the  curve 


which,  in  the  present  point  of  view,  we  regard  as  a  quartic,  there  is  a  singularity  at  the 
infinite  end  of  the  axis  of  y.  If,  in  the  usual  way,  we  introduce  the  variable  z  to  make  the 
equation  homogeneous,  and  then*  put  3/  =  l,  whereby  the  equation  becomes 


we  see  that  the  branches  are,  approximately,  given  by  z—  ±  &r2,  namely  there  is  a  point  of 
self  contact,  the  common  tangent  being  2  =  0.  If  we  assume  that  it  is  legitimate  to  regard 
this  self  contact  as  the  limit  of  two  coincident  double  points,  we  shall  infer  that  the  condi 
tion  of  adjointness  for  a  curve  ^  is  that  it  shall  touch  the  two  branches  of  /  at  the  point. 
For  example  this  condition  is  satisfied  by  the  parabola 


which,  by  the  same  transformation  as  that  above,  reduces  to 

z  =  ax2  +  bxz  +  cz2, 

and  it  is  obvious  that  the  four  intersections  with  /  of  this  parabola,  other  than  those  at 
the  singular  point,  are  determined  by  all  but  p  of  them,  p  being  in  this  case  equal  to  1. 

We  shall  see  in  this  chapter  that  we  can  obtain  these  results  in  a  somewhat  different 
way:  the  equation  y2  =  (l  —  x2)  (1—  £2#2)  is  a  good  example  of  those  in  which  it  is  not 
convenient  to  regard  the  equation  as  a  particular  case  of  a  curve  of  degree  equal  to  the 
highest  degree  which  occurs.  Though  this  method,  of  regarding  any  given  curve  as  a 
particular  case  of  one  whose  degree  is  the  degree  of  the  highest  term  which  occurs  in  the 
given  equation  of  the  curve,  is  always  allowable,  it  is  often  cumbersome. 

Ex.  1.  Prove  that  the  theorem,  that  the  intersections  with  /  of  a  variable  curve  ^  are 
determined  by  all  but  p  of  them,  may  be  extended  to  the  case  where  /  has  multiple  points 

*  This  process  is  equivalent  to  projecting  the  axis  y  =  0  to  infinity. 


84]  THE   ASSOCIATED   EQUATIONS.  117 

of  order  k,  with  separated  tangents,  by  assuming  that  the  condition  of  adjointness  is  that 
i//-  should  have  a  multiple  point  of  order  k  —  1  at  every  such  multiple  point  of  /,  whose 
tangents  are  distinct  from  each  other  and  from  those  of/.  (In  this  case  any  such  multiple 
point  of/  furnishes  a  contribution  \k  (k  —  1)  to  the  number  5-f  K  of/.) 

Ex.  2.  The  curve  y*=(x,  1)6  may  be  regarded  as  a  sextic.  Shew  that  the  singular 
point  at  infinity  may  be  regarded  as  the  limit  of  eight  double  points,  and  that  a  general 
adjoint  curve  is 


Ex.  3.     Shew  that  for  the  curve  tf  =  (x,  l)2p  +  2  a  general  adjoint  curve  is 


For  further  information  on  this  subject  consult  Salmon,  Higher  Plane  Curves  (Dublin, 
1879).  pp.  42—48,  and  the  references  given  in  this  volume,  §  9  note,  §  93,  §  97,  §  112  note, 


84.  In  the  remaining  analytical  developments  of  this  chapter  we 
suppose*  the  equation  associated  with  the  Riemann  surface  to  be  given  in 
the  form 

f(y,  *)  =  y»  +  3r-'(*,  l)Al  +  ...+y(a;,  1)^  +  0,  l)An=0, 

so  that  y  is  an  integral  function  of  x.  Let  a-  +  1  be  the  dimension  of  y  ; 
then  cr  +  1  is  the  least  positive  integer  such  that  y/or+l  is  finite  when  x  is 
infinite;  thus  if  we  put  #=l/f  and  y=i)  !%*+*,  a  -f  1  is  the  least  positive 
integer,  such  that  77  is  an  integral  function  of  £.  This  substitution  gives 
f(y,  x)=Z-n{°+vF(r),  a  where 


so  that  cr  +  1  is  the  least  positive  integer  which  is  not  less  than  any  of  the 
quantities 

X1}  X2/2,  ...,  Xn_j/(n  -  1),  \n/n. 

Ex.  1.     For  the  case 


the  dimension  of  y  as  an  integral  function  of  x  is  3.     Writing  y  =  r)/£3,  where  •£=!/£,  the 
equation  becomes 


and  Tj  is  an  integral  function  of  £  of  dimension  2.     In  fact  yi  =  v/!2=y/#  satisfies  the 
equation 

yf+yi*(x,  i)3+yi(*,  i)4+(-»»  1)5=° 

and  is  finite  when  £  =  oo  ,  or  #  =  0. 

Ex.  2.     Shew  that  in  the  case  in  which  the  equation  associated  with  the  Riemann 
surface  contains  y  to  a  degree  equal  to  the  highest  aggregate  degree  which  occurs,  o-  =  0. 

*  Chap.  IV.  §  38. 


118  HOMOGENEOUS  VARIABLES.  [84 

Whenever  we  are  considering  the  places  of  the  surface  for  which  x  =  oo  , 
we  shall  consider  the  surface  in  association  with  the  equation  F(r),  £)  =  0  ; 
and  shall  speak  of  the  infinite  places  as  given  by  f  =0.  The  original  equation 
is  practically  unaffected  by  writing  x  —  c  for  x,  c  being  a  constant.  We  may 
therefore  suppose  the  equation  so  written  that  at  x  =  0,  the  n  sheets  of 
the  surface  are  distinct  ;  and  may  speak  of  the  places  x  =  0  as  the  places 


85.  By  the  simultaneous  use  of  the  equations  f(y,  #)  =  0,  F(r),  £)  =0, 
we  shall  be  better  able  to  formulate  our  results  in  accordance  with  the  view, 
hitherto  always  adopted,  whereby  the  places  x  =  oo  are  regarded  as  exactly 
like  any  finite  places.  But  it  should  be  noticed  that  both  these  equations 
may  be  regarded  as  particular  cases  of  another  in  which  homogeneous  variables, 
of  a  particular  kind*,  /are  used.  For  put  x  =  ajfz,  y  =  u/z<r+1;  we  obtain 
)  =  g-n«r+D  U(u;  to,  z\  where 

U  (u\  «,  z)  =  un  +  M»-IS<H-I-*I  (w,  z)Kl  +  ...+  uz«l-v  <<H-I)-AH_,  (Wj  ^^_i 


and  it  is  clear  that  U(u;  &>,  z)  is  changed  into  f(y,  so)  by  writing  u  =  y, 
&>  =  #,  z=l,  and  is  changed  into  F(rj,  £)  by  writing  u  =  t),  co  =  1,  z  =  g. 
We  may  speak  of  w,  z  as  forms,  of  degree  1,  and  suppose  that  they  do  not 
become  infinite,  the  values  x  =  oo  being  replaced  by  the  values  z  =  Q.  When 
<»,  z  are  replaced  by  ta>,  tz,  t  being  any  quantity  whatever,  u  is  replaced  by 
ta+1u,  y  and  x  remaining  unaltered.  We  may  therefore  speak  of  u  as  a  form 
of  degree  a  +  1. 

Similarly  U  (u  ;  o>,  z)  is  a  form  of  degree  n  (o-  +  l),  being  multiplied  by 
£tt(<r+D  when  u,  to,  z  are  replaced  by  t*+1u,  tta,  tz  respectively.  That  there 
is  some  advantage  in  using  such  homogeneous  forms  to  express  the  results  of 
our  theory  will  sufficiently  appear;  but  it  seems  proper  that  the  results 
should  first  be  obtained  independently,  in  order  that  the  implications  of  the 
notation  may  be  made  clear.  We  shall  adopt  this  course. 

Some  examples  of  the  change  which  our  expressions  will  undergo  when 
the  results  are  expressed  by  homogeneous  forms,  may  be  fitly  given  here  :  — 
Instead  off(y,  x)  we  shall  have  U(u;  w,  z)  which  is  equal  to  zn(<T+l]f(y,  sc)\ 
instead  of/'  (y)  we  shall  have  U'  (u)  =  z(n~1}  (*+*>/'  (y}  ;  instead  of  the  integral 
function  *f  ^,  of  dimension  T{  +  1,  an  integral  form  ^  of  degree  r;+l,  equal 
to  zTi+1gi,  will  arise  ;  since  2  (rf  +  1)  =  n  +p  —  1,  it  is  easy  to  see  that  the 
determinant  J  A  (1,  glt...,  <7n-i)  is  equal  to  ^2n+^~2  A  (1,  #1,...,  g^).  In 
accordance  with  §  48,  Chap.  IV.  the  former  determinant  will  have  a  factor 

*  This  homogeneous  equation  is  used  by  Hensel.     See  the  references  given  in  Chap.  IV. 
(§  42).     It  may  be  regarded  as  a  generalization  of  the  familiar  case  when  <r  =  Q. 
t  Chap.  IV.  §  42. 
J  Chap.  IV.  §  43. 


86]  HOMOGENEOUS   VARIABLES.  119 

(&)— cz)r  corresponding  to  a  finite  branch  place  of  order  r  where  x  =  c,  and  a 
factor  z8  corresponding  to  a  branch  place  of  order  s  at  x  =  oo .  Further,  if, 
by  the  formula  (H)  of  page  63,  we  calculate  the  form  fa  (u,  co,  z)  from 
glt  ...,  gn-i,  as  fa(x,  y)  is  there  calculated  from  glt  ...,  gn-\,  it  is  easy  to  see 
that  we  obtain  a  form,  fa(u,  w,  z),  which  is  equal  to  zin~1)(a+1)~(Ti+l}  fa(x,  y). 
Hence  also,  if  ult  <olt  zl  denote  special  values  of  u,  co,  z,  the  integral 

[zdw  —  o)dz    fjr1  fa  (u^o),  z)  +  S/A^  fa  (u,  <*,  z)gr(u1>  o^,  z,) 
U1  (u)  oaZi  —  a>iZ 

wherein  /j,  =  (bo)  —  az}l(bwi  —  az}),  a  and  b  being  arbitrary  constants,  is  equal  to 
dx  .  z^  <-+'>    ^  fa  (x,  y)  +  2/^  (z1/z)Tr+^fa(g;) 


f 


{ -j/\  &  ?    (if nr 

I  V  J  4t&\     \W  *Aj\ 

\t/  /  •*•  \ 

and  is  thus  equal  to 

dx       Ar1  fa  (x, 


where  X  =  /jLzJz  =  (bx  —  a)/(bx1  -  a). 

If  in  this  we  put  6  =  0,  we  obtain  the  form  which  we  have  already  shewn 
to  be  part  of  the  expression  of  an  integral  of  the  third  kind  (Chap.  IV.  p.  67). 
But  if  we  put  6=1,  the  integral  is  exactly  what  we  have  already  deduced 
(Chap.  IV.  p.  70,  Ex.  1)  by  the  ordinary  process  of  putting  x—  !/(£-  a) 
and  regarding  %  as  the  independent  variable. 

We  may,  if  we  please,  further  specialise  the  quantities  co,  z,  of  which 
hitherto  only  the  ratio  has  been  used,  supposing*  them  defined  by 
o)=x((x  —  c),  z=I/(x—c),  where  c  is  a  constant.  Then  &>  —  cz—\. 

Ex.  1.  The  integral  of  the  first  kind  obtained  in  Chap.  IV.  §  45,  p.  67,  can  similarly 
be  written 


Ex.  2.     In   the  case  y2=(x,  l)2p  +  2>   wherein  y  is  of  dimension  p  +  1,  the  equation 
U  (u;  u>,  z)  =  0  is 

v?  =  (a>,  2)2P+2 
obtained  by  putting  y  =  u/zp'*'1,  x=a>/z. 

86.  We  shall  be  largely  concerned  here  with  rational  polynomials  which 
are  integral  in  x  and  y.  The  values  of  such  a  polynomial  here  considered 
are  only  those  which  it  has  for  values  of  y  and  x  satisfying  the  fundamental 
equation.  We  shall  therefore  suppose  every  integral  polynomial  in  x  and  y 
reduced,  by  means  of  the  fundamental  equation,  to  a  form  in  which  the 
highest  power  of  y  which  enters  is  yn~l,  say  to  a  form 


*  In  this  view  u  and  z  are  functions.     If  we  regard  c  as  throughout  undetermined,  we  may 
regard  these  functions  as  having  no  definite  infinities. 


120  THE   GRADE   OF    A    POLYNOMIAL.  [86 

If  herein  we  write  y  =  77/f°'+1,  #=  l/£,  cr  +  1  being,  as  before,  the  dimen 
sion  of  y  as  an  integral  function  of  x,  we  shall  obtain  -v^-  (y,  x)  =  £~°  ^  (77,  £), 
where  "^  (77,  £)  is  an  integral  polynomial  in  77  and  £  of  which  a  representative 
term  is 

^n+i  £G-(n-i-i}  (*+D-H(\t  ^  i=Qt  1?  ......  j  (n_1} 

and  G  is  the  positive  integer  equal  to  the  greatest  of  the  quantities 


Thus  (r  is  the  highest  dimension  occurring  for  the  terms  of  -fy  (y,  x), 
and  ¥  (77,  £)  is  not  identically  divisible  by  £.  The  dimension  of  the  integral 
function  -^  (y,  #)  may  be  G  ;  but  if  M*  (77,  £)  vanish  in  every  sheet  at  £  =  0, 
the  dimension  of  ty(y,  x)  will  be  less  than  G.  For  this  reason  we  shall 
speak  of  G  as  the  grade  of  ty  (y,  x).  It  is  clear  that  if  all  the  values  of  TJ 
for  £  =  0  be  distinct,  that  is,  if  Ff  (77)  do  not  vanish  for  any  place  £  =  0,  the 
polynomial  M/"  (77,  £),  of  order  ?i  —  1  in  77,  cannot  vanish  for  all  the  n  places 
f=  0.  In  that  case  the  grade  and  the  dimension  of  ty  (y,  x}  are  necessarily 
the  same.  Further,  by  the  vanishing  of  one  of  the  coefficients,  a  polynomial 
of  grade  G  may  reduce  to  one  of  lower  grade.  In  this  sense  a  polynomial  of 
low  grade  may  be  regarded  as  a  particular  case  of  one  of  higher  grade. 

In  what  follows  we  shall  consider  all  polynomials  whose  grade  is  lower 
than  (n  —  1)  a-  +  n  —  3  or  (n  —  1)  (cr  +  1)  —  2,  as  particular  cases  of  polynomials 
of  grade  (n  —  1)  cr  +  n  —  3  :  the  general  expression  of  the  grade  will  therefore* 
be  (n  —  l)cr  +  n  —  3  +  r,  or  (n  -  1)  (<r  +  1)  +  r  —  2,  where  r  is  zero  or  a  positive 
integer.  The  most  general  form  of  a  polynomial  of  grade  (n  —  l)(cr+l)  +  r  —  2 
is  easily  seen  to  be 

i/r  (y,  x)  =  y^  (x,  l\_2  +  yn~°-  (x,  l\_,  +  ...+  yn-^  (x,  1)^  +  ...+(«,  l)r-i 


wherein  the  first  line  is  to  be  entirely  absent  if  r  =  0,  the  first  term  of  the 
first  line  is  to  be  absent  if  r  =  1,  and  the  first  term  of  the  second  line  is  to  be 
absent  if  cr  =  0. 

Hence  when  r  >  0,  the  general  polynomial  of  grade  (n  —  1)  cr  -f  n  —  3  +  r 
contains 

nr  -  1  +  £  (n  -  1)  (n  -  2  +  na) 

terms,  this  being  still  true  if  cr  =  0  ;  but  when  r  =  0,  the  general  polynomial 
of  grade  (n  —  1)  a  +  n  —  3  contains 


terms.     This  is  not  the  number  obtained  by  putting  r  =  0  in  the  number 
obtained  for  r  >  0. 

*  The  number  is  written  in  the  former  way  to  point  out  the  numbers  for  the  common  case 
when  (r  =  0. 


87]  GENERALIZED   ZEROS.  121 

Further,  putting 


,  x)  =  g-ct-w-c^-v-ripfa  f), 

and  denoting  the  aggregate  number  of  zeros  of  "SP  (77,  £)  at  £  =  0  by  /z,  it 
is  clear  that  the  aggregate  number  of  infinities  of  i/r  (y,  x)  at  x  =  oo  is 
[(n  —  1)  a-  +  n  —  3  +  r]n  —  p.  Since  ty  (y,  x)  is  only  infinite  for  x  =  oo  ,  this 
is  also  the  total  number  of  zeros  of  ty  (y,  x).  We  shall  find  it  extremely 
convenient  to  introduce  a  certain  artificiality  of  expression,  and  to  speak 
of  the  sum  of  the  number  of  zeros  of  ty(y,  a)  and  the  number  of  zeros  of 
^  C7?.  |)  at  £  =  0  as  the  number  of  generalized  zeros  of  -\/r  (y,  x).  This  number 
is  then  n  (n  -  1)  (a  +  1)  -f  n  (r  -  2). 

If  by  a  change  in  the  values  of  the  coefficients  in  ty  (y,  x),  "V  (77,  £  ) 
should  take   the  form   If^i  (77,  £)  where  ^1(77,  &)qJ£c(,f7  integral  polynomial 

in  77  and  £  so  that  ^  (y,  x)  is  w->  .  •  {  l^/,/v      ^  (77,  £),  the  sum  of 

,,  -i          f  n    •/  „  >~iial  for  the  surface         \y>  %,        ^ 

the  number  of  finite  zeros  of  x.  „  fc-"p.       of  zeros  of  YI  (77,  f  ) 

«        '--'.9\    ..9_      2    I     Vi^fZ-    ?  »\»»    >/ 

is   »i(w-  l)(o-+l)  +  n(r-3).     i^ut,  a.^  ,   c,;  is  equal    to  ^(77,  f), 

the  number  of  zeros  of  M/"  (77,  ^)  at  ^  =  0  is  ?i  more  than  the  number  of  zeros 
of  ^  (77,  f  )  at  £  =  0.  Hence  the  sum  of  the  number  of  finite  zeros  of  ty  (y,  x) 
and  the  number  of  zeros  of  M/"  (77,  ^)  at  £  =  0,  is  still  equal  to 

n  (n  -  1)  (o-  +  1)  +  ?i  (r  -  2). 


^r.  i.     The  number  n  (n-  1)  (<r  +  l)  +  ?t  (r-2)  is  clearly  the  number  of  zeros  of  the 
integral  form 


Ex.  ii.     The  generalized  number  of  zeros  of/'  (?/),  for  which  r  =  2,  is  71  (?i  —  1)  (o-  +  1). 
Ex.  iii.     The  general  polynomial  of  grade  d,  <  (n  —  1)  <r  +  ?i  —  3,  contains 

terms' 


^(x-)  being  the  greatest  integer  in  *\     Its  generalized  number  of  zeros  is  nd. 

87.     We  introduce  now  a  certain  speciality  in  the  integral  polynomials 
under  consideration,  that  known  as  adjointness. 

An  integral  polynomial  •x/r  (y,  x)  is  said  to  be  adjoint  at  a  finite  place 
(x  =  a,  y  =  b)  when  the  integral 


fyu/.a-1 
J    f(y} 


is  finite  at  this  place.     If  t  be  the  infinitesimal  at  the  place  (Chap.  I.  §§  2,  3) 
the  condition  is  equivalent  to  postulating  that  the  expression 


f'(y) 


122  ADJOINT   POLYNOMIALS.  [87 

shall  be  finite  at  the  place;   or  again  equivalent  to  postulating  that  the 
expression 

(x-a)^  (y,  x) 

f(y) 

shall  be  zero  at  the  place,  to  the  first  order  at  least. 

As  a  limitation  for  the  polynomial  i/r  (y,  x\  the  condition  is  therefore 
ineffective  at  all  places  where  /'  (y)  is  not  zero.  And  if  at  a  finite  place 
where  /'(y)  vanishes,  i  +  w  denote  the  order  of  zero  of  /'  (y\  w  +  I  being 
the  number  of  sheets  that  wind  at  this  place*,  the  condition  is  that  ty  (y,  x} 
vanish  to  at  least  order  i  at  the  place.  We  shall  call  ^i  the  index  of  the 
place  ;  the  condition  of  adjointness  is  therefore  ineffective  at  all  places 
of  zero  index. 

If  i/r  (y}  x}  be  of  grade  (n  —  1)  a-  +  n  —  3  +  r,  and 

t  (V,  *)  =  {-(^'-(K-V-r  V  (rj,  fr 

the  condition  of  adjointness  of  i/r  (y,  x)  for  infinite  places,  is  that,  at  all 
places  |  =  0  where  F'  (ij)  =  0,  the  function 


should  be  zero,  to  the  first  order  at  least.     It  is  easily  seen  that  this  is 
the  same  as  the  condition  that  the  integral 


fl 

J    of 


dx 


should  be  finite  at  the  place  considered. 

When  the  condition  of  adjointness  is  satisfied  at  all  finite  and  infinite 
places  where  f  (y)  =  0  or  F'  (77)  =  0,  the  polynomial  i/r  (y,  x)  is  said  to  be 
adjoint.  If  II  (x  —  a)  denote  the  integral  polynomial  which  contains  a 
simple  factor  corresponding  to  every  finite  value  of  x  for  which  f'(y)  vanishes, 
and  if  N  denote  the  number  of  these  factors,  it  is  immediately  seen  that  the 
polynomial  ty  (y,  x)  is  adjoint  provided  the  function 


is   zero,  to  the  first  order  at  least,  at  all  the  places   where  /'  (y}  =  0   or 
F'  (r,)  =0. 

Ex.  i.     For  the  surface  associated  with  the  equation 

/  (y,  #)  =  to  y\  +  to  y  )3  +  to  y\  =-•  ° 

there  are  two  places  at  x=Q,  at  each  of  which  y  =  0.    At  each  of  these  places  /'(y)  vanishes 
to  the  first  order,  and  w=0.     Hence  the  condition  of  adjointness  is  that  ^(y,  x)  vanishes 


It  is  easy  to  see  that  i  is  not  a  negative  integer.     Cf.  Forsyth,  Tlieory  of  Functions,  p.  169. 


88]  GENERAL  FORM  OF  PLUCKER'.S  EQUATIONS.  123 

to  the  first  order  at  each  of  these  places.     The  general  adjoint  polynomial  will  therefore 
not  contain  any  term  independent  of  x  and  y. 

Ex.  ii.     For  the  surface 

y*  _  f  [(  1  +  #5)  &  +  !]  +  tfyA  =  0 

there  are  two  places  at  #=0,  at  each  of  which  y  is  zero  of  the  second  order  :  they  are  not 
branch  places.     At  each  of  these  /'(y)  vanishes  to  the  second  order. 

The  dimension  of  y  is  1,  and  the  general  polynomial  of  grade  (n  -  1)  <r  +  n  -  3  +  1  or  2,  is* 

Af  +  By  +  C+  x  [Dy  +  Ex  +  F]. 

In  order  that  this  may  vanish  to  the  second  order  at  the  places  in  question,  it  is  sufficient 
that  (7=0  and  F=0.     Then  the  polynomial  takes  the  form 

By  +  Ay2  +  Dxy  +  Ex\ 
and  if  we  put  x/rj  for  x  and  !/»/  for  y  this  becomes,  save  for  a  factor  17  ~2, 


which  is  therefore  an  adjoint  polynomial  for  the  surface 


Compare  §  83. 

Ex.  iii.     Prove  that  the  general  adjoint  polynomial  for  the  surface 

y2  =  (#-  a)3, 

is  y(x,  l)r_2  +  (^-a)  (x,  l)r_1  =  0. 

(The  index  of  the  place  at  x=  a  is  1.) 

88.  Since  the  number  of  generalized  zeros  of  f'(y}  is  n(n—  l)(o-  +  1), 
(§  86,  Ex.  ii),  we  have,  in  the  notation  here  adopted, 

2(i+w)  =  n(n-I)(<r  +  l), 

or  if  /  denote  2t  and  W  denote  2w,  the  summation  extending  to  all  finite 
and  infinite  places  of  the  surface 

/+  W  =  n(n-l)(<r+l). 

Hence,  as^ 

W  =  2rc  +  2j»  -  2, 
we  can  infer 

p  =  Kn-l)(n-2  +  "<r)-J/, 
shewing  that  /  is  an  even  integer. 

Further  if  X  denote  the  number  of  zeros  of  an  adjoint  polynomial 
•fy  (y,  x),  of  grade  (n  —  1)  <r  +  n  —  3  +  r,  exclusive  of  those  occurring  at  places 
where  /'  (y)  =  0  or  F'  (rj)  =  0,  and  calculated  on  the  hypothesis  that  the 
adjoint  polynomial  vanishes,  at  a  place  where  f'(y)  or  F'  (77)  vanishes,  to  an 
order  equal  to  twice  the  index  of  the  place  J,  we  have  the  equation 

X  +  /  =  n  (n  -  1)  (a-  +  1)  +  n  (r  -  2). 

*  §  86  preceding. 

t  Forsyth,  Tiieory  of  Function*,  p.  349. 

£  So  that  a  place  of  index  ^i  where  ^  (y,  .r),  or  ^  (77,  £),  vanishes  to  order  i  +  \,  will  furnish  a 
contribution  X  to  the  number  X. 


124  TRANSFORMATION   TO   CASE   OF   SIMPLE   NODES.  [88 

Thus,  as 

/  =  n  (n  -  1)  (a-  +  1)  -  2  (n  -  1)  -  2p, 
we  have 

X  =  nr  +  2p  -  2  ; 

and  this  is  true  when  r  =  0. 

These  important  results  may  be  regarded  as  a  generalization  of  some  of 
Pliicker's  equations*  for  the  case  cr=  0. 

Ex.  i.  The  number  of  terms  in  the  general  polynomial  of  grade  (n-l)  o-  +  n-3  +  r  was 
proved  to  be  \(n  -  1)  (n  -  2  +  w<r)  +  nr  -  1  or  |(w  -  1)  (n  -  2  +  wo-),  according  as  r  >  0  or  r  =  0. 
This  number  may  therefore  be  expressed  as  p  +  \I-\-  nr-l  or  p  +  \I  in  these  two  cases. 

Ex.  ii.  It  is  easy  to  see,  in  the  notation  explained  in  §  85,  that  the  homogeneous  form 
A  (1,  u,  w2,  ...  ,  un~l)  is  of  degree  n  (n  -  1)  (0-+  1)  in  &>  and  z,  and  the  form  A  (1,  g^  ...  ,  ffn,j) 
of  degree  W.  The  quotient  A(l,  u,  ...,  un-l)/&(l,  glt  ...  ,  gn_^  is  (§  43)  an  integral  form 
in  o>,  z,  which,  by  an  equation  proved  here,  is  of  degree  7.  It  is  the  square  of  an  integral 
homogeneous  form  v  whose  degree  in  u>,  z  together  is  |/. 

Ex.  iii.  It  can  be  proved  (compare  §  43  b,  Exx.  1,  2,  and  §  48  ;  also  Harkness  and 
Morley,  Theory  of  Functions,  pp.  269,  270,  272,  or  Kronecker's  original  paper,  Crelle,  t.  91) 
that  if  for  y  we  take  the  function 


wherein  X,  Xt,  ...  ,  Xn_1  are  integral  polynomials  in  x,  of  sufficient  (but  finite)  order,  the 
polynomial  v  occurring  in  the  equation, 

A(l,  y,  ...  ,  y»-1)  =  V2A  (1,  fflt  ...  ,  <?„_!), 

cannot,  for  general  values  of  the  coefficients  in  X,  X:,  ...  ,  Xn_:,  have  any  repeated  factor,  or 
have  any  factor  which  is  also  a  factor  of  A(l,  g^  ...,  ffn_1).  And  the  inference  can  be 
madef  that  for  this  dependent  variable  y,  there  is  no  place  at  which  the  index  is  greater 
than  ^,  and  no  value  of  x  for  which  two  places  occur  at  which  f'(y\  or  F'(T}),  is  zero. 

89.  We  proceed,  now,  to  shew  the  utility  of  the  notion  of  adjoint 
polynomials  for  the  solution  of  the  problem  of  finding  the  expression  of 
a  rational  function  of  given  poles. 

Let  R  be  any  rational  function,  and  suppose,  first,  that  none  of  the  finite 
poles  of  R  are  at  places  where  f'(y)  =  0.  Let  ^r  be  any  integral  polynomial, 
chosen  so  as  to  be  zero  at  every  finite  pole  of  R,  to  an  order  at  least  as  high 
as  the  order  of  the  pole  of  R,  and  to  be  adjoint  at  every  finite  place  where 
/'  (y)  vanishes.  Denote  the  integral  polynomial  II  (x  —  a),  which  contains  a 
linear  factor  corresponding  to  every  finite  value  of  x  for  which  /'  (y)  vanishes, 
by  fj,.  Then  the  rational  function 


*  Salmon,  Higher  Plane  Curves  (Dublin,  1879),  p.  65. 

t  See  also  Noether,  Math.  Annal.  t.  xxiii.  p.  311  (Rationale  Ausfiihrung,  u.  s.  w.),  and  Halphen, 
Comptes  Rendus,  t.  80  (1875),  where  a  proof  is  given  that  every  algebraic  plane  curve  may  be 
regarded  as  the  projection  of  a  space  curve  having  only  one  multiple  point  at  which  all  the 
taugents  are  distinct.  But  see  Valentiner,  Acta  Math.,  ii.  p.  137. 


89]  EXPRESSION   OF   RATIONAL   FUNCTION   OF   GIVEN   POLES.  125 

is  finite  at  all  finite  places  where  R  is  infinite,  and  is  finite,  being  zero, 
at  every  finite  place  at  which  /'  (y)  =  Q.  If  2/1,  ...  ,  yn  denote  the  n  values 
of  y  which  belong  to  any  value  of  x,  and  c  be  an  arbitrary  constant,  the 
function 

»  (c-y,)(c-y,)...(c-yn)  ^  ^  ^ 

i  =  \  c  ~  yi 

is  a  symmetrical  function  of  ylt  ...,  yn  and,  therefore,  expressible  as  a  rational 
function  in  x  only;  moreover  the  function  is  finite  for  all  finite  values  of 
x  and,  therefore,  expressible  as  an  integral  polynomial  in  x.  Since  this 
polynomial  vanishes  for  every  finite  value  of  x  which  reduces  the  product 
p  to  zero,  it  must  divide  by  JJL.  Finally,  the  function  is  an  integral  polynomial 
in  c,  of  degree  n  —  l.  Hence  we  have  an  equation  of  the  form 


wherein  A0,  Alt  ...,  -4n-i  are  integral  polynomials  in  x. 

Therefore,  putting  c  =  ?/;,  recalling  the  form  of  the  function  A  (y,  x),  and 
replacing  y{  by  y,  we  have  the  result 


which  we  may  write  in  the  form 

R  = 
^  being  an  integral  polynomial  in  x  and  y. 

Since 

(x  —  a)  ^  _  p  (x  —  a)  ty 

~7rW      ~7W 

^s,  like  ty,  is  adjoint  at  every  finite  place  where  y"  (y)  vanishes. 

Suppose,  next,  that  the  function  R  has  finite  poles  at  places  where  f  (y) 
vanishes.  Then  the  polynomial  ty  is  to  be  chosen  so  that  R  (x  —  a)  ty/f  (y) 
is  zero  at  such  a  place,  a  being  the  value  of  x  at  the  place.  This  may  be 
stated  by  saying  that  -^  is  adjoint  at  such  a  place  and,  besides,  satisfies 
the  condition  of  being  zero  at  the  place  to  as  high  order  as  R  is  infinite. 

Corollary.  Suppose  R  to  be  an  integral  function  ;  and  for  a  finite  place, 
x  =  a,  y=b,  where  /'  (y)  vanishes,  suppose  t  +  1  to  be  the  least  positive 
integer  such  that  (x  -  a)t+l/f'  (y)  has  limit  zero  at  the  place.  Then  the 
polynomial  -^  of  the  preceding  investigation  may  be  replaced  by  the  product 
II  (x  -  a)',  extended  to  all  the  finite  values  of  x  for  which  /'  (y)  is  zero. 
Hence,  any  integral  function  is  expressible  in  the  form 


126  RATIONAL   FUNCTION   OF  GIVEN   POLES.  [89 

where  S-  is  an  integral  polynomial  in  x  and  y,  which  is  adjoint  at  every  finite 
place  where  f  (y)  vanishes. 

If  the  order  of  a  zero  of  f  (y)  be  represented  as  before  by  i  +  w,  it  is 
clear  that  the  corresponding  value  of  t  +  1  is  the  least  positive  integer  for 
which  (t  +  I)(w  +  l)>i  +  w,  or,  for  which  t>(i  —  l)/(w+l).  Hence  the 
denominator  IT  (x  —  a)*  only  contains  factors  corresponding  to  places  at  which 
the  index  |  i  is  greater  than  zero ;  if  the  index  be  zero  at  all  the  finite  places 
at  which  f  (y)  vanishes,  every  integral  function  is  expressible  integrally. 

It  does  not  follow  that  when  the  index  is  zero  at  all  finite  places,  the  functions 
I,  y,  ... ,  yn~\  form  a  fundamental  system  of  integral  functions  for  which  the  condition  of 
dimensions  is  satisfied.  For  the  sum  of  the  dimensions  of  1,  yt  ... ,  yn~l  is  greater  than 
p+n—l  by  the  sum  of  the  indices  at  all  the  places  #  =  oo . 

It  is  clear  that  if  R  be  any  rational  function  whatever,  it  is  possible 
to  find  an  integral  polynomial  in  x  only,  say  X,  such  that  \R  is  an  integral 
function.  To  this  integral  function  we  may  apply  the  present  Corollary. 
The  reader  who  recalls  Chapter  IV.  will  compare  the  results  there  obtained. 

90.  Let  the  polynomial  ty  be  of  grade  (n—l)<r+n—'3+r,  and  the 
polynomial  ^  of  grade  (n  —  1)  a  +  n  —  3  +  s,  so  that 

^  _  fc-  (n-i)  o—  (n-3)  -r  \p-        ^  _  fc-  (n-i)  o—  (n-3)  -s  (S) 

and  JB  =  f-«0/¥, 

®,  "^  being  integral  polynomials  in  77  and  £. 

If  R  have  poles  for  £  =  0,  it  will  generally  be  convenient  to  choose  the 
polynomial  ^  so  that  R^f  is  finite  at  all  places  £  =  0 ;  if  F'  (77)  vanish  for 
any  places  £=  0,  it  is  also  convenient,  as  a  rule,  to  choose  -^  so  that  %ty/F'(r)) 
vanishes  at  every  place  f  =  0  where  F'  (77)  vanishes,  namely,  so  that  i/r 
is  adjoint  at  infinity.  When  both  R  is  infinite  and  F'  (77)  vanishes  at  a 
place  where  f  =  0,  we  may  suppose  ty  so  chosen  that  gRW/F'  (77)  is  zero  at 
the  place.  Let  ty  be  chosen  to  satisfy  these  conditions.  Then,  since 
RW,  =  R-^r .  ^(n~l)<7+n~3+r,  is  finite  at  every  place,  except  f=oo,  and 
(1  —  a£)  W/F'  (77),  =  |:r~1  (x  —  a)  ^rjf '  (y),  vanishes  at  every  place  x  =  a,  y  =  b, 
where  #  is  finite,  at  which  f  (y)  vanishes,  except  £  =  oo  ,  it  follows,  as  here, 
that  R  can  be  written  in  a  form 

R=®,/V> 

wherein  ©x  is  an  integral  polynomial  in  77  and  £. 

Hence  ®j  =  %r~s®,  and  therefore  r  —  s  is  not  negative  :  namely,  the 
polynomial  ^  which  occurs  in  the  expression  of  a  rational  function  in  the 
form  R  =  ^/"fr,  is  not  of  higher  grade  than  the  denominator  i/r,  provided 
-\Jr  be  chosen  to  be  adjoint  at  infinity,  and,  at  the  same  time,  to  compensate 
the  poles  of  R  which  occur  for  x  =  oo .  Since  a  polynomial  of  low  grade 


91]  ^-POLYNOMIALS.  127 

is  a  particular  case  of  one  of  higher  grade  we  may  regard  ^  and  -fy  as  of  the 
same  grade. 

Hence  we  can  formulate  a  rule  for  the  expression  of  a  rational  function  of 
assigned  poles  as  follows  —  Choose  any  integral  polynomial  i/r  which  is  adjoint 
at  all  finite  places  and  is  adjoint  at  infinity,  which,  moreover,  vanishes  at 
every  finite  place  and  at  every  infinite  place*  where  R  is  infinite,  to  as  high 
order  as  that  of  the  infinity  of  R.  If  a  pole  of  R  fall  at  a  place  where 
f'(y),  or  F'  (77),  vanishes,  these  two  conditions  may  be  replaced  by  a  single  one 
in  accordance  with  the  indications  of  the  text.  Then,  choose  an  integral 
polynomial  S-,  of  the  same  grade  as  i/r,  also  adjoint  at  all  finite  and  infinite 
places,  which,  moreover,  vanishes  at  every  zero  of  the  polynomial  -fy  other  than 
the  poles  of  R,  to  as  high  order  as  the  zero  of  ty  at  that  place.  Then  the 
function  can  be  expressed  in  the  form 


91.  We  may  apply  the  rule  just  given  to  determine  the  form  of  the 
integrals  of  the  first  kind. 

If  v  be  any  integral  of  the  first  kind,  dvjdx  is  a  rational  function  having 
no  poles,  for  finite  values  of  x,  except  at  the  branch  places  of  the  surface.  If 
a  be  the  value  of  x  at  one  of  these  branch  places,  the  product  (x  —  a)  dvjdx 
vanishes  at  the  place.  Hence  we  may  apply  to  dvjdx  the  same  reasoning 
as  was  applied  to  the  function  A  (y,  x)  in  §  89,  and  obtain  the  result,  that 
dv/dx  can  be  expressed  in  the  form 

dv     yn~*AQ  +  yn~2A1  +  ...  +  yA^  +  An_, 
dx  f(y) 

wherein  A0,  ...,  An^  are  integral  polynomials  in  x.     Denote  the  numerator 
by  <f>,  and  let  its  grade  be  denoted  by  (n  -  1)  cr  +  n  —  3  +  r  ;   then 


But,  as  a  function  of  £,  dv/dg  has  exactly  the  same  character  as  has  dv/dx 
as  a  function  of  x.  Thus  by  a  repetition  of  the  argument  F'  (77)  dv[d%  is 
expressible  as  an  integral  function  of  rj  and  £.  Thus  r  is  either  zero  or 
negative. 

(IV 

Wherefore,  /'  (y}  -5-   is   an   integral   polynomial   in    x   and   y,   of  grade 

(n  —  I)<r  +  n  —  3  or  less.  It  is  clearly  adjoint  at  all  finite  places,  and, 
reckoned  as  a  particular  case  of  a  polynomial  of  grade  (n  —  1)  <r  +  n—  3,  it  is 
clearly  also  adjoint  at  infinity. 

Conversely,  it  is  immediately  seen,  that  if  $  be  any  integral  polynomial  of 

*  That  is,  if  the  polynomial  be  i//,  of  grade  («-  1)  <r  +  n-3  +  r  and  ^  =  ^|-(»-i)»1-(n-S)-r)  >j> 
vanishes  at  £  =  0  to  the  order  stated.     A  similar  abbreviated  phraseology  is  constantly  employed. 


128      NUMBER  OF   UN  ASSIGNED   COEFFICIENTS   IN   ADJOINT  POLYNOMIAL.    [91 

grade  (n  —  1)  «r  +  n  —  3,  which  is  adjoint  at  all  finite  and  infinite  places,  the 
integral 

/•/  xy> 

I       *i    ,       *    tt-U/j 

is  an  integral  of  the  first  kind. 

Corollary.  We  have  seen  that  the  general  adjoint  polynomial  of  grade 
(n—  l)o-  +  w  —  3  contains  p  +  ^I  terms,  and  we  know  that  there  are  just 
p  linearly  independent  integrals  of  the  first  kind.  We  can  therefore  make 
the  inference 

The  condition  of  adjointness,  for  a  polynomial  of  grade  (n—  1) <r  +  n  —  3, 
is  equivalent  to  ^1  linearly  independent  conditions  for  the  coefficients  of  the 
polynomial,  and  reduces  the  number  of  terms  in  the  polynomial  to  p. 

92.  We  have  shewn  that  a  general  polynomial  of  grade  (n  —  l)o-+n— 3  +  r 
is  of  the  form 


^n-3+r  =  y»-i  (x,  l)r_2  +  y»-s  (x,  l)r_a  +  ...+y(x,  !),_!  +  (x,  l)r_x 

We  shall  assume  in  the  rest  of  this  chapter  that  the  condition  of  adjoint- 
ness  for  a  general  polynomial  of  grade  (n  —  l)cr  +  n  —  3  +r  is  equivalent 
to  as  many  independent  linear  conditions  as  for  a  general  polynomial  of 
grade  (n  —  1)  a  +  n—  3.  Thence,  the  general  adjoint  polynomial  of  grade 
(n—  l)cr  +  n-3  +  r  contains  nr  —  1  +  p  terms. 

Further  we  shewed  that  the  adjoint  polynomial  of  grade  (n  —  1)  a-  +  n  —  3 
has  %p  —  2  zeros  exclusive  of  those  falling  at  places  where  f  (y)  =  0,  or 
F'(r,)  =  0. 

Hence,  the  2p  —  2  zeros  of  the  differential  dv  (Chap.  II.  §  21)  are  the 
zeros  of  the  polynomial  f  (y)  dv/dx,  exclusive  of  those  where  f  (y)  =  0,  or 
*"(,)  =  <>. 

It  is  in  fact  an  obvious  corollary  from  the  condition  of  adjointness  that 

dV/dt  =  Wf(y)]tj 

dx 
only  vanishes  when  0  vanishes.     For,  at  a  place  where  /'  (y)=0,  (/>  vanishes  i  times,  -j- 

vanishes  w  times,  and/'(y)  vanishes  i+w  times. 

Ex.  i.     For  the  surface  associated  with  the  equation 


where  (x,  1)1?  ...  are  integral  polynomials  in  x  of  the  degrees  indicated  by  their  suffixes, 
<r  =  0;  and  the  general  polynomial  of  grade  (n—l)<r  +  n  —  3  or  1,  is  of  the  form  (§  86) 

Ay+Bt+C. 

The  indices  of  the  places  where  /'(y)  =  0  are  easily  seen  to  be  everywhere  zero  —  there 
are  no  places,  beside  branch  places,  at  which  f'(y)  vanishes.  Hence  p  is  equal  to  the 
number  of  terms  in  this  polynomial,  or  p  =  3.  And  this  polynomial  vanishes  in  2/>-2  =  4 
places.  These  results  may  be  modified  when  the  coefficients  in  the  equation  have  special 
values. 


92]  DEFICIENCY   OF   WEIERSTRASS'.S   CANONICAL   SURFACE.  129 

Ex.  ii.     For  the  more  particular  case  when  the  equation  is 


(*,  1)2=0 

there  are  two  places  at  x=Q  at  which  y=0.  For  general  values  of  the  coefficients  in  the 
equation  these  are  not  branch  places  and  f'(y)  vanishes  to  the  first  order  at  each  ;  the 
index  at  each  place  is  therefore  \i  where  i=l,  and  the  condition  for  adjointness  of  the 
general  polynomial  of  grade  1,  is  that  it  shall  vanish  once  at  each  of  these  places.  These 
conditions  are  equivalent  to  one  condition  only,  that  (7=0.  Hence,  as  there  are  no  other 
places  where  the  index  is  greater  than  zero,  the  general  integral  of  the  first  kind  is 


and  p  =  2;  the  polynomial  Ay  +  Rv  vanishes  in  2p-  2  or  2  places  other  than  the  places 
#=0,  y=Q  at  which  /'(y)=0. 

Ex.  iii.  In  general  when  the  equation  of  the  surface  represents  a  plane  curve  with  a 
double  point,  the  condition  of  adjointness  at  the  places  which  correspond  to  this  double 
point,  is  the  one  condition  that  the  adjoint  polynomial  vanish  at  the  double  point*. 

Ex.  iv.     Prove  that  for  each  of  the  surfaces 

l)2  +  (^  1)4=0, 


there  is  only  one  place  at  infinity  and  the  index  there,  in  both  cases,  is  1. 

Shew  that  the  index  at  the  infinite  place  of  Weierstrass's  canonical  surface  f  is  in  all 
cases 


-r-l), 


where 


means  the  least  integer  greater  than  r/a,  and  that  the  deficiency  is  given  by 


where  /'  denotes  the  sum  of  the  indices  at  all  finite  places  of  the  surface. 

Of.  Camb.  Phil.  Trans,  xv.  iv.  p.  430.  The  practical  method  of  obtaining  adjoint  poly 
nomials  of  grade  (n—  1)  <r+n  —  3  which  is  explained  in  that  paper  (pp.  414  —  416)  is  often  of 
great  use. 

Ex.  v.     In  the  notation  of  Chap.  IV.  the  polynomial 

(X,  I)*'"1  $!+...+(#,  Ifn-l-1  <K-i 

is  an  adjoint  polynomial  of  grade  (n  -  1)  v  +  n  —  3. 

Ex.  vi.  We  can  prove  in  exactly  the  same  way  as  in  the  text  that  an  integral  of  the 
third  kind  infinite  only  at  the  ordinary  finite  places  (xlt  yj,  (#/,  y^\  at  the  former  like 
C\og(x-xl)  and  at  the  latter  like  -  C  log  (x  -  #/),  C  being  a  constant,  can  be  written  in 
the  form 


where  ^  is  an  adjoint  integral  polynomial  in  x  and  y,  of  grade  (n-l)<r  +  n—l,  which 

*  The  sum  of  the  indices  at  the  k  places  of  the  surface  corresponding  to  an  ordinary  fc-ple 
point  of  the  curve  is  p  (k  -  1)  ;  the  index  at  each  of  the  places  is  in  fact  %(k  -  1).     Cf.  §  83,  Ex.  i. 
t  Chap.  V.  §  64. 

B.  9 


UNIVERSITY 


130  INTEGRAL   OF   THIRD   KIND.  [92 

vanishes  at  the  (n  —  1)  places  x=xl  where  ?/  is  not  equal  to  yl  and  at  the  (ji-1)  places 
x=x±  where  y  is  not  equal  to  yx'.     Putting  \^  in  the  form 


+  (x-  x^  (x  -  x^  (RQy»  -  1  +  Rtf  -  2  +  .  .  .  +  Rn  _  J, 

where  C0,  ...,  C'n_1,  C^',  ...,  C'n_l  are  constants,  it  follows,  since  (x-x^}yn~l  is  of  grade 
(n  —  l)<r+n,  arid  (^0yn~1  +  Jff1yn~2  +  ...  +  ^n_1)  (x-x^)  (x-x^  is  of  grade  (n-l)<r  +  n+l 
at  least,  that  /£0  is  zero  and  C0  —  0Q'.  Further,  if  the  equation  associated  with  the  surface 
be  written 

and  Xi  (x)  denote 

it  follows,  from  the  condition  for  ^  which  ensures  that  the  integral  P  is  not  infinite  at 
all  the  n  places  x=xly  that  the  factors  of  the  polynomial 


are  the  same  as  those  of/(y,  x}j(y  —  y^  or  of 


Hence,  save  for  a  constant  multiplier,  P  has  the  form 

/dx 
^[fo^-teJtf-ttf-v'te  IXr-i+y"-3^,  l)*r+...  +  (#,  l)(B_l)<r  +  n-3], 

where  (x,  #x)  denotes 

[yn-1+yn-2XlK)  +  -+Xn-l(^l)]/(^-^l), 

so  that  (x,  #!)  =  (#!,  A'),  and  (x,  #/)  denotes  a  similar  expression. 

A  general  polynomial  ^  of  grade  (n-l)tr  +  n-l  contains  2n-l  more  terms  than  a 
general  polynomial  of  grade  (n-  1)  a-  +  n  —  3.  In  accordance  with  the  assumption  made  in 
§  92  the  general  adjoint  polynomial  ^  of  grade  («  —  1)  <r+n—  1  will  contain  2n—  l+p 
terms.  The  condition  that  >//•  vanishes  in  the  2»-2  places  x=xly  x=x^  other  than  those 
where  y=yl,  y=y\  respectively,  will  reduce  the  number  of  terms  to  p  +  1.  This  is  exactly 
the  proper  number  of  terms  for  a  general  integral  of  the  third  kind  (cf.  §  45,  p.  67).  The 
assumption  of  §  92  is  therefore  verified  in  this  instance. 

The  practical  determination  of  an  integral  of  the  third  kind  here  sketched  is  often  very 
useful.  In  the  hyperelliptic  case  it  gives  the  integral  immediately. 

Ex.  vii.     Prove  that  if  the  matrix  of  substitution  Q  occurring  on  p.  62,  in  *he  equation 
(1,  y,  y\  ...  ,  y»-i)  =  a  (!,&...,  #„-,), 

—  1 

be  denoted  by  Qx,  and  the  general  element  of  the  product-matrix  ^Q^     be  denoted  by 
cr,g,  and  if,  for  distinctness  of  expression,  we  denote  the  elements 

x»-i  (*)•  x*-*  (*),  -  •  xi  (#)»  !>  !>  yi,  yi*>  -  .  ^i"'1! 

respectively  by 

UD  UZ)  ••'  >  Mn-l>  ^n>  *i>  *"2>     3'  •••  »     n' 

then  the  function 

</>0  (a?)  +  0!  (ar)  ^  (»i)-f-  ...  +4i»-i(  (*)F»-1  (*i)i 

which  occurs  in  the  expression  of  an  integral  of  the  third  kind  given  in  §  45,  is  equal  to 
cnulkl  +  ...+ciiuiki  +  ...  +  crturk,+ctrugkr+.... 

This  takes  the  form  <ul&1  +  ...+unlkn  obtained  in  Ex.  vi.  when  crs=0  and  crt=l,  namely 
when  Q  is  a  constant.  This  condition  will  be  satisfied  when  the  index  is  zero  at  all  finite 
and  infinite  places. 


92]  INTEGRAL  OF  THIRD  KIND.  131 

Ex.  viii.     Prove  for  the  surface  associated  with  the  equation 
y*+y*fa  \\+y(x,  l),  +  fa  1)4  =  0, 

that  the  condition  of  adjointness  for  any  polynomial  is  that  it  vanish  to  the  second  order 
at  the  place  £  =  0. 

Thence  shew  that  the  polynomial 

(x  -  #/)  |>2 +yXl  fa)  +  Xz  fa)]  -  (x  -  xj  [y*  +y\i  fa)  +  X2  «)] 

+  ( Ay  +  Bx*  +  Cx+D)(x-xl)(x-  #/) 
is  adjoint  provided  B=Q  ;  and  thence  that  the  integral  of  the  third  kind  is 

+yXl  fa)+Xz  fa)    y*  +yxifa')+x^fa)  .  .   ,  /    ,  7)1 


Ex.  ix.  There  is  a  very  important  generalization*  of  the  method  of  Ex.  vi.  for  forming 
an  integral  of  the  third  kind.  Let  /z  be  any  positive  integer.  Let  a  general  non-adjoint 
polynomial  of  grade  /z  be  chosen  so  as  to  vanish  in  the  two  infinities  of  the  integral,  which 
we  suppose,  first  of  all,  to  be  ordinary  finite  places.  Denote  this  polynomial  by  L.  It 
will  vanish f  in  ?i/z-2  other  places  Blt  J52,  ....  Take  an  adjoint  polynomial  \^,  of  grade 
(n  —  l)o-+n  —  3-{-/z,  chosen  so  as  to  vanish  in  the  places  Blt  B2,  ....  The  polynomial  will 
presumably  contain  (§  92)  n^—  1  +p—  (tip  —  2)  or  p  +  l  homogeneously  entering  arbitrary 
coefficients,  and  will  vanish  (§  88)  in  np  +  Sp  —  2  —  (np  —  2)  or  2p  places  other  than  the 
places  Blt  Z?2,  ...  and  places  where  f'(y),  or  F' (9),  vanishes.  Then  the  integral 


is  a  constant  multiple  of  an  elementary  integral  of  the  third  kind. 

The  proof  is  to  be  carried  out  exactly  on  the  lines  of  the  proof  of  the  form  of  an 
integral  of  the  first  kind  in  §  91,  with  reference  to  the  investigation  in  §  89. 

Further  as  we  know  (§  16)  that  dPfdx  is  of  the  form 

C  (dP\dx\  +  Xx  (dv^dx)  -f  .  .  .  +  Xp  (dvp/dx), 

where  C,  Xu  ...  ,  Xp  are  arbitrary  constants,  (dPjdx\  is  a  special  form  of  dPjdx  with  the 
proper  behaviour  at  the  infinities,  and  vlt  ...  ,  vp  are  integrals  of  the  first  kind,  it  follows 
that  the  polynomial  \^,  which  is  an  adjoint  polynomial  of  grade  (n  —  l)<r-fn  —  3  +  /x,  pre 
scribed  to  vanish  at  all  but  two  of  the  zeros  of  a  non-adjoint  polynomial  L  of  grade  /z,  is  of 
the  form 


where  \^0  is  a  particular  form  of  >//•  satisfying  the  conditions,  and  0  is  any  adjoint  poly 
nomial  of  grade  (n—  1)  <r+n  —  3  ;  for  this  is  the  only  form  of  -^  which  will  reduce  dPjdx  to 
the  form  specified. 

Ex.  x.     Shew  that  if  in  Ex.  ix.  one  or  both  of  the  infinities  of  the  integral  be  places 
where  f'(y)  =  0,  the  condition  for  L  is  that  it  vanish  to  the  first  order  in  each  place. 

Ex.  xi.     For  the  case  of  the  surface  associated  with  the  equation 


*  Given,  for  <r  =  0,  /*  =  !,  in  Clebsch  and  Gordan,  Abel.  Functionen  (Leipzig,  1866),  p.  22,  and 
Noether,  "Abel.  Differentialausdriicke,"  Math.  Annal.  t.  37,  p.  432. 

t  Counting  zeros  which  occur  for  x  =  oo  ,  or  supposing  all  the  zeros  to  be  at  finite  places. 
Zeros  which  occur  at  x  =  oo  are  to  be  obtained  by  considering  £^L,  which  is  an  integral  polynomial 
in  f  and  17  (§  86). 

9—2 


132  ANY   RATIONAL   FUNCTION   BY   INTEGRAL   FUNCTIONS.  [92 

for  which  the  dimension  of  y  is  1,  let  us  form  the  integral  of  the  third  kind  with  its 
infinities  at  the  two  places  #  =  0,  y—Q  by  the  rules  of  Exs.  ix.  and  x.  ;  taking  /x  =  l,  the 
general  polynomial  of  grade  1  which  vanishes  at  the  two  places  in  question  is  \x  +  py. 
The  general  polynomial  of  grade  n  -  3  +  /i,  or  2,  is  of  the  form  ax*  +by2  +  2  to/  +  2gx  +  2/y  +  c. 
In  order  that  this  may  be  adjoint,  c  must  vanish  ;  in  order  that  it  may  vanish  at  the  two 
points,  other  than  (0,  0)  at  which  \x  +  ny  vanishes,  it  must  reduce  to  the  form 


Hence  the  integral  of  the  third  kind  is  I  (Ax  +  By  +  C)  dx/f  (y).     (Of.  §  6  |8,  p.  1  9.) 

Ex.  xii.     Obtain  the  other  result  of  §  6  /3,  p.  19  in  a  similar  way. 

Ex.  xiii.  It  will  be  instructive  to  compare  the  method  of  expressing  rational  functions 
which  is  explained  here,  with  a  method  founded  on  the  use  of  the  integral  functions 
obtained  in  Chap.  IV.  We  consider,  as  example,  the  case  of  a  rational  function  which  has 
simple  poles  at  kl  places  where  x=al,  k.2  places  where  x=a.2,  ...,  Jcr  places  at  x  =  ar,  and  for 
simplicity  we  suppose  all  these  values  of  x  to  be  finite,  and  assume  that  the  sheets  of  the 
surface  are  all  distinct  for  each  of  these  values  of  x.  If  R  be  the  rational  function,  the 
function  (x-a^)...(x  -</,.)  R  is  an  integral  function  of  dimension  r,  and  is  expressible  in 
the  form 


this  form  contains  (r+l)  +  (»--T1)  +  ...  +  (?i-Tn_1)  ornr-p  +  l  coefficients  ;  these  co 
efficients  are  not  arbitrary,  for  the  function  (x-al)...(x  —  ar)  R  must  vanish  at  each  of  the 
n  —  i\  places  x—a-^  where  R  is  not  infinite,  and  must  vanish  at  each  of  the  places  x=a2 
where  R  is  not  infinite,  and  so  on.  The  number  of  linear  conditions  thus  imposed  is 
m-(kl+Li  +  ...+kr)  or  rn-Q,  if  Q  be  the  total  number  of  poles  of  the  function  R. 
Hence  the  number  of  coefficients  left  arbitrary  is  nr—  p  +  l-(nr-  Q)  or  Q-p  +  l  ;  this  is 
in  accordance  with  results  already  obtained. 

Ex.  xiv.  If  the  differential  coefficients  of  r  +  1  linearly  independent  integrals  of  the 
first  kind  vanish  in  the  Q  poles,  in  Ex.  xiii.,  the  conditions  for  the  coefficients  are  equi 
valent  to  only  nr—  Q-  (T+  1)  independent  conditions. 

93.  Let  Al,  ...  ,  AQ  be  Q  arbitrary  places  of  the  Riemann  surface.  We 
shall  suppose  these  places  so  situated  that  a  rational  function  exists  of  which 
they  are  the  poles,  each  being  of  the  first  order*.  This  is  a  condition  which 
is  always  satisfied  f  when  Q  >p.  The  general  rational  function  in  question  is 

of  the  form 

X  +  \iZ1  +  .  .  .  +  \qZq, 

wherein  \,  \  ,  .  .  .  ,  \q  are  arbitrary  constants  and  Zl  ,  .  .  .  ,  Zq  are  definite 
rational  functions  whose  poles,  together,  are  the  places  Al,  ...,  AQ. 

The  number  q  is  connected  with  Q  by  an  equation 

Q-q  =  p-T-i, 

where  T  +  1  is|  the  number  of  linearly  independent  linear  aggregates  of  the 
form 


*  We  speak  as  if  the  poles  were  distinct.     This  is  unimportant. 
+  Cf.  Chap.  III.  %  Chap.  III.  §§  27,  37. 


93J  STRENGTH  OF  A  SET  OF  PLACES.  133 

which  vanish  in  Al}  ...,  AQ.  This  aggregate  is  the  differential  coefficient,  in 
regard  to  the  infinitesimal  at  the  place  x,  of  the  general  integral  of  the 
first  kind.  We  have  seen*  that  this  differential  coefficient  only  vanishes 
at  a  zero  of  the  integral  polynomial  of  grade  (n—  1)  <r  +  n  —  3,  which  occurs 
in  the  expression  of  the  integral  of  the  first  kind.  Hence  T  +  1  is  the 
number  of  linearly  independent  adjoint  polynomials  of  grade  (n  —  1)  <r  +  n  —  3 
which  vanish  in  the  places  A1}  ...  ,  AQ  ;  in  other  words,  r  +  1  is  the  number  of 
coefficients  in  the  general  adjoint  polynomial  of  grade  (n—  l)cr  +  n-3 
which  are  left  arbitrary  after  the  prescription  that  the  polynomial  shall 
vanish  in  Al,  ...  ,  AQ. 

Now  we  have  proved  that  if  any  adjoint  polynomial  ty,  of  grade 
(n  —  l)<r  +  n  —  3  +  r  be  taken  to  vanish  at  the  places  A1}  .  ..,  AQ^,  its  other 
zeros  being  Bl  ,  .  .  .  ,  BR,  where  J  R  =  nr  +  2p  -  2  -  Q,  and  ^  be  a  proper  general 
adjoint  polynomial  of  grade  (n  —  l)cr  +  n  —  3  +  r  vanishing  at  51(...,  BR, 
any  rational  function  having  Alt  ...,  AQ  as  poles,  is  of  the  form  ^r/^f.  Hence 
the  rational  functions  Z1}  ...,  Zq  are  of  the  forms  ^a/^,  ...,  \/^,  and  the 
general  form  of  an  adjoint  polynomial  of  grade  (n  —  I)  <r  +  n  —  3  +  r  vanishing 
at  BH  ...,  BB  must  be 


wherein  X,  X1}  ...,  X5  are  arbitrary  constants,  and  ty,  ^i,...,  %  are  special 
adjoint  polynomials  of  grade  (n—  1)  <r  +  w  —  3  +  r  which  vanish  in  B1}  ...  ,  BR, 
some  of  them  possibly  vanishing  also  in  some  of  Alt  ...,  AQ. 

Since  the  general  adjoint  polynomial  ^  of  grade  (n  —  1)  o-  +  n  —  3  +r 
contains  nr—l+p  arbitrary  coefficients,  and  these,  in  this  case,  by  the 
prescription  of  the  zeros  Blt  ...,  BR  for  S-,  reduce  to  q  +  1,  we  may  say  that 
the  places  Blt  ...,  BK,  as  determinators  of  adjoint  polynomials  of  grade 
(n—  l)a+n—  3+r,  have  the  strength  nr—  l+p—  q—  l,or  JR—  (p  —  1)  +  Q  —  q  —  1, 
or  R  —  (r  +  1).  And,  calling  these  places  B1}  ...,  BR  the  residual  of  the 
places  Al}  ...,  AQ,  because  they  are  the  remaining  zeros  of  the  adjoint 
polynomial  ^  of  grade  (n  —  1)  cr  +  n  —  3  +  r  which  vanishes  in  Alt...,  AQ, 
we  have  the  result  :  — 

When  Q  places  Al  .....  AQ  have  ilie  strength  p  —  (r  +  1)  or  Q  —  q  as 
determinators  of  adjoint  polynomials  of  grade  (n—  1)  <r  +  n  —  3,  their  residual 
of  R  =  nr  +  2p  —  2  -  Q  places,  which  are  the  other  zeros  of  any  adjoint 
polynomial  of  grade  (n  —  l)o-  +  ?t  —  3  +  r  prescribed  to  vanish  in  the  places 
Alt...t  AQ,  have  the  strength  R  —  (r+l)  as  determinators  of  adjoint  poly 
nomials  of  grade  (n  —  1)  <r  +  n  —  3  +  r. 

Particular  cases  are,  (i),  when  no  adjoint  polynomial  of  grade  (n-l)o-  +  n  —  3  vanishes 
in  Alt  ...,  Aa;  then  the  places  B1,...,Bll  have  a  strength  equal  to  their  number; 
(ii),  when  one  adjoint  polynomial  of  grade  (n  —  l)o-  +  n  —  3  vanishes  in  Alt  ...,  Au;  then 

*  §  92.  f  A  condition  requiring  in  general  Q<nr-  l+p.  t  §  88. 


134  SPECIAL  SETS.      EQUIVALENT  SETS.  [93 

there  are  R  —  1  of  the  places  Blt  ...,  BR  such  that  every  adjoint  polynomial  of  grade 
(n  —  ])a-  +  n  —  3  +  r,  vanishing  at  these  places,  vanishes  at  the  remaining  place.  For  an 
example  of  this  case  we  may  cite  the  theorem  :  If  a  cubic  curve  be  drawn  through  three 
collinear  points  A^  A2,  A3  of  a  plane  quartic  curve,  the  remaining  nine  intersections 
BU  ...,  Bg  are  such  that  every  cubic  through  a  proper  set  of  eight  of  them  necessarily 
passes  through  the  ninth.  In  general  any  set  of  eight  of  them  may  be  chosen. 

When  r  +  1  is  greater  than  zero  we  may  take  the  polynomial  ty  itself  to 
be  of  grade  (n  —  1)  a  +  n  —  3.  Since  then  a  general  polynomial  ^  of  grade 
(n  —  1)  o-  +  w  -  3  contains  p  arbitrary  coefficients,  we  can  similarly  prove 
that 

When  r  +  1  adjoint  polynomials  of  grade  (n—  1)  <r  +  ?i  —  3  vanish  in  Q 
places  A1}  ..,,  AQ,  so  that  the  Q  places  have  the  strength  Q  —  q  as  deter  - 
minators  of  adjoint  polynomials  of  grade  (n  —  1)  cr  +  n  —  3,  their  residual 
B1}  ...  ,  BR,  of  R  =  2p  —  2  —  Q  places,  have  the  strength  p  —  q  —  1,  or  R  —  r,  as 
determinators  of  adjoint  polynomials  of  grade  (n  —  1)  cr  +  n  —  3.  In  this  case 
the  numbers  are  connected  by  the  equations 


and  the  characters  of  the  sets  Aly  ...,  AQ>  Blt  ...,  BR  are  perfectly  reciprocal*. 

Ex.  When  the  strength  of  a  set  Alt  ...  ,  AQ,  wherein  Q<p,  as  determinators  of  adjoint 
polynomials  of  grade  (n—  l)<r  +  »-3,  is  equal  to  their  number,  so  that  the  number  of 
linearly  independent  adjoint  polynomials  of  grade  (n—  l)o-  +  n  —  3  which  vanish  in  the 
places  of  the  set  is  given  by  r  +  1  =p  —  Q,  it  follows  that  g  =  0.  Thus  if  Blt  ...  ,  BR  be  the 
residual  zeros  of  an  adjoint  polynomial,  <£,  of  grade  (n-l)ar  +  n  —  3,  which  vanishes  in 
Alt  ...,  A01  so  that  R  +  Q=2p  —  2,  only  one  adjoint  polynomial  of  grade  (»—  l)<r+7&—  3 
vanishes  in  B1}  ...  ,  JBR,  namely  <£. 

94.  It  is  known  that  the  number  of  places  *}*  of  the  Riemann  surface 
at  which  a  rational  function  takes  an  arbitrary  value  c,  is  the  same  as  the 
number  of  places  at  which  the  function  is  infinite.  The  sets  of  places  at 
which  c  has  its  different  values,  may  be  called  equivalent  sets  of  places  for 
the  function  under  consideration.  For  such  sets  we  can  prove  the  result  :  — 
if  a  set  of  places  A^,  ...,  A'Q  be  equivalent  to  a  set  Alt  ...,  AQ,  in  the  sense 
that  a  rational  function  g  takes  the  value  c  at  each  place  of  the  former  set 
and  at  no  other  places,  and  takes  the  value  c  at  each  of  Alf  ...,  AQ  and 
at  no  other  places  of  the  Riemann  surface,  then  the  general  rational  function 
with  simple  poles  at  A^,  ...,A'Q  contains  as  many  linearly  entering  arbitrary 
constants  as  the  general  rational  function  whose  poles  are  at  Alt  ...,  AQ. 

*  For  the  theory  of  such  reciprocal  sets  from  the  point  of  view  of  the  algebraical  theory  of 
curves,  see  the  classical  paper,  Brill  u.  Noether,  "Ueber  die  algebraischen  Functionen  u.s.w.", 
Math.  Annal.  vii.  p.  283  (1873). 

t  In  this  Article,  when  a  rational  function  g  is  said  to  have  the  value  c  at  a  place,  it  is 
intended  that  g  -  c  is  zero  of  the  first  order  at  the  place.  A  place  where  g  -  c  is  zero  of  the  k-th 
order  is  regarded  as  arising  by  the  coalescence  of  k  places  where  g  is  equal  to  c. 


95]  COKESIDUAL   SETS.  135 

For  let  the  general  rational  function  with  poles  at  A1}  ...,  AQ  be  denoted 

by  G,  and  be  given  by 

0  =  v0  +  vlGl+  ......  +vqGq, 

where  v0,  ...,  vq  are  arbitrary  constants,  and  Glt  ...  ,  Gq  are  particular  functions 
whose  poles  are  among  Al}  ...,  AQ  —  of  which  one,  say  Glt  may  be  taken 
to  be  the  function  (g  —  c')/(g  —  c).  Then  if  G'  denote  any  function  what 
ever  having  poles  AI,  ...,  A'Q,  and  not  elsewhere  infinite,  the  function 
G'  (g  —  c')/(g  —  c)  is  one  whose  poles  are  at  Al}  .  .  .  ,  AQ  ;  thus  G'  (g  —  c')/(g  —  c) 
can  be  expressed  in  the  form 


for  proper  values  of  v0,  ...,  vq.     Therefore  G'  can  be  expressed  in  the  form 

n>          q  —  c  „  q  —  c  ~    q  —  c 

' 


Since  this  is  true  of  every  function  whose  poles  are  at  A^  ,  ...,  A'Q,  and  that 
the  functions  G%(g  —  c)j(g  —  c)  are  functions  whose  poles  are  at  AI  ,  .  ..,  A'Q, 
the  result  is  obvious. 

95.  If  the  symbol  GO  be  used  to  denote  the  number  of  values  of  an 
arbitrary  (real  or  complex)  constant,  the  general  adjoint  polynomial  ^,  of 
grade  (n  —  1)  cr  -+  n  —  3  +  r,  of  the  form 


which  vanishes  in  the  places  B1}  .  ..,  BR,  gives  rise  to  oo  q  sets  of  places, 
constituted  by  the  zeros  of  S-  other  than  Blt  ...,BR,  each  set  consisting  of, 
say,  Q  places.  Let  Al}  ...,  AQ  be  one  of  these  sets. 

We  shall  say  that  these  sets  are  a  lot  of  sets  ;  that  each  set  is  a  residual 
of  Blt  ...,  BR,  and  that  they  are  co-residual  with  one  another;  in  particular 
they  are  all  co-residual  with  the  set  Alt  ...,  AQ.  Further  we  shall  say  that 
the  multiplicity  of  the  sets,  or  of  the  lot,  is  q,  and  that  each  set  has  the 
sequence  Q  —  q  ;  in  fact  an  individual  set  is  determined  by  q  independent 
linear  conditions,  namely,  of  the  Q  places  of  a  set,  q  can  be  prescribed  and 
the  remaining  Q  —  q  are  sequent. 

It  is  clear  then  that  any  set,  AI,  ...,  A'Q,  which  is  co-residual  with 
Alt...,  AQ,  is  equivalent  with  Alf...,AQ,  in  the  sense  of  the  last  article; 
for  these  two  sets  are  respectively  the  zeros  and  poles  of  the  same  rational 
function  ;  in  fact  if  i/r  be  the  polynomial  vanishing  in  Bit  ...,  BR>  Alf  ...,  AQ, 
and  ^  the  polynomial  vanishing  in  Blt  ...,  BR,  AI,  ...,  A'Q,  the  rational 
function  ^/i/r  has  J./,  ...,  A'Q  for  zeros  and  Alf  ...,  AQ  for  poles.  Hence 
by  the  preceding  article  it  follows  that  the  number  q  +  1  of  linear,  arbitrary, 
coefficients  in  a  general  rational  function  prescribed  to  have  its  poles  at 
AI,  ...,  AQ)  is  the  same  as  the  number  in  the  general  function  prescribed  to 


136  THEOREM   OF   CORESIDUAL  SETS.  [95 

have  its  poles  at  the  co-residual  set  J./,  ...,  A'Q.  In  other  words,  co-residual 
sets  of  places  have  the  same  multiplicity,  this  being  determined  by  the 
number  of  constants  in  the  general  rational  function  having  one  of  these 
sets  as  poles  ;  they  have  therefore  also  the  same  strength  Q  —  q,  or  p  —  (T  +  1), 
as  determinators  of  adjoint  polynomials  of  grade  (n  —  I)<r  +  n  —  3. 

96.  In  the  determination  of  the  sets  co-residual  to  a  given  one,  Alt  ..., 
AQ,  we  have  made  use  of  a  particular  residual,  B1}  ...,  Blt.  It  can  however 
be  shewn  that  this  is  unnecessary  —  and  that,  if  two  sets  be  co-residual  for  any 
one  common  residual,  they  are  co-residual  for  any  residual  of  one  of  them.  In 
other  words,  let  an  adjoint  polynomial  ^r,  of  grade  (n  —  l)a+n—  3  +  r,  be 
taken  to  vanish  in  a  set  A1}  ...,  AQ,  its  other  zeros  (besides  those  where 
y'(^)  =  0(  or  F'  (77)  =  0),  being  Bl}  ...,BR,  and  an  adjoint  polynomial  ^,  of 
grade  (n  —  1)  <r  +  n  —  3  +  r,  be  taken  to  vanish  in  Blt  ...,  BR,  its  other  zeros 
being  the  set  A^,  ...,  A'Q,  co-residual  with  A1}  ...,  AQ;  then  if  an  adjoint 
polynomial,  i/r',  of  grade  (n  —  l)o-  +  n  —  3  +  r',  which  vanishes  in  A1}  ...,  AQ, 
have  BI,  ...,  B'R>  for  its  residual  zeros,  R  being  equal  to  nr'  +  2p  —  2  —  Q,  it 
is  possible  to  find  an  adjoint  polynomial  ^',  of  grade  (n  —  l)cr  +  n  —  3  +  r, 
whose  zeros  are  the  places  B^,  ...,  B'R,,  A^,  ...,  A'Q. 

For  we  have  shewn  that  any  rational  function  having  Alf  ...,  AQ  as  its 
poles  can  be  written  as  the  quotient  of  two  adjoint  polynomials,  of  which  the 
denominator  is  arbitrary  save  that  it  must  vanish  in  the  poles  of  the  function, 
and  be  of  sufficiently  high  grade  to  allow  this.  In  particular  therefore  the 
function  ^f/^r,  whose  zeros  are  AI,  ...,  A'Q,  can  be  written  as  the  quotient  of 
two  polynomials  of  which  ijr'  is  the  denominator,  namely  in  the  form  *$*'  Itf  . 
The  polynomial  ^'  will  therefore  vanish  in  the  places  J3/>  ...,  B'K,  A^,  ...,A'Q, 
as  stated. 

Hence,  not  only  are  equivalent  sets  necessarily  co-residual,  but  co-residual 
sets  are  necessarily  equivalent,  independently  of  their  residual*. 


97.     The  equivalence  of  the  representations  ^/\^,  ^'ty\  nere  obtained,  of  the  same 
function,  has  place  algebraically  in  virtue  of  an  identity  of  the  form 


where  /=0  is  the  equation  associated  with  the  Riemann  surface  and  K  is  an  integral  poly 
nomial  in  x  and  y.  Reverting  to  the  phraseology  of  the  theory  of  plane  curves,  it  can  in 
fact  be  shewn  that  if  three  curves  /=  0,  ^  =  0,  H=  0  be  so  related  that,  at  every  common 
point  of  /  and  •<//-,  which  is  a  multiple  point  of  order  k  for  /  and  of  order  I  for  ^  ,  whereat 
/and  ^  intersect  in  H  +  /3  points,  the  curve  ^Thave  a  multiple  point  of  order  k  +  l-l+ft, 
so  that  in  particular  If  passes  through  every  simple  intersection  of  /  and  ^r,  then  there 
exist  curves  ^'  =  0,  K=0,  such  that,  identically, 


Now  in  the  case  under  consideration  in  the  text,  if  the  only  multiple  points  of  /  be 
multiple  points  at  which  all  the  tangents  are  distinct,  the  adjointness  of  ^  ensures  that  ^ 

*  For  the  theory  of  co-residual  sets  for  a  plane  cubic  curve  see  Salmon,  Higher  Plane  Curves 
(Dublin,  1879),  p.  137.    That  theory  is  ascribed  to  Sylvester;  cf.  Math.  AnnaL,  t.  vii.,  p.  272  note. 


98]  FUNCTIONS    EXPRESSIBLE   BY    ^-POLYNOMIALS.  137 

has  a  multiple  point  of  order  is— I  at  every  multiple  point  of/  of  order  k.  The  adjointness 
of  the  polynomials  ^,  ^'  ensures  that  the  compound  curve  ^'  has  a  multiple  point  of 
order  2  (k-  1)  or  Ic  +  k  - 1  - 1  at  every  multiple  point  of  /  of  order  L  Further,  the  curve 
^^'  passes  through  the  simple  intersections  of  /  and  \^,  which  consist  of  the  sets 
AI,...,AQ,  Si,  ...,BR;  for  ^  passes  through  Bl,...,BR,  and  ^'  is  drawn  through 
AI,  ... ,  AQ.  Hence  the  conditions  are  fully  satisfied  in  this  case  by  taking  11=^^' ;  thus 
there  is  an  equation  of  the  form 


from  which  it  follows  that  the  curve  ^'  is  adjoint  at  the  multiple  points  of  /  and  passes 
through  the  remaining  intersections  of  /  and  ^^',  namely  through  A\,  ...,A'B  and 
B\ ,  ... ,  B'tt. .  This  is  the  result  of  the  text. 

In  case  of  greater  complication  in  the  multiple  points  of/  there  is  need  for  more  care 
in  the  application  of  the  theorem  here  quoted  from  the  algebraic  theory  of  plane  curves. 
But  this  theorem  is  of  great  importance.  For  further  information  in  regard  to  it  the 
reader  may  consult  Cayley,  Collected  Works,  Vol.  i.  p.  26 ;  Noether,  Math.  Annal.  vi. 
p.  351  ;  Noether,  Math.  Annal.  xxiii.  p.  311 ;  Noether,  Math.  Annal.  xl.  p.  140  ;  Brill  and 
Noether,  Math.  Annal.  vii.  p.  269.  Also  papers  by  Noether,  Voss,  Bertini,  Brill,  Baker  in 
the  Math.  Annal.  xvii,  xxvii,  xxxiv,  xxxix,  xlii  respectively.  See  also  Grassmann,  Die 
Ausdehnungslehre  von  1844  (Leipzig,  1878),  p.  225.  Chasles,  Compt.  Rendus,  xli.  (1853). 
de  Jonquieres,  Me'm.  par  divers  savants,  xvi.  (1858). 

98.  From  the  theorem,  that  a  lot  of  co-residual  sets,  of  Q  places,  may  be 
regarded  as  the  residual  of  any  residual  of  one  set,  SQ,  of  the  lot,  it  follows, 
that  every  lot  wherein  the  sequence  of  a  set  is  less  than  p,  may  be  determined 
as  the  residual  zeros  of  a  lot  of  adjoint  polynomials  of  grade  (n  —  1)  <r  +  n  —  3, 
which  have  R  =  2p  —  2  —  Q  common  zeros.  For  the  sequence  Q  —  q  is  equal 
to  p  —  (T  +  1),  and  when  r+l>0  an  adjoint  polynomial  (involving  r-f-1 
arbitrary  coefficients)  can  be  determined  which  is  zero  in  any  one  set,  SQ,  of 
the  lot,  and  in  R  other  places. 

Hence  also,  when  Q  places  are  such  that  the  most  general  rational 
function,  of  which  they  are  the  poles,  contains  more  than  Q  —  p  +  1  arbitrary 
constants,  this  general  rational  function  can  be  expressed  as  the  quotient  of 
two  adjoint  polynomials  of  grade  (n—  l)<r  +  n  —  3;  the  same  is  true  when 
the  Q  places  are  known  to  be  zeros  of  an  adjoint  polynomial  of  grade 
(?i- l)o-  + /i-3. 

It  follows  from  what  was  shewn  in  Chap.  III.  §§  23,  27,  that  if  p  places  be 
the  poles  of  a  rational  function,  an  adjoint  polynomial  of  grade  (n—  l)o-  +  w—  3 
vanishes  in  these  places ;  and  an  adjoint  polynomial  of  that  grade  can  always 
be  chosen  to  vanish  in  p  —  1,  or  a  less  number,  of  arbitrary  places.  Hence, 
every  rational  function  of  order  less  than  p  4- 1,  is  expressible  as  the  quotient 
of  two  adjoint  polynomials  of  grade  (n  —  1)  <r  +  n  —  3. 

Ex.  i.  A  rational  function  of  order  2p  —  2  which  contains  p,  or  more,  arbitrary  constants 
(one  being  additive)  is  expressible  as  the  quotient  of  two  adjoint  polynomials  of  grade 

Ex.  ii.  For  a  general  quartic  curve,  co-residual  sets  of  4  places  with  multiplicity  1  are 
determined  by  variable  conies  having  4  given  zeros  ;  but  co-residual  sets  of  4  places  with 


138  POSSIBLE   DEPENDENCE  [98 

multiplicity  2  are  determined  as  the  zeros    of  variable  polynomials  of  degree  1,  i.e.  by 
straight  lines. 

Ex.  iii.  The  equation  of  a  plane  quintic  curve  with  two  double  points,  can  be  written 
in  the  form  ^S'  -^'S—0,  where  ^,  ^-'  are  cubics  passing  through  the  double  points  and 
seven  other  common  points,  and  S,  S'  are  conies  passing  through  the  double  points  and 
two  other  common  points. 

Ex.  iv.  When  r  +  l  adjoint  polynomials  of  grade  (n—  l)a-  +  n  —  3  vanish  in  a  set,  £fl,  of 
Q  places,  there  must  be  p  —  T—  1  independent  places  Alt  ... ,  Ap_r,1,  in  Ss,  such  that 
every  adjoint  polynomial  of  grade  (n—  \)<r  +  n  —  3  which  vanishes  in  them  vanishes  of 
itself  in  the  remaining  q  places  AP_T,  ... ,  AQ.  Let  SR  be  a  residual  of  SB,  R  being  equal 
to  2p  —  2-Q.  Then,  regarding  SR  and  AP_T,  ...,  Ae,  together,  as  forming  a  residual  of 
Alf  ...,  Ap_r_1,  it  follows  (§  93)  that  there  is  only  one  adjoint  polynomial  of  grade 
(n  —  I)<r+n  —  3  which  vanishes  in  SK  and  in  AP_T,  ... ,  AQ.  Hence  there  exists  no  rational 
function  having  poles  only  at  the  places  Aly  ...,  AP_T_V  For  such  a  function  could  be 
expressed  as  the  quotient  of  two  adjoint  polynomials  of  grade  (n  —  l)<r  +  n  —  3  having 
SR  and  Ap_r,  ... ,  Aa  as  common  zeros.  Compare  §  26,  Chap.  III. 

It  can  also  be  shewn,  in  agreement  with  the  theory  given  in  Chapter  III.,  that  if 
.Z?,,  ... ,  JBr'+i  be  any  r'  +  l  independent  places,  T  being  less  than  T,  there  exists  no  rational 
function  having  poles  in  £fi  and  Blt  ... ,  BT-+I.  In  fact  r-f  1  -  (T'  +  1)  linearly  independent 
adjoint  polynomials  of  grade  (n—  l)<r  +  n  —  3  vanish  in  Ss  and  Bly  ...,  Br'+\.  Let  SR,, 
where  R'  =  2p  —  2  -  (Q + r'  + 1),  be  the  residual  zeros  of  one  of  these  polynomials.  Then  the 
strength  of  SRI,  as  determinators  of  adjoint  polynomials  of  grade  (n  —  l}a-  +  n  —  3  is  (§  93) 
R'  —  (T  —  r')  +  l  =  R  —  T,  where  R  =  2p  —  2  —  Q,  namely  the  strength  of  SR,  is  the  same  as  the 
strength  of  SR,  and  Bv,...,Br'+i  together;  hence  every  adjoint  polynomial  of  grade 
(n—  l)o-+n  —  3  which  vanishes  in  SR,,  vanishes  also  in  Blt  ... ,  Br'+i.  Now  every  rational 
function  having  £2  and  Blt  ... ,  Br'+i  as  poles,  could  be  expressed  as  the  quotient  of  two 
adjoint  polynomials  of  grade  (n-  l)<r+n  —  3  having  SR,  as  common  zeros;  since  each  of 
these  polynomials  will  also  have  Blt  ... ,  -5r'+i  as  zeros,  the  result  is  clear. 

99.  The  remaining  Articles  of  this  Chapter  are  devoted  to  developments 
more  intimately  connected  with  the  algebraical  theory  of  curves. 

We  have  seen  that  an  individual  set  of  a  lot  of  co-residual  sets  of  Q 
places  is  determined  by  the  prescription  of  a  certain  number,  q,  of  the  places ; 
this  number  q  being  less  than*  Q  and  not  )iprSAt6r  than  Q—  p. 

But  it  does  not  follow  that  any  q  places  of  a  set  are  effective  for  this 
purpose ;  it  may  happen  that  q  places,  chosen  at  random,  are  ineffective  to 
give  q  independent  conditions. 

We  give  an  example  of  this  which  leads  (§  100)  to  a  result  of  some  interest. 

Suppose  that  a  set  of  Q  places,  8Q,  is  given,  in  which  no  adjoint  polyno 
mial  of  grade  (n—  l)a-  +  n—  3  vanishes ;  then  r  + 1  is  zero,  and  co-residual 
sets  are  determined  by  Q—  p  places.  Suppose  that  among  the  Q  places  there 
are  p  +  s  —  1  places,  forming  a  set  which  we  shall  denote  by  <rp+s-i ,  which 
are  common  zeros  of  T'  -f  1  adjoint  polynomials  of  grade  (n  —  l)cr  +  n  —  3; 
denote  the  other  Q—  p  —  s  +  1  or  q  —  s  +-I  places  by  <r9_g+1. 

*  The  formula  is  Q  -q=p-  (r  +  1);  if  q  were  Q  and  therefore  r  +  l=p,  all  adjoint  poly 
nomials  of  grade  (n-  1)  <r  +  n-3  would  vanish  in  the  same  Q  places,  contrary  to  what  is  proved 
in  §  21,  Chap.  II. 


100]  OF   PLACES   OF   A   SET.  139 

Take  an  adjoint  polynomial  of  grade  (?i  —  1)  <r  +  n  —  3  +  r  which  vanishes 
in  the  places  of  the  set  SQ,  and  let  SR  denote  its  remaining  zeros,  so  that 
R  +  Q  =  nr  +  2p  —  2.  If  we  now  regard  the  sets  SB,  <rq-t+i  together  as  the 
residual  of  the  set  <Tp+t-i,  it  follows  (§  93)  that  SK,  o-q-g+l  together  have  only 
the  strength  R  +  q  —  s  +  1  —  (T  +  1),  or  nr  +p  —  2  —  (T  +  s),  as  determinators 
of  polynomials  of  grade  (n  —  l)cr  +  7i-3  +  r;  and  if  we  choose  5  —  1  places 
Alt  ...,  Ag_!  from  o-p+g-i,  the  polynomial  of  grade  (n  —  1)  &  +  n  —  3  +  r  with 
zeros  in  SR,  which  vanishes  in  the  q  places  constituted  by  a-q_s+1  and 
A!,  ...,  Ag..!  together,  will  not  be  entirely  determined,  but  will  contain* 
T'  +  2  arbitrary  coefficients,  at  least-}-  :  thus  r'  +  1  further  zeros  must  be 
prescribed  to  make  the  polynomial  determinate. 

A  particular  case  of  this  result  is  as  follows  :  —  Consider  a  lot  of  co- 
residual  sets  of  Q,  =  q  +  p,  places,  in  which  no  adjoint  polynomial  of  grade 
(n  —  l)<r  +  n  —  3  vanishes.  If  p  of  the  places  of  a  set  be  zeros  of  r'+l 
adjoint  polynomials  of  grade  (n—  l)<r  +  w  —  3,  then  the  other  q  places  are  not 
sufficient  to  individualise  the  set  ;  r  +  1  additional  places  are  necessary. 

For  instance  a  particular  set  from  the  double  infinity  of  sets  of  5  places,  on  a  plane 
quartic  curve,  determined  by  variable  cubic  curves  having  seven  fixed  zeros,  is  generally 
determined  by  prescribing  2  places  of  the  set.  But  if  there  be  one  of  the  sets  for  which 
3  of  the  five  places  are  collinear,  then  the  other  two  places  do  not  determine  this  set  ; 
we  require  also  to  specify  one  of  the  three  collinear  places.  It  is  easy  to  verify  this  result 
in  an  elementary  way. 

100.  Consider  now  two  sets  8R,  SQi,  which  are  residual  zeros  of  an 
adjoint  polynomial,  i/^,  of  grade  (n—  1)  a  +  n  —  3  +  rl}  so  that 


Let  Xr_Tl  +  l  be  the  number  of  terms  in  the  general  non-adjoint  polynomial 
of  grade  r  —  1\  and  Nr^fi  be  the  total  number  of  zeros  of  such  a  non-adjoint 
polynomial  of  grade  r  —  r^  Take  Xr_ri  independent  places  on  the  Riemann 
surface,  forming  a  set  which  we  shall  denote  by  Tr_ri,  and  determine  a  non- 
adjoint  polynomial,  ^,  of  grade  r  —  rly  to  vanish  in  Tr_ri.  It  will  vanish  in 
Nr_ri  —  Xr_ri  other  places,  Ur-ri.  Suppose  that  no  adjoint  polynomials  of 
grade  (n—  l)a  +  n  —  3  vanish  in  all  the  places  of  SQt  and  Tr_n.  The  product 
of  the  polynomials  fa  and  %  is  an  adjoint  polynomial  of  grade  (n  —  l)a  +  n 
—  3  +  r.  A  general  adjoint  polynomial  of  grade  (n  —  ~L)  <r  +  n  —  3  +  r  which 
vanishes  in  SR  will  vanish  in  all  the  places  forming  SQl,  Tr_ri,  Ur_ri  together, 
provided  we  choose  the  polynomial  to  have  a  sufficient  number  of  these 
places  as  zeros.  Divide  the  set  SQl  into  two  parts,  one,  T,  consisting  of 
Qi  ~P  +  C^r-r,  -  -XV-r,)  places,  the  other  U  consisting  of  p  -  (Nr_ri  -  Xr_ri) 

*  For  nr+p-2  is  the  number  of  independent  zeros  necessary  to  determine  an  adjoint  poly 
nomial  of  grade  (n  -  l)<r  +  n  -  3  +  r. 

t  More  if  the  8  -I  places  Av  ...,  At_l  be  not  independent  of  the  others  already  chosen. 


140  CAYLEY'S  THEOREM.  [100 

places.  The  sets  T  and  Tr_fi  together  consist  of  Qi  —  p  +  Nr_ri,  or  Q  —  p, 
places,  where 

Q  =  Qi  +  Nr-rt .  =  nr  +  2p—2  —  R, 

for  Nr_Ti  =  n  (r  —  r^,  (§  86,  Ex.  iii.);  if  then  the  sets  U  and  Ur-r^  together 
are  not  zeros  of  any  adjoint  polynomial  of  grade  (n—  l)<r  +  n  —  3,  the  general 
adjoint  polynomial,  of  grade  (n  —  1)  cr  +  n  —  3  +  r,  which  vanishes  in  SR,  will 
be  entirely  determined  by  the  condition  of  vanishing  also  in  the  places  of 
T  and  Tr^fl,  and  will  of  itself  vanish  in  the  remaining  places  U  and  Z7r_ri. 
If,  however,  r'+l  adjoint  polynomials  of  grade  (n  —  1)  a  +  n  —  3  —  (r  —  rx) 
vanish  in  the  places  U,  the  products  of  these  with  the  non-adjoint  polynomial 
^  give  -r'+l  adjoint  polynomials  of  grade  (n  —  1)  a  +  n—  3  vanishing  in  U 
and  Z7r_ri.  In  that  case,  assuming  that  no  adjoint  polynomials  of  grade 
(n—  l)a-  +  n  —  3  vanish  in  the  p  places  U,  Ur-rj,  other  than  those  contain 
ing  %  as  a  factor,  the  adjoint  polynomial  of  grade  (n—  l)<r  +  n  —  3  +  r  which 
vanishes  in  SK,  T  and  Tr_ri,  will  require  T' +  1  further  zeros  for  its  complete 
determination  (§  99). 

Since  now  the  set  Tr-Tl  entirely  determines  the  set  Ur-ri>  we  may  drop 
the  consideration  of  it,  and  obtain  the  result — 

The  adjoint  polynomial,  of  grade  (n—  l)cr  +  n  —  3  +  r,  which  vanishes  in 
all  but  p  —  (Nr-ri  —  Xr-ri)  of  the  zeros  of  an  adjoint  polynomial  of  grade 
(n  —  1)  cr  +  n  —  3  +  rlt  will  have  a  multiplicity  T'  + 1  +  Xr_ri ,  where  r'  +  l  is 
the  number  of  adjoint  polynomials  of  grade  (n  —  1) <r  4 -n  —  3  —  (r  —  i\)  which 
vanish  in  these  other  p  —  Nr-ri  +  Xr_ri  zeros.  When  r'  +  l  is  zero  the  adjoint 
polynomial  of  grade  (n  —  1)  cr  +  n  —  3  +  r  vanishes  of  itself  in  the  remaining 
p  —  Nr-ri+Xr_ri  zeros  of  the  adjoint  polynomial  of  grade  (n  —  l)cr  +  n  —  3+rj. 
When  r'  +  l  is  not  zero  it  is  necessary,  for  this,  to  prescribe  T'  + 1  further 
places  of  these  p  —  Nr-r,  +  Xr_ri  zeros  (provided  r'  +  1  <  p  —  Nr-fl  +  Xr_Ti). 

We  have  noticed  (§  8G,  Ex.  iii.)  that 
Nr_ri  =  n(r-  n), 


where  E  (x)  denotes  the  greatest  integer  in  x. 

For  <r  =  0,  therefore,  the  number  p  -  Nr_Tl  +  Xr_Tl  is  immediately  seen  to 
be  equal  to 


where  7  =  n  -  (r  -  r^,  and  £/  is  the  sum  of  the  indices,  of  the  surface,  for 
finite  and  infinite  places  (§  88). 

Thus  the  result,  for  o-  =  0,—  an  adjoint  polynomial  of  degree  n  —  3  +  r 
which  vanishes  in  all  but  £  (7  -  1)  (7  -  2)  -  \I  of  the  zeros  of  an  adjoint 
polynomial  of  degree  n  —  3  +  r^  (r  >  rl5  7  =  n  -  (r  -  r,)  <fc  3)  will  have  a 


101]  CAYLEY'S  THEOREM.  141 

multiplicity  r  +  1  -f  £  (n  —  7)  (n  —  7  +  3),  where  T  +  \  is  the  number  of  adjoint 
polynomials  of  degree  7-8  which  vanish  in  the  £(7  —  1)  (7  —  2)-  |7  wn- 
assigned  zeros ;  if  r  +  1  is  zero  this  polynomial  of  degree  n  —  3  +  r  will  of 
itself  vanish  in  these  unassigned  zeros :  if  r  +  1  >  0  it  is  necessary,  for  this,  to 
prescribe  r'  +  1  or,  if  r  +  1  >  \  (y  —  1)  (7  —  2)  —  £7,  to  prescribe  all  the  un 
assigned  zeros. 

For  example  let  n  =  5  ;  take  as  the  fundamental  curve  a  plane  quintic  with  2  double 
points  (p  =  4) ;  let  the  remaining  point  of  intersection  with  the  quintic,  of  the  straight  line 
drawn  through  these  double  points,  be  denoted  by  A. 

(i)  Take  r=2,  rt  =  l.  Then  y  =  5-l  =  4,  y-3  =  l;  thus,  an  adjoint  quartic  curve 
vanishing  in  all  but  £(y  —  l)(y  — 2)  —  2,  or  1,  of  the  zeros  of  an  adjoint  cubic,  that  is, 
vanishing  in  10  of  these  zeros,  beside  vanishing  at  the  double  points,  will  have  a  multi 
plicity  T'  + 1  +  £4,  or  T  + 1  +  2,  where  r  + 1  is  zero  if  the  non-assigned  zero  be  not  the  point 
A  :  and  this  quartic  will  then,  of  itself,  pass  through  the  unassigned  zero.  In  this  case,  in 
fact,  the  prescription  of  the  10  +  2  zeros  of  the  quartic  on  the  cubic,  is  a  prescription  of 
more  than  4.3-jOj,  where  pl  is  the  deficiency  of  the  cubic.  Hence  the  quartic  will 
contain  the  cubic  wholly,  as  part  of  itself.  (In  general,  the  condition  to  provide  against 
this  can  be  seen  to  be  r  >  3.) 

(ii)  Take  the  same  fundamental  quintic,  with  r  =  4,  ^  =  3.  Then  an  adjoint  sextic 
curve,  •«//•,  passing  through  all  but  £3 .  2  —  2,  or  1,  of  the  zeros  of  an  adjoint  quintic,  ^,  that 
is  through  20  of  them,  will  have  multiplicity  r'  +  l-j-2,  where  r'+l  is  zero  unless  the  other 
zero  of  the  quintic,  ^,  be  the  point  A. 

If  however  the  unassigned  zero  of  the  quintic,  ^-,  be  the  point  A,  the  20  points  are  not 
sufficient ;  the  sextic,  ^,  has  multiplicity  3  and  the  20  points  plus  A  are  necessary  to 
make  ^  go  through  the  remaining  7  points. 

It  should  be  noticed  that  an  adjoint  curve  of  degree  7  —  8  can  always  be 
made  to  pass  through  ^  (7  —  1)(7  —  2)  —  ^1  —  1  places.  The  peculiarity  in 
the  case  considered  is  that  such  curves  pass  through  one  more  place. 

The  theorem  here  proved  was  first  given  by  Cay  ley  in  1843  (Collected  Works,  Vol.  i. 
p.  25)  without  special  reference  to  adjoint  curves.  A  further  restriction  was  added  by 
Bacharach  (Math.  Annal.  t.  26,  p.  275  (1886)). 

101.  In  the  following  articles  of  this  chapter  we  shall  speak  of  an 
adjoint  polynomial  of  grade  (n  —  1)  <r  +  n  —  3  as  a  ^-polynomial.  In  chapter 
III.  (§  23)  we  have  seen  that  the  set  of  places  constituted  by  the  poles 
of  a  rational  function,  is  such  that  one  of  them  '  depends  '  upon  the  others  ; 
thus  (§  27)  there  is  one  place  of  the  set  such  that  every  ^-polynomial  vanish 
ing  in  the  other  places,  vanishes  also  in  this.  Conversely  when  a  set  of 
places  is  such  that  every  (^-polynomial  vanishing  in  all  but  one  of  the  places, 
vanishes  of  necessity  also  in  the  remaining  place,  this  remaining  place 
depends  upon  the  others*.  When  a  set  S  is  such  that  every  ^-polynomial 

*  Or  on  some  of  them.  For  instance,  if  in  a  two-sheeted  hyperelliptic  surface,  associated  with 
the  equation  y*=(x,  l)2P+2>  we  *a^e  three  places  (arlt  yj,  (x.2,  t/2),  (o^,  -y2),  every  <f>- polynomial, 
(ar-a;,)  (x-o;2)  (x,  l)p_3,  of  order  p-  1  in  x,  which  vanishes  in  (a:,,  ?/j),  (a;2,  j/2),  vanishes  also  in 
(x2,  -i/a).  But  this  last  place  does  not,  strictly,  'depend'  on  (xlt  j/j)  and  (ar2,  y2);  it  depends  on 
(x2,  j/2)  only. 


142  TRANSFORMATION   OF    FUNDAMENTAL    EQUATION  [101 

vanishing  in  S,  vanishes  also  in  places  A ,  B,  . . . ,  it  will  be  convenient,  here,  to 
say  that  these  places  are  determined  by  S. 

Take  now  any  p  —  3  places  of  the  surface,  which  we  suppose  chosen 
in  order  in  such  a  way  that  no  one  of  them  is  determined  by  those  preceding. 
Then  the  general  ^-polynomial  vanishing  in  them  will  be  of  the  form 
\<f>  -f  fjfe  +  v^r,  wherein  A,,  /JL,  v  are  arbitrary  constants  and  <j>,  ^,  ty  are 
^-polynomials  vanishing  in  the  p  —  3  places.  We  desire  now  to  find  a 
place  (ajj)  such  that  all  (^-polynomials  vanishing  in  the  p  — 3  given  places 
and  in  xlt  shall  vanish  in  another  place  ac».  For  this  it  is  sufficient  that 
the  ratios  <f>  (X)  :  S-  (#j)  :  t/r  (o^)  be  equal  to  the  ratios  <£  (#2)  :  ^  (#2)  :  ^  (#2)- 
From  the  two  equations  thus  expressed,  with  help  of  the  fundamental 
equation  of  the  surface,  we  can  eliminate  x2,  and  obtain  an  equation  for  xlt  so 
that  the  problem  is  in  general  a  determinate  one  and  has  a  finite  number  of 
solutions  :  as  a  matter  of  fact  (§  102,  p.  144,  §  107)  the  number  of  positions 
for  xl  is  zp(p  —  3)*,  and  each  determines  the  corresponding  position  of  #2. 
Hence  there  exist  on  the  Riemann  surface  oo  p~3  sets  of  p  —  1  places  such 
that  a  single  infinity  of  ^-polynomials  vanish  in  them ;  such  a  set  can  be 
determined  from  p  —  3  quite  arbitrarily  chosen  places,  and,  from  them,  in 
\P  (P  ~  3)  ways.  Putting  Q  =  p  —  1,  T  +  1  =  2,  we  obtain,  by  the  Riemann- 
Roch  Theorem  q  =  1 .  Hence  to  each  set  once  obtained  there  corresponds 
a  single  infinity  of  co-residual  sets. 

102.  The  reasoning  employed  in  the  last  article,  to  prove  that  there 
are  a  finite  number  of  positions  possible  for  #1}and  the  reasoning  subsequently 
to  be  given  to  determine  the  number  of  these  positions,  is  of  a  kind  that 
may  be  fallacious  for  special  forms  of  the  fundamental  equation  associated 
with  the  Riemann  surface.  An  extreme  case  is  when  the  surface  is  hyper- 
elliptic,  in  which  case  all  the  ^-polynomials  vanishing  in  any  given  place 
have  another  common  zero  (Chap.  V.  §  52).  In  what  follows  we  consider  only 
surfaces  which  are  of  perfectly  general  character  for  the  deficiency  assigned. 

In  particular  we  assume,  what  is  in  accordance  with  the  reasoning  of  the 
last  article,  that  not  every  set  of  p  —  2  places  is  such  that  the  two  (or  more) 
linearly  independent  ^-polynomials  vanishing  in  them,  have  another  common 
zero*f*. 

*  This  result  is  given  in  Clebsch  and  Gordan,  Theorie  der  Abel.  Funct.  (Leipzig,  1866)  p.  213. 

t  Noether  (Math.  Annal.  xvii.)  gives  a  proof  that  this  is  true  for  every  surface  which  is  not 
hyperelliptic.  Take  a  set  of  p  -  2  independent  places,  denoted,  say,  by  S,  and,  if  every  p-  2  places 
determine  another  place,  let  A  be  the  place  determined  by  the  set  S.  Take  a  further  quite 
arbitrary  place,  B.  When  the  surface  is  not  hyperelliptic,  B  will  not  determine  another  place. 
Each  of  the  \  (p  -  1)  (p  -  2)  sets,  of  p  -  3  places,  which  can  be  selected  from  the  p  -  1  places  formed 
by  S  and  A,  constitutes,  with  B,  a  set  of  p-2  places,  and,  in  accordance  with  the  hypothesis 
allowed,  each  of  these  sets  determines  another  place.  It  is  assumed  that  the  p-2  places  S,  and 
the  place  B,  can  be  so  chosen  that  the  J  (p  -  1)  (p  -  2)  other  places,  thus  determined,  are  different 
from  each  other  and  from  the  p  places  constituted  by  S,  A  and  B  together.  Since  the  places  S  are 
independent,  the  ^-polynomial  vanishing  in  S  and  B  is  unique;  and,  by  what  we  have  proved, 


102]  BY   (^-POLYNOMIALS.  143 

Then  it  will  be  possible  to  choose  p  —  3  independent  places,  S,  as  in  the 
last  article,  such  that  there  is  a  finite  number  of  solutions  of  the  problem  of 
finding  a  place  (#j)  such  that  the  ^-polynomials  vanishing  in  S  and  (#j),  have 
another  common  zero  ;  let  p  —  3  places,  forming  a  set  denoted  by  S,  be 
so  chosen.  Let  A  be  a  place  not  coinciding  with  any  of  the  positions  possible 
for  a?,,  and  not  determined  by  S.  Let  <f>,  ^  be  two  linearly  independent 
(^-polynomials  vanishing  in  S  and  A.  Then  the  general  ^-polynomial  vanish 
ing  in  S  and  A  is  of  the  form  \(f>  -I-  fjfo,  \  and  /t  being  arbitrary  constants, 
and  the  general  ^-polynomial  vanishing  in  the  places  S  only  can  be  written 
in  a  form  \(j>  +  /j$r  +  vfy,  wherein  v  is  an  arbitrary  constant  and  ty  is  a 
(^-polynomial  so  chosen  as  not  to  vanish  at  the  place  A. 


Consider  now  the  rational  functions*  z=(f)/ty,  s.=^f/ty,  each  of  the 
(p  +  l)th  order.  They  both  vanish  at  the  place  A. 

These  functions  will  be  connected  by  a  rational  algebraic  equation, 
(s,  z)  =  0,  obtained  by  eliminating  (x,  y}  between  the  fundamental  equation 
and  the  equations  zty  =  <f>,  sty  =  ^  ;  associated  with  the  equation  (s,  z)  =  0 
will  be  a  new  Riemann  surface  ;  to  every  place  (#,  y)  of  the  old  surface 
will  belong  a  definite  place  z  =  <f>/ty,  s  =  *&/ty,  of  the  new  surface  ;  to  every 
place  of  the  new  surface  will  belong  one  or  more  places  of  the  original  surface, 
the  number  being  the  same  for  every  place  of  the  new  surface  f;  since  there 
is  only  one  place  of  the  old  surface  at  which  both  z  and  s  are  zero,  namely 
the  place  which  was  denoted  by  A,  it  follows  that  there  is  only  one  place  of 
the  old  surface  corresponding  to  any  place  of  the  new  surface.  Hence  each 
of  x,  y  can  be  expressed  as  rational  functions  of  s,  z,  the  expression  being 
obtained  from  the  equations  zty  =  <f>,  sty  =  ^,  (s,  2)  =  0  j. 


Since  a  linear  function,  Az  +  jiS  +  y,  equal  to  (X$  +  ^  +  1^)/^,  vanishes*  at  the  variable 
zeros  of  the  polynomial  X0  +  /i^  +  i/^,  namely  in  p  +  l  places,  it  follows  that  the  equation 
(s,  0)  =  0  may  be  interpreted  as  the  equation  of  a  plane  curve  of  order  p  +  l  ;  the  number 

it  vanishes  in  p  +  $  (p  -  1)  (p  -  2)  places.  This  number,  however,  is  greater  than  2p  -  2  when  p  >  3. 
Hence  the  hypothesis,  that  every  p-2  places  determine  another  is  invalid.  In  case  p  =  B  the 
surface  is  clearly  hyperelliptic  when  every  p  -  2  places  determine  another.  In  case  p  =  2  or  1  the 
surface  is  always  hyperelliptic.  It  may  be  remarked  that  when  we  are  once  assured  of  the 
existence  of  a  rational  function  of  p  poles,  we  can  infer  the  existence  of  a  set  of  p  -  2  places 
which  do  not  determine  another  (cf.  §  103).  We  have  already  shewn  (Chap.  III.  §  31)  that  in 
general  a  rational  function  of  order  p  does  exist.  The  reader  may  prove  that  for  a  hyperelliptic 
surface  whose  deficiency  is  an  odd  number  there  does  not  exist  any  rational  function  of  order  p. 

*  It  must  be  borne  in  mind  that,  in  dealing  with  a  rational  function  expressed  as  a  ratio  of 
two  adjoint  polynomials,  we  speak  of  its  poles  as  all  given  by  the  zeros  of  the  denominator;  some 
of  these  may  be  at  x  =  x>  (cf.  §  86),  and  in  that  case  their  existence  is  to  be  shewn  by  considering 
(§  84),  instead  of  the  polynomial,  \f/,  of  grade  /*,  the  polynomial  in  •>]  and  £,  given  by  £/*  \f/.  Or  we 
may  use  homogeneous  variables  (§  85).  For  instance,  forp-S,  we  may,  in  the  text,  have  (§  92, 
Ex.  i.)  <f>=x,  $=y,  \l/  =  l.  Then  0:£:^=l:ij:  £=«:«:«;  and  \f/  has  a  zero  at  z  =  oo. 

t  Chap.  I.  §  4. 

J  Or  by  the  direct  process  of  §  5,  Chap.  I. 


144  THE   3p  —  3    IRREMOVEABLE   CONSTANTS.  [102 

of  its  double  points  will,  therefore*,  be  \p  (p-V)-p,  or  \p  (p  -  3),  though  it  is  not  shewn 
here  that  they  occur  as  simple  double  points.  These  double  points  are  the  transforma 
tions  of  the  pairs  of  places,  (x^,  (#2),  on  the  old  surface,  which  were  such  that  every 
^-polynomial,  vanishing  in  the  p  —  3  fixed  places  S,  and  in  xlt  also  vanished  in  A'2. 

Since  a  double  point  of  a  curve  requires  one  condition  among  its  coefficients,  and  the 
number  of  coefficients  that  can  be  introduced  or  destroyed,  in  the  equation  of  a  curve,  by 
general  linear  transformation  of  the  coordinates  is  8,  it  follows  that  a  curve  of  order  m  has 


constants  which  are  not  removeable  by  linear  transformation.  In  the  case  under  con 
sideration  here,  there  are  p  —  3  places,  £,  of  each  of  which  an  infinite  number  of  positions 
is  possible,  independently  of  the  others,  and  the  most  general  linear  transformation  of 
*  and  z  is  equivalent  only  to  adopting  three  new  linear  functions  of  </>,  ^,  \^,  instead  of 
$>  ^,  \^,  in  order  to  express  the  general  ^-polynomial  through  the  places  S.  Hence 
there  are,  in  the  new  surface  (s,  z)  effectively 


that  is,  3/>  —  3  intrinsic  constants  :  this  is  in  agreement  with  a  result  previously  obtained 
(Chap.  I.  §  7). 

103.  The  p  —  3  places  S  may  be  defined  in  a  particular  way,  thus  :  — 
In  general  there  are  (Chap.  III.  §  31)  (p  —  l)p(p  +  1)  places  of  the  original 
surface,  for  each  of  which  a  rational  function  can  be  found,  infinite  only 
at  such  place  and  infinite  to  the  pih  order.  Every  rational  function,  whose 
order  is  less  than  p  +  1,  can  be  expressed  as  the  quotient  of  two  (^-polynomials 
(§  98).  The  (^-polynomial,  (f>,  occurring  in  the  denominator  of  the  function, 
willf  vanish  p  times  at  the  place  where  the  function  has  a  pole  of  order  pi, 
and  will  vanish  in  p  —  2  other  places  forming  a  set  T.  The  general 
^-polynomial  §  through  these  p  —  2  places  T  will  not  have  another  fixed 
zero,  or  it  would  be  impossible  to  form  a  rational  function  of  order  p  with  (f> 
as  denominator.  Let  now  A  denote  any  place  of  the  set  T,  the  remaining 
p  —  3  places  being  denoted  by  S.  Then  we  may  continue  the  process  exactly 
as  in  the  last  Article. 

The  p  variable  zeros  of  the  ^-polynomials,  of  the  form  \<£  +  /j$t,  which 
vanish  in  the  p  —  2  places  T  will,  for  the  transformed  curve,  become  the 
variable  intersections  of  it  with  the  straight  lines,  \z  +  fis  =  0,  which  pass 
through  the  place  s  =  0,  z  =  0.  We  enquire  now  how  many  of  these  straight 
lines  will  touch  the  new  curve.  This  number  may  be  found  either  by  the 
ordinary  methods  of  analytical  geometry  ||  or  as  the  number  of  places  where 

*  By  the  formula  p  =  %(n  -  1)  (no-  +  n  -  2)  -  £  Si,  for  it  is  clear  that  s  is  an  integral  function  of  z 
of  dimension  1,  so  that  o-  =  0.  And  we  have  remarked  that  i  is  1  at  each  of  the  places  cor 
responding  to  a  double  point  of  the  curve,  so  that  5  +  /c=4Si  ;  cf.  Forsyth,  Theory  of  Functions, 
§182. 

t  See  the  note  (  *)  of  §  102. 

J  This  is  the  fact  expressed  by  the  vanishing  of  the  determinant  A  in  §  31,  Chap.  III. 

§  Which  we  assume  to  be  of  the  form  X0  +  (j&,  involving  q  +  1  =  2  arbitrary  coefficients.  If  q 
were  greater  than  unity,  it  would  be  possible  to  construct  a  function  of  lower  than  the  yth 
order.  This  possibility  is  considered  below  (§  105  ff.). 

||  See  for  example  Salmon's  Higher  Plane  Curves. 


' 
UN.; 


103]  THESE   CONSTANTS   DETERMINE   THE   EQUATION.  14)5 


the  differential  of  the  function  ^/(f>,  of  order  p,  vanishes  to  the  second  order, 
namely*  2p  +  2p—2.  Among  these  tangents,  however,  there  is  one  which 
touches  the  transformed  curve  in  p  points,  counting  as  p—  1  tangents. 
There  are,  therefore,  3p  —  1  other  tangents.  Of  the  3^  distinct  tangent 
lines  thus  obtained,  there  are  3p  —  3  distinct  cross  ratios,  formed  from  the 
3p  —  3  distinct  sets  of  four  of  them,  and  these  cross  ratios  are  independent  of 
any  linear  transformation  of  the  coordinates  s  and  z. 

There  are  thus  3p  —  3  quantities  obtainable  for  the  transformed  curve. 
We  prove,  now-f,  that  they  entirely  determine  this  curve,  and  may,  therefore, 
since  the  transformation  is  reversible,  be  regarded  as  the  absolute  constants 
of  the  original  curve.  For  take  any  arbitrary  point  0  ;  draw  through  it 
3  arbitrary  straight  lines  and  draw  3p  —  3  other  straight  lines  which  form 
with  the  3  straight  lines  first  drawn  pencils  of  given  cross  ratios.  Then  the 
coefficients  of  a  curve  of  order  p  +  I,  which  passes  through  0,  has  %p(p  —  3) 
double  points,  and  touches  3p  straight  lines  through  0,  one  of  them  in  p 
consecutive  points,  are  subject  to  1  +  %p(p  -  3)  +  3p  —  l+p  —  1  or  ^p^+^p—  1 
linear  conditions.  The  number  of  these  coefficients  is  ^(p+I)(p  +  4<)  or 
zP*  +  §P  +  2-  Hence  there  are  three  coefficients  left  arbitrary  ;  besides  these 
there  are  five  other  constants  in  the  equation  of  the  curve,  namely,  those 
which  settle  the  position  of  0  and  the  three  arbitrary  straight  lines  through 
0.  The  eight  constants  thus  involved  in  the  curve  can  be  disposed  of  by 
a  linear  transformation. 

The  reader  will  recognise  here  a  verification  of  the  argument  sketched  in 
§  7,  Chap.  I.  ;  the  present  argument  is  in  fact  only  a  particular  case  of  that, 
obtained  by  specialising  the  dependent  variable  of  the  new  surface,  and  the 
order  of  the  independent  variable  g.  The  restriction  that  the  p  poles  of  g 
shall  be  in  one  place  can  be  removed,  with  a  certain  loss  of  definiteness  and 
conviction. 

The  argument  employed  clearly  fails  for  the  hyperelliptic  case,  since 
then  the  p  —  2  fixed  zeros  of  the  polynomials  <£  and  S-  determine  other  places, 
and  the  function  ^/<£  is  not  of  the  pih  order. 


Forp=3  we  have  the  result  :  —  If  an  inflexional  tangent  of  a  plane  quartic  curve  meet 
the  curve  again  in  0,  eight  other  tangents  to  the  curve  can  be  drawn  from  0.  The  cross 
ratios  of  the  six  independent  sets  of  four  tangents,  which  can  be  formed  from  these  nine 
tangents,  determine  the  curve  completely  —  save  for  constants  which  can  l>e  altered  by 
projection. 

More  generally,  from  any  point  0  of  the  quartic,  ten  tangents  to  the  curve  can  be 
drawn.  The  seven  cross  ratios  of  these  tangents  leave,  by  elimination  of  the  coordinates 
of  0,  six  quantities  from  which  the  curve  is  determinate,  save  for  quantities  altered  by 
projection. 

*  Chap.  I.  §  6. 

t  Cayley,  Collected  Works,  vol.  vi.  p.  6.     Brill  n.  Noether,  Math.  Annal.  t.  vn.  p.  303. 

«•  10 


146  SPECIAL  SETS.  [104 

104.  It  is  a  very  slight  step  from  the  process  of  the  last  Article  to  take 
the  independent  variable  to  be  g  =  ^/$,  where  ^,  <f>  are  (^-polynomials,  having 
p  —  2  common  zeros  forming  a  set  such  that  a  single  infinity  of  ^-polynomials 
vanish  in  the  places  of  the  set.     And  it  may  be  convenient  to  take  another 
dependent  variable. 

In  the  process  of  Article  102,  the  fixed  zeros  of  the  polynomials  used 
are  p  —  3  in  number,  and  a  double  infinity  of  ^-polynomials  vanish  in  the 
places  of  the  set. 

These  two  processes  are  capable  of  extension.  If  we  can  find  a  set  SQ, 
of  Q  places,  in  which  just  (T  +  1  =)  3  ^-polynomials  vanish,  and  if  the  places 
SQ  be  such  that  these  three  ^-polynomials  have  no  other  common  zero,  while 
the  problem  of  finding  a  further  place  xl  ,  such  that  the  two  ^-polynomials 
vanishing  in  SQ  and  x^  have  another  common  zero  x2,  is  capable  of  only  a 
finite  number  of  solutions,  then  we  can  extend  the  process  of  Article  102  ; 
we  can  then,  in  fact,  transform  the  surface  into  one  of  2p  —  2  —  Q  sheets. 
The  dependent  variable  in  the  new  equation  will  be  of  dimension  unity, 
and  the  equation  such  as  represents  a  curve  of  order  2p  —  2  —  Q.  If,  there 
fore,  we  can  find  sets  SQ  in  which  Q  >  p  —  3,  the  new  surface  will  have  a 
less  number  of  sheets,  and  therefore,  in  general,  a  simpler  form  of  equation, 
than  the  surface  obtained  in  §  102. 

Similarly,  if  we  can  find  a  set,  SQ,  which  are  the  common  zeros  of 
(r  +  1  =)  2  ^-polynomials,  say  ^  and  <£,  we  can  use  the  function  g  =  ^/(/>,  with 
a  suitable  other  function,  as  independent  and  dependent  variables  respectively, 
to  obtain  a  new  form  of  equation  for  which  there  are  2p  —  2  —  Q  sheets  :  and 
if  we  can  get  Q>p  —  2  the  new  surface  will  be  simpler  than  that  obtained 
in  |  103. 

105.  We  are  thus  led  to  enquire  what  are  the  conditions  that  r  +  l 
linearly  independent  ^-polynomials  should  vanish  in  any  Q  places  aly  ...,  aQ. 

If  the  general  (^-polynomial  be  written  in  the  form  \1(j>1(x)+...+\p(f)p(a;), 
where  X1}  ...,  \p  are  arbitrary  constants,  the  conditions  are  that  the  Q 
equations 

,(ai)=0,  (*'=1.  2'  •••>  Q) 


should  be  equivalent  to  only  p  —  r  —  1  equations,  for  the  determination  of 
the  ratios  \  :  .  .  .  :  \p  ;  we  suppose  Q  >  p—  r  —  1,  and  further  that  the  notation 
is  so  chosen  that  the  independent  equations  are  the  first  p  —  T  —  1  of  them. 
Then  there  exist  Q  —  (p  —  T  —  1)  sets,  each  of  p  equations,  of  the  form 

<f>j  (ap_r_1+a)  =  m^j  (aj)  +  .  .  .  +  mp_T_l  fe  (fl^-j),         (j  =  1,  2,  .  .  .  ,  p) 

for  each  value  of  a-  from  1  to  Q  —  (p  —  r  —  1),  the  values  of  ml,  ...,  7>ip_T_1 
being,  for  any  value  of  <r,  the  same  for  every  value  of  j.  The  set,  of  p,  of 


105]  SPECIAL   SETS.  147 

these  equations,  for  which  a-  has  any  definite  value,  lead  to  T  +  1  equations, 
of  the  form 

=  0, 

4>P~r-l+k 

arising  for  k  =  1,  2,  . . . ,  T  +  1. 

Putting  q  =  Q  —  (p  —  T  —  1),  we  have  therefore  q  (r  +  1)  such  equations* 
connecting  the  Q  places  a1;  ...,  «Q. 

It  is  obvious  from  the  method  of  formation  that  these  q(r  +  1)  equations 
are  in  general  independent ;  in  what  follows  we  consider  only  the  cases  in 
which  they  are  independent  and  determinate.  Then,  taking  Q—  ^(T+I) 
quite  arbitrary  places,  it  is  possible  to  determine  q  (T  +  1)  other  places,  such 
that  there  are  r  +  1  linearly  independent  ^-polynomials  vanishing  in  the 
total  Q  places. 

The  determination  of  the  q(r  +  l)  places,  from  the  arbitrary  Q  —  q(r  +  l)  places,  may  be 
conceived  of  as  the  problem  of  finding  p  —  r-1  —  [Q  —  <?(T  +  I)],  or  qr,  places,  T,  to  add  to 
the  Q  —  q(r  +  \]  arbitrary  places,  S,  such  that  all  ^-polynomials  vanishing  in  the  resulting 
p  —  T—l  places  S,  T,  may  have  Q-(p-r  —  1),  or  q,  other  common  zeros.  The^  — T  — 1 
places  S,  T  are  independent  determinators  of  ^-polynomials. 

For  instance,  when  Q=p-  1,  r  +  l  =  2,  it  follows  that  q  =  l  and  Q  —  q  (T  +l)=p  —  3,  and 
hence,  from  the  theory  here  given,  it  follows  that  we  can  determine  p  —  1  places  in  which 
two  0-polynomials  vanish,  and,  of  these,  p  —  3  places  are  arbitrary.  The  problem  of 
determining  the  other  two  places  may  be  conceived  of  as  the  problem  of  determining 
p-r-l-[Q  —  q  (r  +  1)],  or  one,  other  place,  to  add  to  the  p  —  3  places,  such  that  all  $- 
polynomials  vanishing  in  the  resulting  p  -  2  places,  which  are  independent  determinators 
of  0-polynomials,  may  have  <?  =  !  other  common  zero.  We  have  already  seen  reason  for 
believing  that,  when  the  p  —  3  places  are  given,  the  other  two  places  can  be  determined  in 
>  — 3)  ways. 


To  every  set  of  Q  places  thus  determined,  there  corresponds  a  co-residual 
lot  of  sets  of  Q  places,  the  multiplicity  of  the  lot  being  q ;  and  every 
corresidual  set  will  have  the  same  character  as  the  original  set.  The  number, 
q,  of  places  of  a  co-residual  set  which  are  arbitrary,  cannot,  obviously,  be 
greater  than  the  number,  Q-q(r+l),  of  the  original  set,  which  are 
arbitrary.  Hence,  the  self-consistence  of  the  theory  clearly  requires  that 
Q-q(T  +  I)>q.  From  this,  by  means  of  the  relation  Q-  q  =  p  —  T—  1,  we 
can  deduce  the  two  important  results 

P  >  (q  +  1)  (r  +  1),     Q>q+p  -2-j  • 

These  equations  are  necessary  in  order  that  alt  ...,  a^  should  be  the  poles  of  a  rational 
function. 

10—2 


148  NORMAL   EQUATION.  [105 

Putting  Q  —  q  (r  +  1)  =  q  +  a,  we  obtain 


1[  _. 

From  each  such  set  SQ  we  can  deduce,  as  its  residuals,  sets,  SB,  of 
R,  =  2p—2  —  Q,  places,  in  which  q  +  l  ^-polynomials  vanish,  and  it  is 
immediately  seen  that 


106.  -If  now  we  determine,  in  accordance  with  this  theory,  a  set  SQ  in 
which  r  +  l=3  ^-polynomials  vanish,  it  being  assumed  that  these  three 
(^-polynomials  have  no  other  common  zero,  and  determine  <£,  S-  to  be  two 
(^-polynomials  vanishing  in  SQ  and  in  one  other  place  0,  ty  being  another 
(^-polynomial  vanishing  in  SQ  but  not  in  0,  then  the  equations  z  =  tfr/ty, 
s  =  S-/I/T,  determine,  as  before,  a  reversible  transformation  of  the  surface,  to 
a  new  surface  of  which  the  number  of  sheets  is  R  =  2p  —  2  —  Q,  and  in  which 
s  is  of  dimension  1  in  regard  to  z. 

Since  R  >  r  +  pr/(r  +  1),  the  value  of  R  is  >  2  +  \p.  Thus  writing  p  =  STT, 
or  STT  +  1,  or  3?r  +  2,  according  as  it  is  a  multiple  of  3  or  not,  R  is  p  —  TT  +  2 
in  all  cases. 

From  R=p-7r  +  2  follows  Q=p-4  +  7r;  thus  q=  Q  -  p  +  3  =  TT  -  1, 
and  Q  —  q(T  +  l)=p  +  7r  —  4<-37r+3=p  —  27r  —  l.  This  is  the  number 
of  places  of  the  set  SQ  which  may  be  taken  arbitrarily.  If  this  number 
be  equal  to  q  =  ir  —  \)  it  follows  that,  by  taking  two  different  sets  of 
Q  —  q(r  +  l),  =p  —  2-7T  —  1,  places,  we  get  only  two  co-residual  sets,  and 
for  the  purposes  of  forming  the  functions  (fr/ty,  *&/$*,  one  is  as  good  as  the 
other.  If  however  Q  —  q  (r  +  1)  >  q,  we  do  not  get  co-residual  sets  by  taking 
different  arbitrary  sets  of  Q  —  q  (r  +  1)  places  :  —  and  there  is  a  disposeableness 
which  is  expressed  by  the  number  of  the  arbitrary  places,  Q  —  q  (r  +  1  ), 
which  is  in  excess  of  the  number,  g,  which  determines  the  sets  co-residual  to 
any  given  one. 

Now  Q  —  q(r+l)  —  q=p  —  27T—  1  —  TT  +  1  =  p  -  3?r.  And,  in  a  surface 
of  m  sheets  and  deficiency  p,  the  number  of  constants  independent  of  linear 
transformations  is  3m  +p  —  9  (§  102).  Hence  the  number  of  unassignable 
quantities  in  the  equation  of  the  surface  is 

3  (p  -  TT  +  2)  +p  -  9  -  (p  -  3-Tr)  or  3p  -  3  ; 
and  this  is  in  accordance  with  a  result  previously  obtained  (§  7,  Chap.  I.). 

Ex.  i.  The  values  of  TT  for  p  =  4,  5  are  1,  1  respectively,  and  p  —  Tr  +  2,  in  those  cases, 
=  5,  6  respectively. 

Hence  a  quintic  curve  with  two  double  points  (jo  =  4),  can  be  transformed  into  a 
quintic  ;  this  will  also  have  two  double  points,  in  general,  since  the  deficiency  must  be 
unaltered.  We  determine  a  set  consisting  of  Q,  =1,  quite  arbitrary  place.  Let  the 


107]  ANOTHER   FORM.  149 

general  conic  through  this  place,  and  the  two  double  points,  be  X0  +  [*&  +  vty  =  0.  Then  the 
formulae  of  transformation  are  2  =  <£/^,  s  =  ^/\^.  As  in  the  text,  we  may  suppose  0,  ^ 
to  have  another  common  point,  in  which  ^  does  not  vanish. 

Ex.  ii.  A  quintic  with  one  double  point  (p  =  5)  can  be  transformed  into  a  sextic  With, 
in  general,  jr(6  —  1)  (6  —  2)  —  5  =  5  double  points.  For  this  we  take  p  —  2n—  1  =  2  arbitrary 
points  ;  if  A$  +  /^  +  j/^  be  the  general  conic  through  the  two  points  and  the  double  point, 
the  equations  of  transformation  are  z  =  ({)/\^,  S=^/A//-. 

Ex.  iii.  Shew  that  the  orders  p  —  IT  +  2  of  the  curves  obtainable  by  this  method  to 
represent  curves  of  deficiencies 

^  =  6,  7,  8,  9 

are  respectively  R  =  6,  7,  8,  8. 

107.  But,  as  remarked  (§  104),  we  can  also  make  use  of  sets  of  R  places 
for  which  T  +  1  =  2,  to  obtain  transformations  of  our  original  surface. 

We  can  obtain  such  a  set  by  taking  R  —  T  (q  +  1),  or  R  —  q  —  1,  arbitrary 
places,  and  determining  the  remaining  q  -\-  1  such  that  q  +  1  ^-polynomials 
vanish  in  the  whole  set  of  R  places. 

It  is  proved  by  Brill*  that  the  number  of  sets  of  q+l  thus  obtainable 
from  R  —  q  —  1  arbitrary  places,  is 


where  p  =  ^q  or  ^(q  +  l),  according  as  q  is  even  or  odd,  and  [    J  denotes 


For  instance  with  R=p,  q  =  0,  the  series  reduces  to  one  term,  whose  value  is  p-1, 
which  is  clearly  right  ;  while,  when  R=p  —  1,  <?  =  !,  the  series  reduces  to 


p-2 
or  $p(p-S),  as  in  §  101,  §  102,  p.  144. 

When  p  is  even  and  R  =  \p  +  1,  q  =  ^p  —  1,  this  series  can  be  summed, 
and  is  equal  to 

2 


When  p  is  odd  and  R  =  |  (p  +  1)  +  1,  q  =  \  (p  —  1)  —  1,  the  series  can  be 
summed,  and  is  equal  to 

4^  |p-2/|j(l>-3)  Hi  +  3). 

Now  let  \(f>  +  /jfo  be  the  general  ^-polynomial  vanishing  in  a  set  which  is 
residual  to  one  of  these  sets  of  R  places,  \  and  p,  being  arbitrary  constants  ; 
we  may  transform  the  surface  with  z  =  ^J<f>  as  the  new  independent  variable. 
The  new  surface  obtained  will  have  R  sheets.  The  new  dependent  variable 
may  be  chosen  at  will,  provided  only  the  transformation  be  reversible. 

*  Math.  Annal.  xxxvi,  pp.  354,  358,  369.     See  also  Brill  and  Noether,  Math.  Annal.  vn.  p.  296. 


150  RIEMANN'S  NORMAL  EQUATION.  [107 


The  function  /^-t-X,  =/iS/<£  +  X,  depends  on  2  +  R-q-l  arbitrary  quantities,  namely 
the  constants  X,  /*  and  the  position  of  the  R-q-l  arbitrarily  taken  places.  There  are 
2/<!  +  2j0-2  places  where  dz  is  zero  to  the  second  order,  namely,  2/i!  +  2/?-2  places  where 
the  curve  a^  +  b<p  =  0  touches  the  fundamental  curve  ;  there  remain  then 

2R  +  2p-2-(R-q  +  l),   =  R  -  1  -p  +  q+  1  +  3jo-3,   =  3p-3 

of  the  2/Z  +  2J0-2  values  which  z  has  when  dz  vanishes  to  the  second  order,  which  are 
quite  arbitrary.     Compare  §  7,  Chap.  I. 

The  least  possible  value  of  R  is  given  by  the  formula  R  >  T  +  pr/(r  +  1). 
If  then  p  be  written  equal  to  STT,  or  2?r  +  1,  according  as  p  is  even  or  odd,  we 
may  take*  R  =  p  —  TT  +  1,  that  is  \p  +  1  or  \  (p  +  1)  +  1,  according  as  p 
is  even  or  odd. 

Hence,  when  p  is  even,  we  can  determine  a  single  infinity  of  co-residual 
sets  of  ^p  +  1  places,  these  sets  being  the  zeros  of  ^-polynomials,  X<£  +  fjfe, 
which  have  ^p  —  3  common  zeros.  To  determine  one  of  these  sets  of  \p  +  1 
places,  we  may  take  one  place,  A,  arbitrarily.  The  other  \p  places  can 
then  be  determined  in  2  \p  —  If  ^p  —  1  \%p  +  I  ways.  Let  two  of  these  ways 


be  adopted,  corresponding  to  one  arbitrary  place  A  ;  the  resulting  sets  of 
\p  +  1  places  will  not  be  co-residual  ;  for  the  sets  co-residual  with  a  given 
set  have  a  multiplicity  1,  and  therefore  no  two  of  these  sets  can  have  a 
place  common  without  coinciding  altogether.  Let  the  sets  co-residual  to 
these  two  sets  be  given  by  A</>  +  yu&  =  0,  V</>'  +  //$•'  =  0,(f>  and  </>'  being  chosen 
so  as  to  vanish  in  A  :  we  assume  that  </>,  <£'  have  no  other  common  zero. 

Then  the  equations  z  =  <f>fo,  s  =  $'/*&'  will  determine  a  reversible  trans 
formation,  as  is  immediately  seen  in  a  way  analogous  to  those  already 
adopted.  In  the  new  equation  z  and  s  enter  to  a  degree  \p-\-\,  and,  since 
there  exists*  no  rational  function  of  lower  order  than  \p-\-\,  no  further 
reduction  of  the  degree  to  which  z  and  s  enter,  is  possible. 

The  new  equation  may  be  interpreted  as  the  equation  of  a  curve  of  order  p  +  2  :  it 
will  have  the  form 

(z,  iynsm  +  (z,  l)msm-l  +  ...  +  (z,  l)m=0, 
wherein  m= 


By  putting  z  =  \/z1,  s=\/sl,  it  is  reduced  to  the  equation  of  a  curve  of  order  p.     The 
form  possesses  the  interest  that  it  was  employed  by  Elemann. 

Ex.     Obtain  the  2  sets  of  \p  +  1  places  corresponding  to  a  given  arbitrary  point  for  a 
quintic  curve  with  two  double  points,  and  transform  the  equation. 

108.     If  we  have  a  set  of  R  places^,  for  which  r  +  1  =  4,  the  co-residual 
places   being   given   by  the    variable   zeros  of  ^-polynomials   of  the   form 
+  v<f>3  +  i/r,  we  can,  by  writing 


*  Thus,  for  perfectly  general  surfaces  of  deficiency  p,  no  rational  function  exists  of  order  less 
than  1  +  ip.     Cf.  Forsyth,  Theory  of  Functions,  p.  460.     Biemann,  Gesam.  Werke  (1876),  p.  101. 
t  Wherein  R  -  r  <p,  or  R  <p  +  3. 


109]  CORRESPONDENCE   WITH   CURVES   IN   SPACE.  151 

and  eliminating  x,  y  from  these  three  equations  and  the  fundamental  equation 
associated  with  the  Riemann  surface,  obtain  two  rational  algebraic  equations 
connecting  X,  Y,  Z\  these  equations  determine  a  curve  in  space,  of  order  R', 
for  this  is  the  number  of  variable  zeros  of  the  function  \X  +  fj,Y  +  vZ  +  1. 
To  a  point  X  =•  Xl,  Y=  F1;  Z  =  Z^  of  the  curve  in  space,  will  correspond  the 
places  of  the  surface,  other  than  the  fixed  zeros  of  </>1;  </>2,  <£>3,  ty,  at  which 


and  it  is  generally  possible  to  choose  </>],  $2,  <f>3,  -ty-  so  that  these  equations 
have  only  one  solution. 

The  lowest  order  possible  for  the  space  curve  is  given  by 


If  then  p  =  4-7T,  or    4?r  +  1,  or  4?r  +  2,  or  4?r  +  3,  R    may  be   taken  equal 
to  p  -  TT  +  3. 

For  instance  with  *  p  =  4,  R  =  Q,  taking  a  plane  curve  with  double  points  at  the  places 
#=oo,  y  =  Q  and  x=0,  y=°o  ,  given  by 

x*f  (x,  y\  +  xy  (x,  y\  +  (ar,  y)3  +  (x,  y\  +  (x,  y\  +  A  =  0, 

we  mayf  take  X01  +  /i02  +  //03  +  ^  =  X^y  +  ^  +  j/i?/4-l  ;  the  places  residual  to  the  variable 
set  of  R  places  are,  in  number,  2p  —  2-6,  =0.     Then  the  equations  of  transformation  are 

X=xt/,   Y=x,   Z=y, 

and  these  give  points  (X,  I7*,  Z)  lying  on  the  surfaces, 
X=  YZ, 


of  which  the  first  is  a  quadric  and  the  second  a  cubic. 

A  set  of  R  places  with  multiplicity  r  =  3  may  of  course  also  be  used 
to  obtain  a  transformation  to  another  Riemann  surface.  With  the  same 
notation  we  may  put  z  =  <j>i/^r,  s  =  (j>J^.  It  is  clear  that  the  resulting 
equation,  regarded  as  that  of  a  plane  curve,  is  the  orthogonal  projection,  on 
to  the  plane  Z=  0,  of  the  space  curve  just  obtained. 

A  set  of  R  places  with  multiplicity  r  >  3  may  be  used  similarly  to  obtain 
a  curve  of  order  R  in  space  of  r  dimensions.  Some  considerations  in  this 
connexion  will  be  found  in  the  concluding  articles  of  this  chapter. 

109.  It  has  already  been  explained  that  the  methods  of  transformation 
given  in  §§  101  —  108  of  this  chapter  are  not  intended  to  apply  to  surfaces 
which  are  not  of  general  character  for  their  deficiency,  and  that,  in  particular, 
hyperelliptic  surfaces  are  excluded  from  consideration.  We  may  give  here  a 
practical  method  of  obtaining  the  canonical  form  of  a  hyperelliptic  surface, 

*  Since  p  must  be  5:  (T  +  1)  (q  +  1),  this  is  the  first  case  to  which  the  theory  applies. 

t  It  is  easy  to  shew  that  this  is  the  general  adjoint  polynomial  of  degree  w-3.  We  may  also 
shew  that  the  integrals,  \xydxj  f'(y),  etc.,  are  finite,  or  use  the  method  given  Camb.  Phil.  Trans. 
xv.  iv.  p.  413,  there  being  no  finite  multiple  points. 


152  HYPERELLIPTIC    CASE.  [109 

whose  existence  has  already  been  demonstrated  (Chap.  V.  §  54).  Suppose 
first  that  p>l.  In  the  hyperelliptic  case  every  </>-polynomial  vanishing 
in  any  place  A  will  vanish,  of  itself,  in  another  place  A'.  Any  one  of  these 
^-polynomials  will  have  2p  —  4  other  zeros,  forming  a  set  which  we  shall 
denote  by  S.  Putting  Q  =  2  and  r  +  1  =  p  —  1  in  the  formula  Q  —  q=p  —  r  —  \, 
we  find  q  =  1,  so  that  the  general  ^-polynomial  vanishing  in  the  places  S 
will  be  of  the  form  A,^  —  X,^,  wherein  X1(  X2  are  arbitrary  constants;  in 
fact  these  2/>  —  4  places  S  consist  of  p  —  2  independent  places  and  the  other 
p  —  2  places  determined  by  them,  one  by  each.  Thus  a  function  of  the 
second  order  is  given  by  z  —  fa/fa.  A  general  adjoint  polynomial  of  grade 
(n  —  1 )  cr  +  n  -  2  will  contain  n+p—l  terms  and  vanish,  in  all,  in  n  +  2p  —  2 
places ;  thus  the  general  adjoint  polynomial,  of  this  grade,  which  is  prescribed 
to  vanish  in  a  set  T  of  n  4-  p  —  3  arbitrary  places,  will  be  of  the  form 
f*ifa  + P&*i  pi,  /^  being  arbitrary  constants,  and  will  vanish  in  p+  1  other 
places.  We  may  suppose  ^  so  chosen  that  it  vanishes  in  one  of  the  two 
zeros  of  fa  which  are  not  among  the  set  S,  and  we  shall  assume  that  ty2 
does  not  vanish  in  this  place,  and  that  fa  does  not  vanish  in  the  other 
of  these  two  zeros  of  fa.  Then  the  functions  z  =  fa/fa,  s  =  ^i/^o,  are 
connected  by  a  rational  equation,  (s,  z)  —  0,  with  which  a  new  Riemann 
surface  may  be  associated ;  to  any  place  of  the  old  surface  there  corresponds 
only  one  place  z=  fa/fa,  s  =  i/r1/ijr2,  of  the  new  surface;  to  the  place  z  =  0, 
s  =  0  of  the  new  surface  corresponds  only  one  place  of  the  original  surface, 
and  the  same  is  therefore  true  of  every  place  of  the  new  surface.  Thus 
the  equation  (s,  z)  =  0  is  of  degree  2  in  s  and  degree  p  +  1  in  z.  The  highest 
aggregate  degree  in  s  and  z  together,  in  the  equation  (s,  z)  =  0,  is  the  same 
as  the  number  of  zeros  of  functions  of  the  form  \z  +  JAS  +  v,  for  arbitrary 
values  of  \,  p,  v,  and  therefore  if  the  poles  s  be  different  from  the  poles 
of  z,  namely,  if  the  zeros  of  \Jr2  other  than  T,  be  different  from  the  zeros 
of  fa2  other  than  S,  the  aggregate  degree  of  (s,  z)  in  s  and  z  together  will 
be  p  +  3 ;  thus  the  equation  will  be  included  in  the  form 

s2a  +  s/3  +  7  =  0, 

where  a,  /3,  7  are  integral  polynomials  in  z  of  degree  p  4-1. 
If  we  put  a-  =  so.  +  £/3,  this  takes  the  form 

0-2  =  ia2  _  a% 

which  is  of  the  canonical  form  in  question. 

Ex.  A  plane  quartic  curve  with  a  double  point  (p  =  2)  may  be  regarded  as  generated 
by  the  common  variable  zero  A  of  (i)  straight  lines  through  the  double  point,  vanishing 
also  in  variable  points  A  and  A',  (ii)  conies  through  the  double  point  and  three  fixed 
points,  vanishing  also  in  variable  points  A,  £,  C. 

When  p  is  1  or  0,  the  method  given  here  does  not  apply,  since  then 
adjoint  ^-polynomials  (which  in  general  vanish  in  2p  —  2  variable  places) 


110]  INVARIANT    EXPRESSION   OF    FUNCTIONS   THAT   OCCUR.  153 


have  no  variable  zeros.  In  case  p  =  1  or  p  =  0,  if  /A^  +/i2\/r2  -f  ^3-^3,  with 
Mi.  fa,  fa  arbitrary,  be  the  general  adjoint  polynomial  of  grade  (n  —  1)  a  +  n  —  2 
which  vanishes  in  n+p  —  4  fixed  places,  fa,  ty3  being  chosen  to  have  one 
other  common  zero  beside  these  n+p  —  4  fixed  places,  we  may  use  the 
transformation  z  =  ^/ijr.,,  s  =  fa/  fa,  z  being  a  function  of  order  p  +  I,  and  s 
being  a  function  of  order  p  +  2.  Then,  since  the  function  \z  +  /JLS  +  v  vanishes 
in  p  +  2  places,  we  obtain  an  equation  of  the  form  * 

s2  (z,  l)p  +  s  (z,  1  ),,+1  +  (z,  l)p+2  =  0, 
of  which  the  further  reduction  is  immediate. 

Ex.  For  a  plane  quartic  curve  with  two  double  points  (^9  =  1)  let  nl\jsl  +  p.$z  +  ^3^3  be 
the  general  conic  through  the  double  points  and  a  further  point  A,  \^x  and  \/r3  being  chosen 
also  to  vanish  at  any  point  B.  Then  we  may  use  the  transformation  £  =  Vri/V'3i  S  =  ^r2/Vr3- 

110.  In  the  transformations  which  have  been  given  we  have  made 
frequent  use  of  the  polynomials  which  we  have  called  (^-polynomials,  namely 
adjoint  polynomials  of  grade  (n—  l)cr  +  n  —  3.  For  this  there  is  the  special 
reason,  already  referred  to-f,  that,  in  any  reversible  transformation  of  the 
surface,  their  ratios  are  changed  into  ratios  of  ^-polynomials  belonging  to 
the  transformed  surface  ;  thus  any  property,  or  function,  which  can  be 
expressed  by  these  ^-polynomials  on.ly,  is  invariant  for  all  birational  trans 
formations.  We  give  now  some  important  examples  of  such  properties. 

Let  the  general  ^-polynomial  be  always  supposed  expressed  in  the  form 
\fa  +  ...  +  \p<f>p,  \i,  ...,  Xp  being  arbitrary  constants.  Instead  of  fa,  ...,  <f>p 
we  may  use  any  p  linearly  independent  linear  functions  of  fa,  ...,  tj>p> 
agreed  upon  beforehand.  A  convenient  method  is  to  take  p  independent 
places  GU  ...,  cp  and  define  fa  as  the  ^-polynomial  vanishing  in  all  of  c1?  ...,cp 
except  d  ;  but  we  shall  not  adhere  to  that  convention  in  this  place.  Let  any 
general  integral  homogeneous  polynomial  in  fa,  ...,  fa,  of  degree  fi,  be 
denoted  by  <E>w  or  <&'&*>.  This  polynomial  contains  p(p  +  l)...(p+p-  l)/p  ! 
terms. 

In  a  polynomial  <l><2>  there  are  $p(p  +  l)  products  of  two  of  fa,  ...,fa. 
But  these  &p(p+l)  products  of  pairs  are  not  linearly  independent.  For 
example  in  a  hyperelliptic  case,  we  can  choose  a  function  of  the  second  order, 
z,  such  that  the  ratios  of  p  independent  (^-polynomials  are  given  by 

fa  :  fa  :  ...  :  fa  =  1  :  z  :  z2  :  ... 
then  there  will  be  p  —  2  identities  of  the  form 

=  fa/fa  =  ...    =  fa/fa-!  , 


*  Further  developments  are  given  by  Clebsch,  Crelle,  t.  64,  pp.  43,  210.  For  this  subject  and 
for  many  other  matters  dealt  with  in  this  Chapter,  the  reader  may  also  consult  Clebsch- 
Lindemann-Benoist,  Legons  sur  la  Geometric  (Paris  1883),  t.  in. 

t  Chap.  II.  §  21. 


154  LINEARLY   INDEPENDENT  [110 

whereby  the  number  of  linearly  independent  products  of  pairs  of  fa,  ...,  fa 
is  reduced  to  \  p  (p  + 1)  —  (p  —  2),  at  most.  But  we  can  in  fact  shew, 
whether  the  surface  be  hyperelliptic  or  not,  that  there  are  not  more  than 
3  (p  —  1)  linearly  independent  products  of  pairs  of  fa,  ...,  fa.  For  consider 
the  4  (p—  2)  places  in  which  any  general  quadratic  polynomial,  <3>(2),  vanishes. 
If  fa  fa  be  any  product  of  two  of  the  polynomials  fa,  ...,  fa,  the  quotient 
fafa/&(-}  represents  a  rational  function  having  no  poles  except  such  as  occur 
among  the  zeros*  of  <I>(21  ;  there  are  therefore  at  least  as  many  linearly 
independent  rational  functions,  with  poles  among  the  zeros  of  <I>(2),  as  there 
are  linearly  independent  products  of  pairs  of  fa,  ...,  fa,.  But  the  general 
rational  function  having  its  poles  among  the  4  (p  —  1)  zeros  of  <I>(2),  contains 
only  4>(p  —  1)—  p  +  1,  =3(p  —  1),  arbitrary  constants.  Hence  there  are  not 
more  than  this  number  of  linearly  independent  pairs  of  fa,  ...,  <f>p.  In 
precisely  the  same  way  it  follows  that  there  are  not  more  than  (2/j,  —  l)(j»  —  1) 
linearly  independent  products  of  p,  of  the  polynomials  fa,  ...,  fa. 

111.  But  it  can  be  further  shewn  that  in  general ^  there  are  just 
(2/4  —  1)  (p  —  1)  linearly  independent  products  of  //,  of  the  polynomials 
fa,  ...,  fa',  so  that  there  are 


identical  relations  connecting  the  products  of  p,  of  the  polynomials  fa,  ...,  fa. 

Consider  the  case  p,  =  2.  Take  p  -  2  places  such  that  the  general 
(^-polynomial  vanishing  in  them  is  of  the  form  \fa  +  /j.fa,  A,  and  p  being 
arbitrary,  and  fa,  fa  having  no  zero  common  beside  these  p  -  2  places.  Let 
4>(D>  <|>'(i)  denote  two  general  linear  functions  of  fa,  ...,  fa.  The  polynomial 


is  quadratic  in  fa,  ...,  fa.  It  contains  2p  terms.  But  clearly  these  terms 
are  not  linearly  independent,  for  the  term  $2  fa  occurs  both  in  fa<&w  and 
in  </>2<£>'(1).  Suppose,  then,  that  there  are  terms,  faWw,  occurring  in  fa$>'(l}, 
which  are  equal  to  terms,  ^>i^(1),  occurring  in  fa$>m.  The  necessary  equation 

for  this, 

V®  =  fa 
~         ~  fa  ' 


shews  that  ^(1)   vanishes  in  the  p  zeros  of  fa  which  are  not  zeros  of  fa. 
But  since  these  p  zeros  form  a  set  which  is  a  residual  of  a  set  (of  p  —  2  places) 

*  Here,  as  in  all  similar  cases,  the  zeros  of  the  polynomial  are  its  generalised  zeros  when  it 
is  regarded  as  of  its  specified  grade. 

t  Precisely,  the  theorem  is  true  when  the  surface  is  sufficiently  general  to  allow  the  existence 
of  p-2  places  such  that  the  general  0-polynomial,  vanishing  in  them,  is  of  the  form  X^  +  pfa, 
\  and  M  being  arbitrary  constants,  and  fa,  <f>.2  having  no  common  zero  other  than  the  p  -  2 
places.  We  have  already  given  a  proof  that  this  is  always  the  case  when  the  surface  is  not 
hyperelliptic  (§  102). 


Ill]  PRODUCTS   OF   ^-POLYNOMIALS.  155 

in  which  two  (^-polynomials  vanish,  it  follows*  that  only  one  ^-polynomial 
vanishes  in  these  p  places;  and  such  an  one  is  fa.  Hence  "^(1)  must  be 
a  multiple  of  fa,  and  therefore  XP'(1)  a  multiple  of  fa.  Thus  the  polynomial 


contains  2p  —  1  linearly  independent  products  of  pairs  of  fa,  ...,  fa,. 

Let  now  fa  be  a  ^-polynomial  not  vanishing  in  the  common  zeros  of 
</>,,  fa,  and  let  fa,  ...,  fa  be  chosen  so  that  fa,  fa,  fa,  ...,  fa  are  linearly 
independent.  Consider  the  polynomial 

4>  =  fa<&n  +  fa&  «')  +  fa  \\3fa  +  .  .  .  +  \pfal 

wherein  \3,  ...,  \p  are  arbitrary  constants.  Herein  fa(\^fa  +  ...+\pfa) 
cannot  contain  any  terms  fa  (X/$3  +  .  .  .  +  ^p'fa)  which  are  equal  to  terms 
already  occurring  in  the  part  fa<btl}  +  fa<&'ft),  or  else  \3'<f>3  +  ...  +  \p'fa  would 
vanish  in  the  p  —  2  common  zeros  of  fa  and  fa  ;  and  this  is  contrary  to  the 
hypothesis  that  \fa  +  ufa  is  the  most  general  ^-polynomial  vanishing  in 
these  p  —  2  places.  Hence  the  polynomial  <E>  contains  2p  —  1  +  p  —  2,  or 
Sp  —  3,  independent  products  of  twos  of  the  polynomials  fa,  ...,fa.  As 
we  have  proved  that  a  greater  number  does  not  exist,  3p  —  3  is  the  number 
of  such  products  of  pairs. 

Consider  next  the  case  yu,  =  3.  Since  co-residual  sets  of  2p  —  1  places 
have  f  a  multiplicity  p  —  1,  it  follows  that  the  general  polynomial,  \f(2),  of 
the  second  degree  in  fa,  ...,  fa,  which  vanishes  in  2p  —  3  fixed  places,  and 
therefore  in  2p  —  I  variable  places,  contains  p  arbitrary  coefficients.  If  then 
the  2p—  3  fixed  zeros  of  ^(2)  be  zeros  of  a  definite  polynomial,  fa,  it  follows 
that  ¥<->  is  of  the  form  fa^f^,  ^  being  of  the  first  degree  in  fa,  fa,  ...,  fa. 
Hence,  as  in  the  case  /u-  =  2,  it  can  be  proved  that  if  fa,  fa  be  ^-polynomials 
with  one  common  zero,  the  reduction  in  the  number,  2('3p  —  3),  of  terms 
in  a  polynomial  </>!<!>  (2>  +  fa&{2),  which  arises  in  consequence  of  the  occurrence 
of  terms,  faW®,  in  fa<&'(2),  which  are  equal  to  terms,  -  faW®,  occurring 
in  fa<&{2).  is  at  most  equal  to  p.  Hence  the  polynomial  fa<&®  +  fa<&'{2) 
contains  at  least  5p  —  6  linearly  independent  products  of  threes  of  fa,  ...,  fa. 
Hence  taking  fa,  and  a  quadratic  polynomial  3>"<2»,  such  as  do  not  vanish 
in  the  common  zero  of  fa,  fa,  it  follows  that  a  cubic  polynomial  with  at  least 
op  —  5  linearly  independent  products,  is  given  by 


We  have   thus  proved  that   in  the  cases  /*  =  2,  /A  =  3,  the   polynomial 
contains  (2/u,-  l)(p  —  1)  linearly  independent  products.     Assume  now 
that   4>^-»)    contains   (2/*-  3)  (p-  1)   independent   terms,  and   that    <£<"-2» 

*  From  the  formula  (Chap.  VI.  §  93) 

Q-R  =  2(q-r), 
putting  Q=jp-2,  R=p,  r=l,  we  obtain  q  =  0. 

t  From  Q-q=p-(r  +  l),  putting  r+l=0  (because  2p-  l>2p-2)  Q  =  2p-l,  q=p-l. 


156  THE    ^-POLYNOMIALS    FORM   A   COMPLETE   SYSTEM.  [Ill 


contains  (2/x  —  5)(p  —  1)  independent  terms.  A  general  polynomial 
vanishing  in  the  zeros  of  a  definite  ^-polynomial,  <£2,  will  have  2(/i  —  2)(j9  —  1) 
variable  zeros;  and  the  multiplicity  of  co-residual  sets  of  2  (/A  —  2)(p  —  1) 
places,  when  /x  >  3,  is  (2/j,  —  5)(p  —  1)  —  1,  which  by  hypothesis  is  the  same 
as  the  multiplicity  of  the  sets  of  zeros  of  a  polynomial  <$>,?¥  (>i~z),  in  which 
-2)  nas  i£s  most  general  form  possible.  Hence  the  general  polynomial 
vanishing  in  the  zeros  of  <£2,  is  of  the  form  <f>^^~2).  If  then,  in  a 
polynomial,  (j)^^"^  +  <f>2<&'  (*~v  ,  of  the  yu-th  degree  in  </>l5  ...,  <f)p,  wherein 
<j)1}  $z  have  no  common  zeros,  there  be  terms,  fy.W  '(ft~1)  ,  occurring  in  <£2<l>/('1~1), 
which  are  equal  to  terms,  -  <£1Mr('t~1),  occurring  in  ^>1<I>('t~1),  then  ty^-v  must 
be  of  the  form  ^F^-2*,  and  ^V-1'  of  the  form  c^'^-2',  and  the  resulting 
reduction  in  the  number,  2  (2/i  -  3)(p  -  1),  of  terms  in  ^tl?"*-1*  +  ^2<l>/"t-1), 
is  at  most  equal  to  the  number,  (2//,  —  5)  (p  —  I),  of  terms  in  a  polynomial 
^c*-2*.  Thus,  there  are  at  least 

2  (2,1  -  3)  G>-1)-  (2,1-5X0-1),  =  (^-l)(p-l\ 

linearly  independent  terms  in  the  polynomial  ^^^"^  +  $.,&>'  ^~l)  ;  as  we  have 
proved  that  no  greater  number  exists,  it  follows  that  (2/i  —  l)(p—  1)  is  the 
number  of  linearly  independent  products  of  yu,  of  the  polynomials  <f>1}  ...,  (f>p. 

112.  Another  most  important  theorem  follows  from  the  results  just 
obtained  :  Every  rational  function  whose  poles  are  among  the  zeros  of  a 
polynomial  ^w  can  be  expressed  in  a  form  (pM/tyM.  For  the  most  general 
function  having  poles  in  these  2/u,  (p  —  1)  places  contains  2/x(p  —  1)  —  p+  1 
arbitrary  constants*,  and  we  have  shewn  that  a  polynomial  <&w  contains  just 
this  number  of  terms;  thus  the  quotient  ^**>/¥w,  which  clearly  has  its 
poles  in  the  assigned  places,  is  of  sufficiently  general  character  to  represent 
any  such  function. 

For  further  information  on  the  matter  here  discussed  the  reader  may  consult  Noether, 
Math.  Annal.  t.  xvn.  p.  263,  "  Ueber  die  invariante  Darstellung  algebraischer  Func- 
tionen."  And+  ibid.  t.  xxvi.  p.  143,  "Ueber  die  Normalcurven  fiirjo  =  5,  6,  7." 

In  order  to  explain  the  need  for  the  theorem  just  obtained,  we  may  consider  the  simple 
case  where  the  fundamental  equation  is  that  of  a  general  plane  quartic  curve,  f(x,  y,  z)  =  0, 
homogeneous  coordinates  being  used.  If  we  take  the  four  polynomials, 

^i  =  ^2>  ^2=#2>  ^s=^>  ^h=^> 
which  are  not  ^-polynomials,  from  which  we  obtain 

x  :  y  :  z  =  ^  :  ^3  :  ^4, 

*  When  ^>1.     The  theorem  has  already  been  proved  for  ^i  =  l  (§  98,  Chap.  VI.). 

t  In  the  present  chapter  all  the  polynomials  considered  in  connexion  with  the  fundamental 
equation  have  been  adjoint;  there  is  also  a  geometrical  theory  for  polynomials  of  any  grade  in 
extension  of  the  theory  here  given,  in  which  the  associated  polynomials  are  not  adjoint.  For  its 
connexion  with  the  theory  here,  the  reader  may  compare  Klein,  "Abel.  Functionen,"  Math. 
Annal.  t.  36,  p.  60,  Clebsch-Lindemann-Benoist,  Lemons  sur  la  Geometric,  Paris  1883,  t.  m.,  also 
Lindemann,  Untersuchungen  iiber  den  Riemtmn-Roch''  'schen  Satz  (Teubner  1879),  pp.  10,  30  etc., 
Noether,  Math.  Annal.  t.  15,  p.  507,  "Ueber  die  Schnittpunktssysteme  einer  algebraischen 
Curve  mit  nicht  adjungirten  Curven." 


113]  NOETHER'S  NORMAL  CURVE  IN  HIGHER  SPACE.  157 

then  the  general  rational  function  with  poles  at  the  sixteen  zeros  of  a  polynomial,  ¥<2>,  of 
the  second  order  in  fa,  fa,  fa,  fa,  contains  14  homogeneously  entering  arbitrary  con 
stants.  Now  there  are  only  ten  terms  in  the  general  polynomial  *<2),  of  the  second  order 
in  fa,  ...  ,  ^4  ;  and  these  are  equivalent  to  only  nine  linearly  independent  terms,  because 
of  the  relation  fafa  =  fa*.  Hence  the  rational  function  in  question  cannot  be  expressed  in 
the  form 


113.  The  investigations  in  regard  to  the  ^-polynomials  fa,  ...,  fa,  which 
have  been  referred  to  in  §§  110  —  112,  find  their  proper  place  in  the  con 
sideration  of  the  theory  of  algebraic  curves  in  space  of  higher  than  two 
dimensions. 

Let  fa,  ...,  fa  be  linearly  independent  adjoint  polynomials  of  grade 
(n  -  1)  a  +  n  -  3,  defined,  suppose,  by  the  invariant  condition  that  if 
clt  ...,cp  be  p  independent  places  on  the  Riemann  surface,  fa  vanishes  in 
all  of  d,  ...,  cp  except  a.  Let  xlt  ...,  xp  be  quantities  whose  ratios  are 
defined  by  the  equations 

a?i  :x2  :  ...  :  xp  =  fa  :  fa  :  ...  :  fa. 

We  may  suppose  *  that  there  is  no  place  of  the  original  surface  at  which 
all  of  a:,,  ...,  xp  are  zero,  and,  since  only  the  ratios  of  these  quantities  are 
defined,  we  may  suppose  that  none  of  them  become  infinite. 

Hence  we  may  interpret  #,,  ...,  xp  as  the  homogeneous  coordinates 
of  a  point  in  space  of  p  -  1  dimensions  ;  we  may  call  this  the  point  as. 
Corresponding  then  to  the  one-dimensionality  constituted  by  the  original 
Riemann  surface,  we  shall  have  a  curve,  in  space  of  p  -  I  dimensions.  Its 
order,  measured  by  the  number  of  zeros  of  a  general  linear  function 
A^  +  ...  +  \yxp,  will  be  2/>  -  2.  To  any  place  x  of  this  curve  there  cannot 
correspond  two  places  c,  c'  of  the  original  surface,  unless 

fa(c)  :  fa(c)  :  ...  :  fa  (c)  =  fa  (c')  :  fa(c')  :  ...  :  <^(c'). 

Now,  from  these  equations  we  can  infer  that  the  (^-polynomials  corre 
sponding  to  the  normal  integrals  of  the  first  kind,  have  the  same  mutual 
ratios  at  c  as  at  c'  ;  such  a  possibility,  however,  necessitates  the  existence  of 
a  rational  function  of  the  second  order,  expressible  in  the  form 

MY  —  /*r*/, 

where  X,  p  are  constants  whose  ratio  is  definite,  and  T*',  rj  are  normal 
elementary  integrals  of  the  second  kind  with  unassigned  zeros.  Hence  the 
correspondence  between  the  original  Riemann  surface  and  the  space  curve, 
6^-2,  is  reversible  except  in  the  hyperelliptic  case. 

In  the  hyperelliptic  case  the  equations  of  transformation  are  reducible  to 
a  form 

xl  :  #2  :  .  .  .  :  xp  =  1   :  z  :  z*  :  .  .  .   :  zP~\ 
*  Chap.  II.  §  21. 


158  NOETHER'S  NORMAL  CURVE.  [113 

To  any  point  x  of  the  space  curve  corresponds,  therefore,  not  only  the  place  (s,  z)  of  the 
Riemann  surface,  but  equally  the  place  (  -  s,  z).  The  space  curve  may  be  regarded  as  a 
doubled  curve  of  order  p  —  l.  (Of.  Klein,  Varies,  ub.  d.  Theorie  der  ellip.  Modulfunctionen, 
Leipzig,  1890,  t.  I.  p.  569.) 

For  the  general  case  in  which  p  =  3,  the  curve,  C2p_2,  is  the  ordinary 
plane  quartic  curve.  For  the  general  case,  p  =  4,  the  curve  (7^-2  is  a  sextic 
curve  in  space  of  three  dimensions,  lying*  on  \p(p  4-  1)  —  (3p  —  3),  =  1, 
surface  of  the  second  order  and  %p(p  +  l)(p  +  2)  —  (op  —  5),  =  5,  linearly 
independent  surfaces  of  the  third  order. 

Ex.  If,  for  the  case  jo  =  4,  we  suppose  the  original  surface  to  be  associated  with  the 
equation  f 

f(x,y}  =  tff  (Lx  +  My)  +  xy  (ax*  +  Ihxy  +  by2)  +  Px3  +  Qafiy  +  Rxy* 

+  Sy3  +  Ax2  +  ZHxy  +  Bf  +  Cx  +  Dy  +  1  =  0, 

and  put  Z—xy,  X=x,  Y=y,  as  the  non-homogeneous  coordinates  of  the  points  of  the 
curve  C"2p_2,  the  single  quadric  surface  containing  the  curve  is  clearly  given  by 

U2  =  Z-XY=0, 
and  one  cubic  surface,  containing  the  curve,  is  given  by 

2)  +  PX3  +  QX2Y+RXY* 


Four  other  cubic  surfaces,  T71  =  0,  F"2  =  0,  F3  =  0,  Tr4  =  0,  can  be  obtained  from  t/"3  =  0  by 
replacing  XYby  Z,  respectively  in,  (i)  the  coefficient  of  h,  (ii)  the  coefficient  of  Q,  (iii)  the 
coefficient  of  /?,  (iv)  the  coefficient  of  H  ';  these  are  linearly  independent  of  I73  =  0,  and  of 
one  another.  Other  cubic  surfaces  can  be  obtained  from  U3=0  by  replacing  XY  by  Z  in 
two  of  its  terms  simultaneously  ;  for  instance,  if  we  replace  XY  by  Z  in  the  coefficients  of 
h  and  JT,  we  obtain  a  surface  of  which  the  equation  is  Vl-  U3+Vt=0.  Similarly  all 
others  than  #3=0,  V1  =  0,  ...  ,  F4=0,  are  linearly  deducible  from  these. 

114.  As  an  example  of  more  general  investigations,  consider  now  the 
correspondence  between  the  space  curve  C.2p_2,  for  p  =  4,  and  the  original 
Riemann  surface.  Let  us  seek  to  form  a  rational  function  having  p  +  1  =  5 
given  poles  on  the  sextic  curve.  A  surface  of  order  //,  can  be  drawn  through 
5  arbitrary  points  of  the  curve  when  //,  is  great  enough  ;  we  may  denote 
its  equation  by  ^W=0,  in  accordance  with  §  110.  It  was  proved  that 
the  rational  function  can  be  written  in  the  form  c^w/vpw,  <J>M  being  another 
polynomial,  of  order  p  in  the  space  coordinates,  which  vanishes  in  the  6/^  —  5 
zeros  of  "^^  other  than  the  5  given  points.  Since  a  general  surface  of 
order  /A  contains  (ft  +  3,  3)|  terms,  the  most  general  form  possible  for  <l>('x>, 
when  subject  to  the  conditions  enunciated,  will  contain 

(At  +  3,  3)-(6/x-5) 

arbitrary,  homogeneously  entering,  coefficients  ;  the  polynomials  which 
multiply  these  coefficients,  represent,  equated  to  zero,  all  the  linearly  inde- 

*  §  111  preceding. 

f  Cf.  §  108. 

$  Where  (/x,  v)  is  used  for  the  number  n(/j,-l)...(/j.-v 


115]  PARTICULAR   CURVE   IN   THREE    DIMENSIONS.  159 

pendent  surfaces  of  order  /A  which  vanish  in  the   6/u.  —  5  points  spoken  of; 
they  will  therefore  include  the 


-,  or     *-,-,t- 


surfaces  of  the  /ith  order  which*  contain  the  sextic  curve.  Denote  the 
number  of  these  surfaces  by  r  and  their  equations  by  U^  =  0,  .  .  .  ,  Ur  =  Q. 
Then  the  general  form  of  the  equation  of  a  surface,  <I>W  =  0,  vanishing  in  the 
6/j.  —  5  given  points  will  be 


wherein  \1?  ...,  Xr,  X,  /j,  are  arbitrary  constants,  and  U  is  a  surface  of  order  /*, 
other  than  M^',  which  vanishes  in  the  6/u.  —  5  points,  and  does  not  wholly 
contain  the  curve.  The  intersections  of  the  surface  ^^  =0  with  the  sextic 
are  the  same  as  those  of  the  surface  \^M  +  ^U  =  0  ;  and  the  general  form  of 
the  rational  function  having  the  ^  +  1  =  5  given  points  as  poles  is 


involving    the    right    number    (q  +  l=Q-p  +  l  =  5-4;  +  l)   of    arbitrary 
constants. 


Ex.  i.     There  are  sixteen  of  the  surfaces  X*<M)  +  ^C/T=0  which  touch  the  sextic  (in  points 
other  than  the  6/1  -  5  fixed  points). 

For  there  are  2.5  +  2.4-2,  =16,  places  at  which  the  differential,  dz,  of  the  rational 
function  z=  £7/¥M,  is  zero  to  the  second  order. 


Ex.  ii.     In  the  example  of  the  previous  Article,  prove  that 

86r2  Sf/3     3*73  8C72 

r(*)~W''3z~W'~5z)  -Asa^' 

and  that  the  integrals  of  the  first  kind,  expressed  in  terms  of  X,  F,  Z,  are  given  by 

jfc  J  +  X2  r+  \3Z+  X4)  rfA'/A, 
for  arbitrary  values  of  the  constants  X1}  X2,  X3,  X4f. 

115.  We  abstain  from  entering  on  the  theory  of  curves  in  space  in  this 
place.  But  some  general  considerations  on  the  same  elementary  lines  as 
those  referred  to  in  §§  81  —  83,  as  applicable  to  plane  curves,  may  fitly 
conclude  the  present  chapter^  The  general  theorem  considered  is,  that 
of  the  intersections  of  a  curve,  in  space  of  k  dimensions,  which  is  defined 
as  the  complete  locus  satisfying  k  —  1  algebraic  equations,  with  a  surface 

*  §111. 

t  The  canonical  curve  discussed  by  Klein,  Math.  Annal.  t.  36,  p.  24,  is  an  immediate 
generalisation  of  the  curve  Cap_a  here  explained.  But  it  includes  other  cases  also. 

t  See  the  note  in  Salmon,  Higher  Plane  Curves  (Dublin  1879),  p.  22,  "on  an  apparent 
contradiction  in  the  Theory  of  Curves"  and  the  references  there  given,  which  include  a  reference 
to  a  paper  by  Euler  of  date  1748.  For  further  consideration  of  curves  in  space  see  Appendix  I.  to 
the  present  volume. 


160  PARTICULAR   CURVE   IN   THREE   DIMENSIONS.  [115 

of  sufficiently  high  order,  r,  there  are  a  certain  number,  P,  which  are  deter 
mined  by  prescribing  the  others,  P  being  independent  of  r. 

We  take  first  the  case  of  the  curve  in  three  dimensions,  defined  as  the 
complete  intersection  of  two  surfaces  of  orders  m  and  n,  say  Um  =  0,  Un  =  0. 
The  curve  is  here  supposed  to  be  of  the  most  general  kind  possible,  having 
only  such  singularities  as  those  considered  in  Salmon,  Solid  Geometry 
(Dublin,  1882,  p.  291).  For  instance  the  surfaces  Um=Q,  Un  —  0  are  not 
supposed  to  touch ;  for  at  such  a  place  the  curve  would  have  a  double  point. 
We  prove  that  if  r>m+n  —  4,  all  but  ^mn  (m  +  n  —  4)  +  1  of  the  inter 
sections  of  the  curve  Um  =  0,  Un  =  0  with  a  surface  of  order  r,  Ur  =  0,  are 
determined  by  prescribing  the  others,  whose  number  is 

rmn  —  \mn  (m  +  n  —  4)  —  1. 

For  when,  firstly,  r>m  +  n—l,  the  intersections  of  Ur  =  0  with  the 
curve  are  the  same  as  those  of  a  surface 

Uf        U in  r  r—in        Un  '  r—n        U in,U n  '  r — m—n  =  V, 

wherein  Vr^m,  Vr_n,  Vr_m_n  are  general  polynomials  whose  highest  aggregate 
order  in  the  coordinates  is  that  given  by  their  suffixes.  Hence,  in  analogy 
with  the  argument  given  in  §  81,  it  may  at  first  sight  appear  that,  of  the 
(r  +  3,  3)  coefficients  in  Ur,  we  can  reduce  a  certain  number,  K,  given  by 

K=  (r- m  +  3,  3)  +  (r  -  n  +  3,  3)  +  (r  -  m  -n  +  3,  3), 

to  zero,  by  using  the  arbitrary  coefficients  in  Vr-m,  Vr-n,  Vr_m_n.  This 
however  is  not  the  case.  For  if  Wr—in-n,  Tr_m_n  denote  general  polynomials, 
of  the  orders  of  their  suffixes,  we  can  write  the  modified  equation  of  the 
surface  of  order  r  in  the  form 

TT  —  TT   ( V        -  JT  W          \—TT<V       -  77   T          } 

l/r        ^  m\  '  r—m        u  n  ''  r—m—n)        u  n  \  '  r—n        V  m-1-  r—m—n) 

U m  w»  \  'r—m—n         "  r— m— n       -*-  r—m—n)  =  "• 

Now,  whatever  be  the  values  assigned  to  the  coefficients  in  PFr_m_n,  Tr_m_n, 
the  coefficients  in  Fr_w_n—  Wr-m-n—  Tr_m_n  are  just  as  arbitrary  as  those 
of  Fr_m_n.  And  we  may  use  the  coefficients  in  Wr-m-n>  Tr_m_n  to  reduce 
(r  —  m  —  n  +  3,  3)  of  the  coefficients  in  each  of  the  polynomials 

V        -  JT  W  V       -  IT  T 

'  i — m         ijn''r—m—ny     'r—n        '-'m-Lr—m—n) 

to  zero. 

Hence  the  K  equations  by  which  we  should  reduce  the  number  of 
effective  coefficients  in  Ur  to  (r  +  3,  3)  —  K,  are  really  unaltered  when 
2  (T —  m  —  n  +  3,  3)  of  the  disposeable  quantities  entering  therein,  are  put 
equal  to  zero.  Thus  we  may  conclude,  that  so  far  as  the  intersections  of  Ur 
with  the  curve  are  concerned,  its  coefficients  are  effectively 

(r  +  3,  3)  -  (r  -  m  +  3,  3)  -  (r  -  n  +  3,  3)  +  (r  -  m  -  n  +  3,  3) 
in  number.     Provided  the  linear  equations  reducing  the  others  to  zero  are 


116]  THEOREM  OF  SEQUENCE.  161 

independent,  what  we  prove  is  that  the  number  of  effective  coefficients 
is  certainly  not  more  than  this. 

This  number  can  immediately  be  seen  to  be  equal  to 

rmn  —  \nin  (m  +  n  -  4). 

Hence,  we  cannot  arbitrarily  prescribe  more  than  rmn  —  \nm (m  +  n-  4)  —  1 
of  the  intersections  of  Ur  =  0  with  the  curve. 

This  result  is  obtained  on  the  condition  that  r>m  +  n  —  1.  If  r  =  m  +  n—  1, 
m  +  n—  2  or  m  +  n  —  3,  the  number  of  effective  coefficients  in  Ur  cannot 
be  more  than  in  the  polynomial 

*J,t        U m  '  r—m        Un  V  r_n, 

namely,  than 

(r  +  3,  3)-(r-m+3,  3)-(r-w+3,  3). 
By  the  previous  result  this  number  is  equal  to 

rmn  —  \mn  (m  +  n  —  4)  —  (r  —  m  —  n  +  3,  3), 

and  (r  -  m  -  n  +  3,  3),  =  (r  -  m  -  n  +  1)  (r  -  m  -  n  +  2)  (r  -  m  -  n  -  3)/3  ! , 
vanishes  when  r  =  m  +  n—l,  m  +  n -2,  or  m  +  w-3.  Hence  the  result 
obtained  holds  provided  r  >  m  +  n  —  4. 

If  we  denote  the  number  fynn  (m  +  n  —  4)  +  1  by  P,  the  result  is,  that 
when  r>m  +  n  —  4<,  we  cannot  prescribe  more  than  mnr  —  P  of  the  inter 
sections  of  the  curve  Um  =  0,  Un  =  0  with  a  surface  of  order  r ;  the  prescription 
of  this  number  of  independent  points  determines  the  remaining  intersections. 

Corollary.  Hence  it  follows,  when  (?•+  3,  3)  -  1  >  rmn-  P  +  1,  that 
a  surface  of  order  r  described  through  rmn  —  P  +  1  quite  general  points 
of  the  curve,  will  entirely  contain  the  curve.  Hence,  in  general,  the  curve 
lies  upon  (?-  +  3,  3)-rmn+P  —  1  linearly  independent  surfaces  of  order 
r,  r  being  greater  than  m  +  n  —  4. 

Ex.  i.  For  the  curve  of  intersection  of  two  quadric  surfaces,  P=  1  ;  every  surface  of 
order  r  drawn  through  4r  quite  arbitrary  points  of  the  curve  entirely  contains  the  curve  ; 
the  4r  intersections  of  a  surface  of  order  r,  which  does  not  contain  the  curve,  are  deter 
mined  by  4r-l  of  them.  When  r  =  2,  the  number  (r  +  3,  3)-rmn  +  P-I  is  equal  to  2. 
This  is  the  number  of  linearly  independent  quadric  surfaces  containing  the  curve. 

Ex.  ii.  For  the  curve  of  intersection  of  a  quadric  surface  with  a  cubic  surface,  P  =  4  ; 
of  the  Qr  intersections  of  the  curve  with  a  surface  whose  order  r  is  >1,  6r-4  determine 
the  others.  The  number  (r  +  3,  3)-rwm  +  P-l  is  equal  to  1  when  r  =  2,  and  equal  to  5 
when  r=3;  thus,  as  previously  found,  the  curve  lies  on  one  quadric  surface  and  on  five 
linearly  independent  cubic  surfaces  ;  the  number,  for  any  value  of  r,  is  in  agreement  with 
the  result  of  §  111. 

116.  In  regard  to  the  intersections,  with  the  curve,  of  a  surface  of 
order  m  +  n- 4,  such  a  surface  has  effectively  not  more  coefficients  than  are 
contained  in  the  polynomial 

^m+n-4        U m  '  n— 4  ~  U n  '  m— 4> 
B. 


162  THERE   ARE  p   INTEGRALS  [116 

for  arbitrary  values  of  the  coefficients  in  Fn_4  and  Fm_4.  Here  we  firstly 
suppose  m  >  3,  n  >  3. 

Now  we  can  prove,  as  before,  that 

(m  +  n-l,  3)-O-l,  3)-(m-l,  3)  =  %mn(m  +  n-4)  +  1,  =P. 
Hence,  also  when  m  >  3  and  n  =  3,  2  or  1, 
(TO  +  n  _  i,  3)  _  (m  -  I,  3),  -  \mn  (m  +  n  -  4)  +  1  +  (n  -  1)  (n  -  2)  (n  -  3)/6, 

is  equal  to  P,  and  the  number  of  effective  coefficients  in  a  polynomial 
Um+n-4-  UnVm-i,  wherein  the  coefficients  in  Fm_4  are  arbitrary,  is  as  before 
equal  to  P.  Similarly  for  other  cases. 

Hence  P  is  the  number  of  coefficients  in  a  polynomial  Um+n-t,  which  are 
effective  so  far  as  the  intersections  of  the  curve  with  the  surface  I7m+n_4  =  0 
are  concerned  ;  in  other  words,  P  -  1  of  the  intersections  determine  the 
others.  The  total  number  of  intersections  is  mn  (m  +  n  -  4),  =  2P  -  2. 

The  analogy  of  these  polynomials  of  order  m  +  n  -  4  with  the  (^-poly 
nomials  in  the  case  of  a  plane  curve  is  obvious. 

117.  If  now,  the  homogeneous  coordinates  of  the  points  of  the  curve  in 
space  being  denoted  by  Xlt  X2,  X3,  X4,  the  symbol  [i,  j]  denote  the  Jacobian 
9  (  Um,  Un)/d  (Xi}  Xj),  and  (X1  +  dX,,  X2  +  dX2,  X3  +  dX3,  X4  +  dX,)  denote 
a  point  of  the  curve  consecutive  to  (Xl}  X2,  X3}  X,),  it  follows  from  the 
equations 

9  Um  -.  v      o  Um  ,  Y    ,  ^  Um  j  Y  —  A 

^+        Xs  +  -~  dx*~ 

U*  4-  r  8i^ 
A*       ' 


and  the  similar  equations  holding  for  Un,  that  the  ratios 

X2dX3-  XsdX2  :  X.dX.-X.dX,  :  X,dXz-  X2dX,  :  X,dX. 

-  X.dX,  :  X2dX.  -  X<dX,  :  XzdX,  -X.-  dX3, 
are  the  same  as  the  ratios 

[1,4]:  [2,  4]:  [3,  4]  :  [2,  3]  :  [3,  !]:[!,  2]; 

each  of  these  rows  is  in  fact  constituted  by  the  coordinates  of  the  tangent 
line  of  the  curve.  If  then  u,,  ua,  u3,  ut,  v1}  v.2,  v3,  v,  denote  any  quantities 
whatever,  and,  in  each  of  these  rows,  we  multiply  the  elements  respectively  by 

U2V3  —  U3V2,  U3Vi  —  U^Va,  U^  —  U2V1}  U^t  —  W4Vj,  M2^4  —  W4^2,  ^3^4  —  "5^3, 

and  add  the  results,  we  shall  obtain  for  the  first  row 

2  (u*v3  -  u3v2)  (X2dX3  -  X3dXz)  =  udv  -  vdu, 
where 
u  =  u1Xl  +  u2X.>  +  u3X3  +  u4X4,  du  =  u^X^  +  u2dX2  +  u3dX3  +  u4dXt,  etc., 


117]  WHICH    ARE    EVERYWHERE    FINITE.  163 

and,  for  the  second  row  we  shall  obtain  the  determinant 

t*j      ,          U2     ,         U3     ,          *W4 

o  v    >       3  tr    .       ^\r    >       ~^~v 

O-A-i          vA~2          OJL3          OJL 

O  "!/•      i       o  -yr     >        '-\  -tr     t        ^V 

CA.  i         OA.  2         0  A  3         0  A. , 

which  we  may  denote  by  (uvUmUn). 

From  the  proportionality  of  the  elements  of  the  two  rows  considered, 
it  follows,  therefore,  that  the  ratio  (udv  —  vdu)/(uvUmUn)  is  independent  of 
the  values  of  the  quantities. w1}  ... ,  v4.  This  ratio  is  of  degree 


in  the  homogeneous  coordinates;  namely,  if  Xl}  X2,  X3,  X4  be  replaced  by 
pXlt  pX2,  pX3,  pXt,  the  ratio  will  be  multiplied  by  p- <»»+»- *).  Hence,  if 
Um+n-4  be  any  polynomial  of  degree  m  +  n  —  4,  the  product 

Um+n-i  (udv  —  vdu)/(uV  Um  Un} 

is  a  functional  differential,  independent  of  the  arbitrary  factor  of  the  homo 
geneous  coordinates. 

The  integral, 

udv — vdu 


ju 


f       TT     TT  \  j 
(UVUmUn) 

can  only  be  infinite  at  the  places  where  the  curve  is  intersected  by  the 
surface  (uvUmUn)  =  0  :  if  u  =  0,  v  =  0  be  regarded  as  the  equations  of  planes, 
this  equation  expresses  that  the  straight  line  u  =  0,  v  =  0,  is  intersected 
by  the  tangent  line  of  the  curve  at  the  point  (Xlt  X2)  Xs,  Z4).  The 
differential 

udv  -  vdu,  =  2  (uava  -  u3v2}  (X2dX3  -  X3dX2), 

is  zero,  to  the  second  order,  when  the  line  u=0  =  v  is  intersected  by  the 
tangent  line,  whose  coordinates  are  X2dX3  -  X3dX2>  etc.  Hence  the  ratio 
(udv  —  vdu)/(uvUmUn)  is  never  infinite,  and  the  integral  above  is  finite  for  all 
points  of  the  curve. 

Hence*,  since  Um+n_^  contains  P  terms,  we  can  obtain  P  everywhere-finite 
algebraical  integrals. 

The  same  result  is  obtained  if  ult ...,  v4  be  polynomials  in  the  coordinates, 
MI,  ...,  ut  being  of  the  same  degree,  and  v1} ... ,  v4  of  the  same  degree. 

As  stated,  we  are  considering  a  curve  without  singular  points.  If  the  curve  had  a  double 
point,  the  polynomial  (uvUmUn)  would  vanish  at  that  point,  for  all  values  of  w1(  ...,  v4.  We  could 
then  prescribe  Um+n_4  =  Q  to  pass  through  the  double  point,  thus  obtaining  a  reduction  of  one  in 
the  number  of  finite  integrals.  Etc. 

11—2 


164  TRANSFORMATION   TO   A   RIEMANN   SURFACE.  [117 

Ex.  i.     For  a  plane  curve  of  order  n,  without  multiple  points,  prove  similarly  that  we 
can  obtain  p  finite  algebraical  integrals  in  the  form 

!>„  _  3  (udv  —  vdu)l(uvf ), 

where /(#!,  #2,  #3)  =  0  is  the  homogeneous  equation  of  the  curve,  U=u1x1+u2x2  +  tiye3,  etc., 
and  (uvf)  denotes  a  determinant  of  three  rows. 


Ex.  ii.     Shew  that  a  surface  of  order  m  +  n  —  4  +  fj.  which  vanishes  in  all  but  two  of  the 
intersections  of  the  curve  in  space  with  a  surface  of  order  p,  £^,.  =  0,  is  of  the  form 


where  X,  X1}  ...  ,  \P  are  arbitrary  ;  and  that  an  integral  of  the  third  kind  is  of  the  form 

udv  —  vdu 


/i 


p  (uvl7mUn)' 


118.  Retaining  still  the  convention  that  u  =  0,  v  =  0  are  the  equations  of 
planes,  let  u'  =  0,  v'  =  0  be  the  equations  of  other  planes  whose  line  of  inter 
section  does  not  coincide  with  the  line  u  =  0  =  v. 

From  the  equations 

zu-v  =  0,  su'-v'  =  0,  Um=Q,   Un  =  0, 

wherein  z,  s  have  any  values,  we  can  eliminate  the  coordinates  of  the  points 
of  the  curve  in  space,  and  obtain  a  rational  equation,  (s,  z)  —  0,  with  which 
we  may  associate  a  Riemann  surface*.  To  any  point  of  the  curve  corre 
sponds  a  single  point,  z  =  v/u,  s  =  v'/u,  of  the  Riemann  surface  ;  to  any  point 
of  the  Riemann  surface  will  in  general  correspond  conversely  only  one  point 
of  the  curve  in  space.  Hence  the  Riemann  surface  will  have  mn  sheets, 
the  places,  at  which  z  has  any  value,  being  those  which  correspond  to  the 
places,  on  the  curve  in  space,  at  which  the  plane  zu  —  v  =  0  intersects  this 
curve.  Thus  the  Riemann  surface  will  have  2mn  +  2p  —  2  branch  places, 
p  being  the  deficiency  of  the  surface.  These  are  the  places  where  dz  is  zero 
of  the  second  order.  Thus  they  correspond  to  the  places,  on  the  curve  in 
space,  where  udv  —  vdu  is  zero  to  the  second  order.  We  have  seen  that  these 
are  given  as  the  intersections  of  this  curve  with  the  surface  (iivUmUn}  =  0, 
of  order  m  +  n  —  2  ;  their  number  is  therefore  mn  (m  +  n  —  2)  =  Zmn  +  2P  —  2. 
Hence  the  number  P,  obtained  for  the  curve  in  space,  is  equal  to  the 
deficiency  p  of  the  Riemanu  surface  with  which  it  is  reversibly  related. 
The  same  result  can  be  proved  when  u,  v  are  polynomials  of  any,  the  same, 
order,  and  u',  v'  are  polynomials  of  any,  the  same,  order. 

And  from  the  reversibility  of  this  transformation  it  follows  that  the 
everywhere-finite  integrals  for  the  Riemann  surface  are  the  same  as  those 
here  obtained  for  the  curve  in  space. 

*  We  may  of  course  interpret  the  equation  as  that  of  a  plane  curve  ;  a  particular  case  is  that 
in  which  this  curve  is  a  central  projection  of  the  space  curve. 


119]  REFERENCES.  165 

Ex.     Prove  that  if  elt  e2,  e3  be  such  that  el+ez  +  e3=0, 
(b-c)(c-a)(a-b)  =  (b-c)(a-d)/(e2-e3)  =  (c-a)(b-d)/(e3-e1)  =  (a-b)(c-d)!(e1-e2), 

the  points  of  the  curve  aX2  +  bY2+cZ2+dT*  =  0,  X2+  Y2  +  Z2+T2  =  0  can  be  expressed 
in  terms  of  two  quantities,  x,  y,  satisfying  the  equation  y2  =  4  (x  -  ej  (&  -  e2)  (x  —  e3),  in  the 
form  T  :  X  :  Y  :  Z 


=y  ••  V^c  [(a?  -  etf  -  (e1  -  ez)  (et  -  &,)]  :  *J^a  [(x  -  e2)2  -  (e2  -  es)  (e2  -  ej\ 

:\/a-b[(x-  e3)2  -  (e3  -  ej  (e3  -  e2)]. 
Find  x,  y  in  terms  of  X,  Y,  Z,  T  in  the  form 


(e2  -  e3)  Ar/    b  -c  +  e2  (e3  -  el 


See  Mathews,  London  Math.  Soc.  t.  xix.  p.  507. 

119.  As  already  remarked  we  have  considered  here  only  the  case  of  a  non-singular 
curve  in  space  which  is  completely  denned  as  the  intersection  of  two  algebraical  surfaces. 
For  this  case  the  reader  may  consult  Jacobi,  Crelle,  t.  15  (1836),  p.  298  ;  Pliicker,  Crelle. 
t.  16,  p.  47  ;  Clebsch,  Crelle,  t.  63,  p.  229  ;  Clebsch,  Crelle,  t.  64,  p.  43  ;  Salmon,  Solid 
Geometry  (Dublin,  1882),  p.  308  ;  White,  Math.  Annal.  t.  36,  p.  597  ;  Cayley,  Collected 
Works,  passim.  For  the  more  general  case,  in  connexion  however  with  an  extension  of  the 
theory  of  this  volume  to  the  case  of  two  independent  variables,  the  following,  inter  alia, 
may  be  consulted  :  Noether,  Math.  Annal.  t.  8  (1873),  p.  510  ;  Clebsch,  Comptes  Rendus  de 
I'Acad.  des  Sciences,  t.  67,  July—  December,  1868,  p.  1238  ;  Noether,  Math.  Annal.  t.  2, 
p.  293,  and  t.  29,  p.  339  (1887)  ;  Valentiner,  Acta  Math.  t.  ii.  p.  136  (1883)  ;  Halphen, 
Journal  de  VEcole  Polyt.  t.  lii.  (1882),  p.  1  ;  Noether,  Abh.  der  Akad.  zu  Berlin  (1882)  ; 
Cayley,  Collected  Works,  Vol.  v.  p.  613,  etc.  ;  and  Picard,  Liouv.  Journ.  de  Math. 
1885,  1886  and  1889. 

Ex.  i.     Prove  that 
(r+t,  k)-2(r  +  k- 


where  (r,  M)  denotes  r(r-  !)...(/•-  /u+  1)/M  !,  m1(  ...  ,  mk_^  k  are  any  positive  integei-s,  r  is  a 
positive  integer  greater  than  mx+  »i2+...  +mk_1-  k  -  1,  2  denotes  a  summation  extending 

to  all  the  values  i=l,  2,  ...,  (k-  1),  2  denotes  a  summation  extending  to  every  pair  of  two 

2 

unequal  numbers  chosen  from  the  series  m^  m2,  ...,  mk_l,  and  so  on.  Hence  infer  that 
of  the  intersections  of  a  general  curve  in  space  of  k  dimensions,  which  is  determined  as  the 
complete  locus  common  to  k-l  algebraic  surfaces  of  orders  mlt  m2,  ...,  mk_l,  with  a 
surface  of  order  r,  all  but 


are  determined  by  the  others.     The  result  is  known  to  hold  for  £  =  2.     We  have  here  been 
considering  the  case  £  =  3. 

Ex.  ii.  With  the  notation  and  hypotheses  employed  in  Salmon's  Solid  Geometry  (1882), 
Chap.  XII.  (p.  291)  (see  also  a  note  by  Cayley,  Quarterly  Journal,  t.  vn.,  or  Collected  Works, 
Vol.  v.  p.  517),  where  m  is  the  degree  of  a  curve  in  space,  n  is  its  class,  namely  the  number 
of  its  osculating  planes  which  pass  through  an  arbitrary  point,  r  is  its  rank,  namely  the 
number  of  its  tangents  which  intersect  an  arbitrary  line,  a  is  the  number  of  osculating 
planes  containing  four  consecutive  points  of  the  curve,  /3  the  number  of  points  through 
which  four  consecutive  planes  pass,  x  the  number  of  points  of  intersections  of  non-consecu- 


166  EXAMPLES.  [119 

tive  tangents  which  lie  in  an  arbitrary  plane,  y  the  number  of  planes  containing  two  non- 
consecutive  tangents  which  pass  through  an  arbitrary  point,  h  the  number  of  chords  of  the 
curve  which  can  be  drawn  through  an  arbitrary  point,  g  the  number  of  lines  of  intersection 
of  two  non-consecutive  osculating  planes  which  lie  in  an  arbitrary  plane,  ^  the  number  of 
tangent  lines  of  the  curve  which  contain  three  consecutive  points,  prove,  by  using  Pliicker's 
equations  (Salmon,  Higher  Plane  Curves,  1879,  p.  65)  for  the  plane  curve  traced  on  any 
plane  by  the  intersections,  with  this  plane,  of  the  tangent  lines  of  the  curve  in  space,  that 
the  equations  hold, 

(1)  n  =  r(r-l)-2x-3m-3^,  (3)     r  =  n(n-  1)  -2#-3a, 

(2)  a  =  3r(r-2)-6^-8(m+^),  (4)     m+^  =  3n(n-2)-Gg-8a, 

pl-l=%r(r-2>)-x-m  —  ^=%n(n  —  S)—g  —  a  .....................  (A), 

p1  being  the  deficiency  of  this  plane  curve. 

Prove  further,  by  projecting  the  curve  in  space  from  an  arbitrary  point,  and  using 
Pliicker's  equations  for  the  plane  curve  in  which  the  cone  of  projection  is  cut  by  an 
arbitrary  plane,  the  equations 

(5)  r  =  m(m-I)-2h-3p,  (7)     m  =  r  (r-  l)-2#- 

(6)  S.+?i  =  3m(m-2)-6A-8/3,  (8)     /3  = 

/>2-l  =  im(»i-3)-A-0  =  ir(r-3)-y-n-$.  ....................  (B), 

p2  being  the  deficiency  of  this  plane  curve. 

From  the  equations  (1)  and  (7)  we  can  infer  n  -  m  =  3n  —  3m  —  2  (x-y\  and  therefore 

Hence  Pi=pz. 

Ex.  iii.  For  the  non-singular  curve  which  is  the  complete  intersection  of  two  algebraic 
surfaces  of  orders  p,  v,  prove  (cf.  Salmon,  Solid  Geometry,  pp.  308,  309)  that  in  the  notation 
of  Ex.  ii.  here, 


Hence,  by  the  equations  (B)  of  Ex.  ii.  prove  that,  now, 
p^Pz^pvfa  +  v-ty  +  l. 
This  is  the  number  we  have  denoted  by  P. 

Ex.  iv.     Denoting  the  number  pl=p2j  in  Ex.  ii.,  by  p,  prove  from  equations  (5)  and  (B) 
that 

=  3  (r+j8-2m). 


Hence  shew  that  if,  through  a  curve  C  of  order  m,  lying  on  a  surface  S  of  order  /n,  we 
draw  a  surface  of  order  v,  cutting  the  surface  S  again  in  a  curve  C"  of  order  m',  and  if 
p,  p'  denote  the  values  of  p  for  these  curves  C,  C'  respectively,  then 


(see  Salmon,  pp.  311,  312).     Shew  that  each  of  these  numbers  is  equal  to  the  number,  i, 
of  points  in  which  the  curves  C,  C'  intersect,  and  interpret  geometrically  the  relation 

i+r  +  0=m(fji  +  v-2'). 

Ex.  v.  If  in  Ex.  iv.  a  surface  <£  of  order  p  +  v  -  4  be  drawn  through  (/*  +  v  —  4)  m'  —p'  +  1, 
or  i—l+p',  of  the  points  of  the  curve  C",  prove  that,  so  far  as  its  intersections  with  the 
curve  C  are  concerned,  the  surface  (f)  contains  effectively  p  terms.  Prove  further  that  0 
contains  the  curve  C'  entirely. 


119]  EXAMPLES.  167 


Ex.  vi.  Prove  that  a  surface  of  order  p  +  v  —  4  passing  through  i—  1  of  the  intersections 
of  the  curves  0,  C',  in  Ex.  iv.,  will  pass  through  the  other  intersection. 

Ex.  vii.  An  example  of  the  case  in  Ex.  iv.  is  that  in  which  /i  =  2,  i/  =  2,  m  =  3,  m'  =  l. 
Then  C"  is  a  straight  line  and  p'  =  0  :  hence  p  is  given  by  —  2  =  2p  -  2.  Hence,  for  the 
cubic  curve  of  intersection  of  two  quadrics  having  a  common  generator,  p  =  Q.  And  in  fact 
coordinate  planes  can  be  chosen  so  that  the  homogeneous  coordinates  of  the  points  of  the 
cubic  can  be  expressed  in  the  form 

X  :   Y  :  Z  :  T=\   :  6  :  0*  :  <93, 

6  being  a  variable  parameter.  For  instance  (using  Cartesian  coordinates)  the  polar  planes 
of  a  fixed  point  (X'Y'Z1)  in  regard  to  quadrics  confocal  with  X2/a  +  Yzjb  +  Z*/c  =  l  are  the 
osculating  planes  of  such  a  cubic  curve,  the  coordinates  of  whose  points  are  expressible  in 
the  form 

XX'  =  (a  +  \}*l(a-b)(a-c\   YY'  =  (b  +  \)3l(b-c)(b-a),  ZZ'  =  (c  +  \)3/(c-a)(c-b), 
\  being  a  variable  parameter. 

Ex.  viii.  For  the  quintic  curve  of  intersection  of  a  quadric  and  a  cubic  surface  having 
a  common  generator  we  obtain,  from  Ex.  iv.,  putting  m'=l,  p'  =  0,  m  =  5,  that  p  =  2  ;  the 
results  of  Exx.  iv.,  v.,  vi.  can  be  immediately  verified  for  this  curve  ;  further,  if  the  surfaces 
be  taken  to  be  yU-zV=0,  yS-zT=0,  where  U,  V  are  of  the  first  degree  in  x,  y,  z  and 
S,  T  of  the  second  degree,  and  we  put  y  =  zg,  x=zrj,  we  obtain 


where  the  Greek  letters  au  a2,  .  .  .  denote  polynomials  in  £  of  the  degrees  of  their  suffixes. 
Hence,  if  a-  be  defined  by  the  equation, 

XI(T  =  2?  (X^ft  +X1a1y1  +  Vi2)  +  Vfo  +  Xi  (al72  +  «27i)  +  2Vi«2  , 

we  obtain  o-2  =  (£,  1)6  ;  £,  a-  are  rational  functions  of  x,  y,  z  and  x,  y,  z  are  rational  functions 
of  £,  o-. 

Ex.  ix.  Prove  that  if  the  sextic  intersection  of  a  cubic  surface  and  a  quadric  surface, 
break  up  into  a  quartic  curve  and  a  curve  of  the  second  order,  the  numbers  p,  p'  for  these 
curves  are  p  =  l,  p'  =  Q  or  p=0,  p'=  -  1  according  as  the  curve  of  the  second  order  is  a 
plane  curve  or  is  two  non-intersecting  straight  lines. 

Ex.  x.  In  analogy  with  Ex.  iv.,  shew  that  the  deficiencies  of  two  non-singular  plane 
curves  of  orders  m,  m'  are  connected  by  the  equation 

m  (m  +  m'  -  3)  -  (2jo  -  2)  =  mm'  =  m'  (m  +  m'  -  3)  -  (2p'  -  2), 

and  further  in  analogy  with  Ex.  v.  that  if  a  plane  curve,  of  order  m+m'  -3,  be  drawn 
through  (m+.m1  -  3)  m'  -p'+l  independent  points  of  the  curve  of  order  m',  only  p  -  I  of  its 
intersections  with  the  curve  of  order  m  can  be  prescribed. 

Further  indications  of  the  connexion  of  the  theory  of  curves  in  space  with  the  subject 
of  this  chapter  will  be  found  in  Appendix  I. 


[120 


CHAPTER    VII. 

COORDINATION  OF  SIMPLE  ELEMENTS.    TRANSCENDENTAL  UNIFORM 

FUNCTIONS. 

120.  WE  have  shewn  in  Chapter  II.  (§§  18,  19,  20),  that  all  the  funda 
mental  functions  are  obtainable  from  the  normal  elementary  integral  of  the 
third  kind.  The  actual  expression  of  this  integral  for  any  given  form  of 
fundamental  equation,  is  of  course  impracticable  without  precise  conventions 
as  to  the  form  of  the  period  loops,  and  for  numerical  results  it  may  be  more 
convenient  to  use  an  integral  which  is  denned  algebraically.  Of  such 
integrals  we  have  given  two  forms,  one  expressed  by  the  fundamental 
integral  functions  (Chap.  IV.  §§  45,  46),  the  other  expressed  in  the  terms  of 
the  theory  of  plane  curves  (Chap.  VI.  §  92,  Ex.  ix.).  In  the  present  Chapter 
we  shew  how  from  the  integral  P^'",  obtained  in  Chap.  IV.*,  to  determine 
algebraically  an  integral  Qf' a  for  which  the  equation  Qx' a  =  Qz'c  has  place ; 

incidentally  the  character  of  P*' " ,  as  a  function  of  z,  becomes  plain ;  and 
therefore  also  the  character  of  the  integral  of  the  second  kind,  £%' a ,  which 
was  found  in  Chap.  IV.  (§§  45,  47). 

This  determination  arises  in  close  connexion  with  the  investigation  of 
the  algebraic  expression  of  the  rational  function  of  x  which  was  obtained  in 
§  49  and  denoted  by  -fy  (x,  a ;  z,  clt  ...  cp).  It  was  there  shewn  that  every 
rational  function  of  x  can  be  expressed  in  terms  of  this  function.  It  is  shewn 
in  this  Chapter  that  any  uniform  function  whatever,  which  has  a  finite 
number  of  distinct  infinities,  which  may  be  essential  singularities,  can  be 
expressed  by  such  a  function. 

Further,  it  is  here  shewn  how  to  obtain  an  uniform  function  of  x  having 
only  one  zero,  at  which  it  vanishes  to  the  first  order,  and  one  infinity ;  and 
that  any  uniform  function  can  be  expressed  in  factors  by  means  of  this 
function. 

*  For  the  integral  of  the  third  kind  obtained  in  Chap.  VI.  the  reader  may  compare  Clebsch 
and  Gordan,  Theorie  der  Abel.  Functionen  (Leipzig,  1866),  p.  117,  and,  for  other  important  results, 
Noether,  Math.  Annul,  xxxvn.  (1890),  pp.  442,  448;  also  Cayley,  Amer.  Journal,  v.  (1882),  p.  173. 


122]  NOTATION.  169 

121.     Let  Wi'a,  ...,Upa  denote  any  p  linearly  independent  integrals  of 
the  first  kind,  vanishing  at  the  arbitrary  place  a.     Let  t  denote  the  infinit 
esimal  at  x,  and  let  Du*,  ......  ,  Du*  denote  the  differential  coefficients  of  the 

integrals  in  'regard  to  t,  all  of  which  are  everywhere  finite.  Let  d  ,  ...,  cp 
denote  any  p  fixed  places  of  the  Riemann  surface,  so  chosen  that  no  linear 
aggregate  of  the  form 


where  Xx,  ...,  \  are  constants,  vanishes  in  all  the  places  c,,  ...,  cp,  but  such 
that  one  linear  aggregate  of  this  form  vanishes  in  every  set  of  p  —  1  of  these 
places*;  and  let  Wi(x)  denote  the  linear  aggregate,  of  this  form,  which 
vanishes  in  all  of  c1}  ...,  cp  except  d,  and  is  equal  to  1  at  the  place  c;. 

Then  Wi(x)  is  expressible  as  the  quotient  of  two  determinants;  the 
denominator  has  Dusr  for  its  (r,  s)th  element,  the  numerator  differs  from  the 
denominator  only  in  the  t'-th  row,  which  consists  of  the  quantities  Du[  ,  .  .  .  , 
DM*  ;  thus  w1(x),  ...,  (Op(x)  are  determinable  algebraically  when  «*,  ...  ,  uxp  are 
given.  Conversely  the  differential  coefficients  of  the  normal  integrals  of  the 
first  kind  (§§  18,  23)  are  clearly  expressible  by  wl(x),  ...,  wp(x),  in  the  form 

H;  O)  =  wj  (x}  £li  (d)  +  ......  +  cop  (x)  fli  (Cp). 

We   have   already   used   ef*    as    a    notation   for   the    normal    integral 

i    rx  fx 

H-  .  I    nt  (ai)  dtx.   In  this  chapter  we  shall  use  the  notation  V*'a  =  I    ca{  (x)  dtx. 

67TI  J  a  J  a 

If  the  period  of  the  integral  u^  at  the  j-ih  period  loop  of  the  first  kindf 
be  denoted  by  Citj,  we  can  express  vfa  as  the  quotient  of  two  determinants, 
the  denominator  having  Cjti  for  its  (i,j)tfi  element,  and  the  numerator  being 
different  from  the  denominator  only  in  the  tth  row  which  consists  of  the 
elements  u*'a,  ...,  ux'  a. 

122.     Consider  now  the  function  of  #  expressed  j  by 

p 

rx,  a        -s?          /_\  -p-r,  a 
'    -  Z  a)r(z)L       , 

r=\ 

z  being  any  place  whatever.  The  function  is  clearly  infinite  to  the  first 
order  at  the  place  z,  like  —t~l,  tz  being  the  infinitesimal  at  z  ;  it  is  also 
infinite  at  each  of  the  places  cl}  ...,  cp,  and,  at  Cj,  like  &i(*)£  ,  tc.  being  the 
infinitesimal  at  C;.  The  function  has  no  periods  at  the  period  loops  of  the 

*  Thus  there  exists  no  rational  function  infinite  only  to  the  first  order  at  each  of  clt  ...,  cp. 
Cf.  §§  23,  26. 

t  C(i>  is  the  quantity  by  which  the  value  of  u*'a  on  the  left  side  of  this  period  loop  exceeds 
the  value  on  the  right  side.  See  the  figure,  §  18,  Chap.  II. 

t  Klein,  Math.  Annul,  xxxvi.  p.  9  (1890),  Neumann,  loc.  cit.  p.  14,  p.  259. 


170  A   FUNDAMENTAL   FUNCTION  [122 

first  kind.  At  the  tth  period  loop  of  the  second  kind  the  function  has  the 
period 

fM*)- 1  r^ooao,.), 

r=\ 

which,  as  remarked  (§  121),  is  also  zero.  Hence  the  function  is  a  rational 
function  of  x.  It  vanishes  at  the  place  a.  We  shall  denote  the  function  by 
•fy  (x,  a;  z,  c1}  ...,  Cp).  It  is  easy  to  see  that  it  entirely  agrees,  in  character, 
with  the  function  given  in  §  49. 

For  the  places  c1;  ...,  cp  have  been  chosen  so  that  no  aggregate  of  the 
form 

Xjflj  (#)  + +  XpOj,  (x) 

vanishes  in  all  of  them.  Hence  (Chap.  III.  §  37)  the  general  rational  function 
having  poles  of  the  first  order  at  the  places  z,  c1}  ... ,  cp  is  of  the  form  Ag  -f  B, 
where  g  is  such  a  function,  and  A,  B  are  constants.  These  constants  can  be 
uniquely  determined  so  that  the  residue  at  the  pole,  z,  is  —  1,  and  so  that 
the  function  vanishes  at  the  place  a. 

Ex.  For  the  case^>  =  l,  if  we  use  Weierstrass's  elliptic  functions,  the  places  x,  a,  z,  c, 
being  represented  by  the  arguments  u,  a,  v,  y1}  and  put  x  =  $u,  y  =  %>'(u)  etc.,  we  may 
take,  supposing  v  not  to  be  a  half  period, 


and  obtain 

or 

Vr(#,  a;  z,  Cj)  = 


and  any  doubly  periodic  function  can  be  expressed  linearly  by  functions  of  this  form, 
in  which  the  same  value  occurs  for  yx  and  different  values  for  v.     (Of.  §  49,  Chap.  IV.) 

123.     Since  mdz),  =  ^r  Vs'  c,  is  a  linear  function  of  ^(z),  ...,  Qp(z),  it 
atz     * 

follows    that    &>;(»/j7   is    a  rational   function    of  z\   and  r*'a,  =  -^-  H^'*, 
I  at  °*s 


=  (ux,*\<       is  such  that*  Tx'a  1-  is  a  rational   function  of  z\   hence 
\dz     *>  c  J  dt,  "    I  dt 


*  Throughout  this  chapter  such  an  expression  as  f(z)  —  is  used  to  denote  the  limit,  when  a 


variable  place  £  approaches  the  place  z,  of  the  expression  /(£)  ^-,  t  being  the  infinitesimal  for 


124]  WITH  p  +  1    POLES.  171 

Idz 
i/r  (x,  a;  z,  d,  ...,Cp)j-jr  is  a  rational  function  of  z.     It  is  easy  also  to  see, 

dc- 

from  the  determinant  expression  of  W{  (z),  that  &>j  (z)  -~  is  a  rational  function 

cut 

of  cn  ...,  cp. 

Hence  i/r  (x,  a;  z,  d,  ...,  cp)/  -j-  is  a  rational  function  of  the  variables  of 
all  the  places  x,  a,  z,  d ,  . . . ,  cp. 

Further,  as  depending  upon  z,  i/r  (x,  a  ;  z,  c1}  ...,  cp)  is  infinite  only  when 

F*'  a  is  infinite ;  and  F*' a,  =  -j-  Uz'a,  is  infinite  only  when  z  is  at  x  or  at  a. 

atz     x> a 

At  the  place  x,  Tx'a  is  infinite  like   -7-  log  tx,  namely  like  the  inverse  of  the 

atx 

infinitesimal  at  the  place  x. 

Hence  ty  (x,  a  ;  z,  cl ,  . . . ,  cp),  regarded  as  depending  upon  z,  is  infinite  only 
when  z  is  in  the  neighbourhood  of  the  place  x,  or  in  the  neighbourhood  of  the 
place  a.  At  the  place  x,  ^r(x,  a;  z,  c1;  ...,  cp)  is  infinite  like  the  positive 
inverse  of  the  infinitesimal,  at  the  place  a  it  is  infinite  like  the  negative  inverse 
of  the  infinitesimal.  The  rational  function  of  z  denoted  by 

i  /  \  Idz 

yfca;  z,  d,  ...,  Cp)l  fa 

will  therefore  be  infinite  at  the  place  x  like T  and  at  the  place  a 

wl  +  1  z  —  x 

like ,  where  w^  +  1,  w.2  +  1  denote  the  number  of  sheets  that 

w2  +  L  z  —  a 

wind  at  the  places  x,  a  respectively;  and  will  be  infinite  at  every  branch 

A 

place,  like  ,          ^-w,  t  being  the  infinitesimal  at  the  place,  w  +  l  the  number 

\U)  -7-  1  j  t 

of  sheets  that  wind  there,  and  A  the  value  of  ty(x,  a;  z,  cl}  ...,  cp)  when  z  is 
at  the  branch  place. 

The  actual  expression  of  the  function  i/r  (x,  a ;  z,cly  ...,  cp)  is  given  below 
(S  130). 

124.     From  the  function  ty(x,  a ;  z,  cl} ...,  cp)  we  obtain  a  function, 

„  t      N      J**(jf' a;  *•  °"  - •  c"> dt*       n*f. a -  I  v'r- c r*' a 
E(x,z)  =  e  ,=e*      r=i 

wherein   c   is  an  arbitrary  place,  which    has  the  following  properties,  as  a 
function  of  x. 

the  neighbourhood  of  the  place  z.    When  z  is  not  a  branch  place  -  =  1 ;  when  w  +  l  sheets  wind 

ttt 

at  Z>  dt  =  ^W  +  1^"  ^cf'  ^  2'  3;  CliaP-  I-)-     AmPle  practice  in  the  notation  is  furnished  by  the 
examples  of  this  chapter. 


172  UNIFORM   FUNCTION   WITH   ONE   ZERO.  [124 

(i)  It  is  an  uniform  function  of  x.  For  the  exponent  has  no  periods  at 
the  period  loops  of  the  first  kind,  and  at  the  iih  period  loop  of  the  second 
kind  it  has  the  period 

27T^'C-    I     V^n^Cr) 
r=l 

which,  as  follows  from  the  equation 

n,;  (Z)  =  «!  (Z)  flf  (Cl)  +  ......  +  0)p(z)fli  (Cp), 

is  equal  to  zero.     Further  the  integral  multiples  of  27rt,  which  may  accrue 
to  Hx'  a  when  x  describes  a  contour  enclosing  one  of  the  places  z,  c,  do  not 

Z,    C 

alter  the  value  of  the  function. 

(ii)     The  function  vanishes  only  at  the  place  z,  and  to  the  first  order. 
(iii)     The  function  has  a  pole  of  the  first  order  at  the  place  c. 

(iv)  The  function  is  infinite  at  the  place  d,  like  evi  tci  ,  tc.  being  the 
infinitesimal  at  the  place.  We  may  therefore  speak  of  c1}  ...,  cp  as  essential 
singularities  of  the  function. 

125.  In  order  to  call  attention  to  the  importance  of  such  a  function 
as  this,  we  give  an  application.  Let  R  (x}  denote  a  rational  function,  having 
simple  poles  at  a.l,  ...,  ctm,  and  simple  zeros  at  /?1;  ...,  /3W.  We  suppose  these 
places  different  from  the  fixed  places  c,  a,  c1}  ...,  cp.  Then  the  product 


is  an  uniform  function  of  as,  which  becomes  infinite  only  at  the  places  c1}  ...  cp  ; 
at  Ci  it  is  infinite  like  a  constant  multiple  of 


Now,  in  fact,  \ogF(x)  is  also  an  uniform  function  of  x:  for  it  is  only 
infinite  at  the  places  clf  ...,  cp,  and,  at  the  place  d,  like  —  (  X  V°?'  r\  F^a. 

\r=l  ' 

r  rpf  (x\ 

Hence  the  integral   U  log  F(as\  =    -TTT^/  dx,  taken  round  any  closed  area 
J  J  F(x) 

on  the  Riemann  surface  which  does  not  enclose  any  of  the  places  Ci,  . ..,  cp,  is 

m  a     f  (It 

certainly  zero,  and  taken  round  the  place  d  is  equal  to  —  2  V ^  r  I  ~ _',  taken 

r=l  J    t 

Ci 

round  d,  and  is,  therefore,  also  zero. 

But  an  uniform  function  of  x  which  is  infinite  only  to  the  first  order  at 
each  of  cls  ...,  cp  does  not  exist.  For  the  places  c1}  ...,  cp  were  chosen 
so  that  the  conditions  that  the  periods  of  a  function,  of  the  form 


125J  FACTORIZATION   OF  ANY   RATIONAL   FUNCTION.  173 

wherein  \lt  ...  ,\p  are  constants,  should  be  zero,  namely  the  conditions 
\A.(d)+  ......  +  V^-  (CP)  =  °>  r=l,  2,  ......  ,p, 

are  impossible  unless  each  of  Xn  .  ..,  \p  be  zero. 

m 

Hence  we  can  infer  that  S  Va.r>  r  =  0,  for  i  =  I,  2,  .  .  .  ,  p,  and  that  F  (x)  is 

r=l 

a  constant;  this  constant  is  clearly  equal  to  F  (a),  for  E  (a,  z)  —  1  for  all 
values  of  2. 

Hence,  any  rational  function  can  be  expressed  as  a  product  of  uniform 
functions  of  x,  in  the  form 


where  a1,  ...,ocm  are  the  poles  and  /31;  ...,  ftm  the  zeros  of  the  function.  We 
have  given  the  proof  in  the  case  in  which  the  poles  and  zeros  are  of  the  first 
order.  But  this  is  clearly  not  important. 

Further,  the  zeros  and  poles  of  a  rational  function  are  such  that 

2    V"C  =    2    V?r'°,  i=l,  2,  ...,p, 

r=l  r=l 

c  being  an  arbitrary  place.  This  is  a  case  of  Abel's  Theorem,  which  is  to  be  considered  in 
the  next  Chapter.  We  remark  that  in  the  definition  of  the  function  JS(x,  z)  by  means  of 
Eiemann  integrals,  the  ordinary  conventions  as  to  the  paths  joining  the  lower  and  upper 
limits  of  the  integrals  are  to  be  regarded  ;  these  paths  must  not  intersect  the  period  loops. 

r,       •        r,        , ,  „:*;,  a      ,         (X  —  Z  a  —  C\  .    -p.  .  (x  —  Z)  (« —  C] 

Ex.  i.     For  the  case  «  =  0,  n      =log  (  and  E  (x.  z)=± J-± ' 

z,c          °  \x-ca-zj  (x-c)(a-z) 

Ex.  ii.     For  the  case  p  —  l,  supposing  the  place  c  represented  by  the  argument  y,  we 
have 


fz  (v 

=       t(*t«:  *»ci»  ...,<V)&-»- 

J  c  J  y 


and  therefore 


a-  (u  —  y)  a-  (a  —  v) 
Ex.  iii.     Prove,  if  a',  cf  denote  any  places  whatever,  that 

E(x,c'}E(a',z)~ 

Ex.  iv.  The  rational  function  of  #,  ^(x,  f ;  z,  clt  ... ,  cp),  will,  beside  f,  have  p  zeros, 
^y  Yi>  ••• »  7p>  such  that  the  set  f,  yu  ... ,  yp  is  equivalent  with  or  coresidual  with  the  set 
z,  c,,  ... ,  cp  (§§  94,  96,  Chap.  VI.).  Hence,  in  the  product 

^ (x>  f  >  zi  c\->  •••  >  CP)  "A  (-r>  z\  C>  7i>  •••  >  VP)> 


174  MODIFICATION   WHEN   THE   FIXED   PLACES  [125 

the  zeros  of  either  factor  are  the  poles  of  the  other,  and  the  product  is  therefore  a  constant. 
To  find  the  value  of  this  constant,  let  x  approach  to  the  place  z.  Then  the  product 
becomes  equal  to 

-  tx-1  .  tx  [Dx^  (x,z;  £  7l,  ...  ,  yv}]x=z  . 

It  is  clear  from  the  expression  of  >//•(#,  a  ;  z,  clt  ...  ,  cp)  which  has  been  given,  that 
Dx^f(x,  a  ;  z,  ct,  ...,  cp)  does  not  depend  upon  the  place  a.  Thus,  by  the  symmetry,  we 
have  the  result 

z;  f,  yi,  ...,  yp)  =  -  D,+  (z,  a  ;  £  yn  ...,  yp) 


where  a  is  a  perfectly  arbitrary  place,  and  the  sets  z,  clt  ...,  cln  f,  yu  ...,  yp  are  subject  to 
the  condition  of  being  coresidual. 

Hence  also  if  W(x  ;  z,  c1,  ...,  cp)  denote  the  expression 

Dx  [+  (x,  a;  z,  c1?  ...  ,  cp)  -  1^1  a]  , 
we  have 

W(z;  f,  yj,  ...,  yp)  =  W(£  ;  «,  c^  ...,  cp), 

provided  only  the  set  2,  clt  ...,  cp  be  coresidual  with  the  set  f,  yn  ...,  yp. 

Ex.  v.     Prove,  with  the  notation  of  Ex.  iv.,  that 
^(x,  a;  z,  clt  ...,  cp)^(a,  a;  f,  yl5  ...,  yp)  =  ^(^,  f;  2,^,  ...,cp)^(^,  a;  £  y1?  ...,yp). 

126.  These  investigations  can  be  usefully  modified*;  we  can  obtain 
a  rational  function  ty  (x,  a  ;  z,  c),  having  the  same  general  character  as 
•fy  (x,  a;  z,  Cj,  ...,  Cp)  but  simpler  in  that  its  poles  occur  only  at  two  distinct 
places  z,  c,  of  the  Riemanu  surface,  and  we  can  obtain  an  uniform  function 
E  (x,  z)  having  only  one  zero,  of  the  first  order,  at  the  place  z,  which  is 
infinite  at  only  one  place,  c,  of  the  surface. 

The  limit,  when  the  place  x  approaches  the  place  c,  of  the  rth  differential 
coefficient  of  £li(x)  in  regard  to  the  infinitesimal  at  the  place  c,  will  be 
denoted  by  ftfCc),  or  simply  by  n<r).  We  have  shewn  (Chap.  III.  §  28) 
that  there  are  certain  numbers  kL>  ...,  kp,  such  that  no  rational  function 
exists,  infinite  only  at  the  place  c,  to  the  orders  k1}  ...,  kp.  The  periods  of  a 
function  of  the  form 

T\k  -  1  -pia;,  a       ^     T^fc,  -  1  r\x,  a  •*       Tjfc/j-1  -pa;,  a 

Vc        lc      ~^L'c        Lc       ~  ......  -^P^e         Lc     ' 

wherein  Xlt  ...,\p  are  constants,  and  2)kc~lTxc'a  denotes  f  the  limit,  when  z 
approaches  c,  of  the  &th  differential  coefficient  of  the  function  IF'  "  in  regard 
to  the  infinitesimal  at  c,  /u,  being  an  arbitrary  place,  are  all  of  the  form 


These  periods  cannot  all   vanish   when   k   is  any  one  of  the   numbers 
klt  ...,kp;  thus  the  determinant  formed  with  the  p2  quantities  OJ          does 

*  Giinther,  Crelle,  cix.  p.  199  (1892). 

t  For  purposes  of  calculation,  when  c  is  a  branch  place,  it  is  necessary  to  have  care  as  to  the 
definition. 


127]  COALESCE  AT  ONE  PLACE.  175 

not  vanish ;  but  \ ,  . . . ,  \p  can  be  chosen  to  make  all  these  periods  vanish 
when  k  is  not  one  of  the  numbers  klt  . . . ,  kp. 

127.     Consider  now  the  function 

i   /  \         T&> a  o   /  ,v\  r»    /  ~\ 

•yr(x,a;  z,c)=    L  ,    ili(z)  ,    •    ,    *«yvf] 


,(*r-D 


wherein  r  =  1,  2,  .  .  .  ,  £>. 

Since  the  period  of  Tx'  a,  at  the  ith  period  loop  of  the  second  kind,  is 
£li(z),  the  periods  of  the  elements  of  the  first  column  of  the  first  deter 
minant  are  the  elements  of  the  various  other  columns  of  that  determinant. 
Thus  the  function  is  a  rational  function  of  x. 

We  shall  denote  the  minors  of  the  elements  of  the  first  column  of  the 
first  determinant,  divided  by  the  second  determinant,  by  1,  —  twj  (2),  ...,  —  a)p  (z), 
although  that  notation  has  already  (|  121)  been  used  in  a  different  sense. 
Before,  o.\  (z)  was  such  that  o>;  (cr)  =  0  unless  r  =  i  in  which  case  Wi  (d)  =  1  ; 

now,  as  is  easy  to  see,  [-D*7""1  Wi  (z)~]g=e  is  0  or  1  according  as  r  is  not  equal  or 

ft 

is  equal  to  i.     The  integrals      coi(z)dtz  are  linearly  independent  integrals  of 

the  first  kind  (cf.  Chap.  III.  §  36). 
Then  the  function  can  be  written 


t=i 
~l 


the   function  is  infinite  at  z  like  —  t~l,  tz  being  the  infinitesimal  at    the 
place  z,  and  is  infinite  at  c  like  * 


tc  being  the  infinitesimal  at  the  place  c.     It  is  not  elsewhere  infinite.     The 
function   vanishes    when   as   approaches   the   place   a.      As   before   (§    123) 

fdz 
•fy(x,a;  z,  c)/-jr  is  a  rational  function  of  all  the  quantities  involved;  and 

/    CLt 

•^  (x,  a  ;  z,  c),  as  depending  upon  z,  is  infinite  only  at  the  places  x,  a,  in  each 
case  to  the  first  order. 

*  This  is  clear  when  c  is  not  a  branch  place,  since  then,  when  x  is  near  to  c,  r*'"  is  infinite 
like  --  —  ;  and  the  (fc-l)th  differential  coefficient  of  this  in  regard  to  c  is  -  \k-l(x-c)~*. 

When  c  is  a  branch  place,  exactly  similar  reasoning  applies  if  we  first  make  a  conformal  repre 
sentation  of  the  neighbourhood  of  the  place,  as  explained  in  Chap.  II.  §§  16,  19. 


176  MODIFIED   FUNCTION   WITH   ONE   ZERO.  [128 

128.  If  now  R(x)  be  a  rational  function  with  poles  of  the  first  order  at 
the  places  zlt  ...,  zm,  it  is  possible  to  choose  the  constants  \,  ...,  \p  so  that 
the  difference 

R  (as)  -  Xi^/r  (x,  a  ;  zly  c)-\^(x,  a;  z2,c)-  ......  -Xm>/r(#,  a;  zm,  c) 

is  not  infinite  at  any  of  the  places  zlt  ...,  zm;  this  difference  is  therefore 
infinite  only  at  the  place  c,  and  is  infinite  at  c  like 

-(A,  l&j-l*;*1  +  ......  +  Ap  'fep-l  t;kp), 

where 

At  =  X1&>;  (^)  +  ......  +  \mCOi  (>m),  (i  =  1,  2,  .  .  .  ,  p). 

But,  a  rational  function  whose  only  infinity  is  that  given  by  this  ex 
pression,  can  be  taken  to  have  a  form 


wherein  A  is  a  constant;  and  we  have  already  remarked  (§  126)  that  the 
periods  of  this  function  cannot  all  be  zero  unless  each  of  Alt  ...,  Ap  be  zero. 
Hence  this  is  the  case,  and  we  have  the  equation 

R(x)  =  A  +  \-^(x,  a;  zlt  c)  +  ......  +  \mty(x,  a;  zm,  c), 

whereby  any  rational  function  with  poles  of  the  first  order  is  expressed  by 
means  of  the  function  ty(x,  a;  z,  c).  It  is  immediately  seen  that  the 
equations  Al  =  Q=...  =  Ap  enable  us  to  reduce  the  constants  X^  .  ..,  Xm  to 
the  number  given  by  the  Riemann-Roch  Theorem  (Chap.  III.  §  37). 

When  some  of  the  poles  of  the  function  R  (x)  are  multiple,  the  necessary 
modification  consists  in  the  introduction  of  the  functions 

Dzty  (x,  a  ;  z,  c\  D\ty  (as,  a;  z,  c),  ....... 

Ex.     If  »!(#),  •••>«*(#)  denote  what  are  called  <at(o;),  ...,  u»p(x)  in  §  121,  and   the 
notation  of  §  127  be  preserved,  prove  that 

P  ki~l_ 

mr(z)=  2  u>i(z)Dc       u>r(c), 

t=l 
and  that 


129.     From  the  function  ^  (x,  a  ;  z,  c)  we  derive  a  function  of  ar,  given  by 

fV(ar,a;«,c)««»  Hx-a  -  2  F2'cD*r"'r^" 

E  (x,  z)  =  e  °  ,  =  e  *'      »-=i 

rg 
where,  in  the  notation  of  8  127,  V*'e  =      a)r(z}dtz,  which  has  the  following 

-'c 

properties  : 

(i)     It  is  an  uniform  function  of  x  ;  there  exists  in  fact  an  equation 


•   z,c  •£>     T7*' 

iv,    =»  2«  r_ 

r=l 


130]  ALGEBRAICAL   EXPRESSION   OF   THE   FUNCTIONS.  177 

(ii)     The  function  vanishes  to  the  first  order  when  the  place  x  approaches 
the  place  z  ;  and  is  equal  to  unity  at  the  place  a. 

(iii)     The  function  is  infinite  only  at  the  place  c,  and  there  like 

_!     I  Vz;°\kr  -It;*- 
tc    er=l 

As  before  we  can  shew  that  any  rational  function  R(x),  with  poles  at  aly  ...,  a,n,  and 
zeros  at  fa,  ...,  /3m,  can  be  written  in  the  form 


this  being  still  true  when  some  of  the  places  au  ...,<%,  or  some  of  the  places  fa,  ...,  /3OT 
are  coincident. 

130.  We  pass  now  to  the  algebraical  expression  of  the  functions  which 
have  been  described  here*.  We  have  already  (Chap.  IV.  §  49)  given  the 
expression  of  the  function  \|r  (x,  a;  z,  c1}  ...,  cp)  in  the  case  when  all  the 
places  a,  z,  cl5  ...,  cp  are  ordinary  finite  places.  In  what  follows  we  shall 
still  suppose  these  places  to  be  finite  places;  the  necessary  modifications 
when  this  is  not  so  can  be  immediately  obtained  by  a  transformation  of 
the  form  x  =  (£  —  k)~l,  or  by  the  use  of  homogeneous  variables  (cf.  §  46, 
Chap.  IV.,  §  85,  Chap.  VI). 

If,  s  being  the  value  of  y  when  x  =  z,  we  denote  the  expression 


byf  (z,  x),  and  use  the  integrands  &>i(#),  ...,  Q>p(x)  defined  in  §  121,  the 
rational  expression  of  ty(x,  a;  z,  C1}  ...,  cp),  which  was  given  in  §  49,  can  be 
put  into  the  form 

g 
^  (x,  a  ;  z,  d,  .  .  .  ,  Cp)  =  (z,  x)  -  (z,  a)  -  z  wr  (z)  [(ci}  x)  -  (a,  a)]. 

r=\ 

In  case  z  be  a  branch  place,  the  expression  (z,  x)  is  identically  infinite  in 
virtue  of  the  factor  f  (s)  in  the  denominator,  and  this  expression  can  no 
longer  be  valid.  But,  then,  the  limit,  as  £  approaches  z,  of  the  expression 

*  It  is  known  (Klein,  Math.  Annal.  xxxvi.  p.  9  (1890);  Giinther,  Crelle,cix.  p.  199  (1892))  that 
the  actual  expressions  of  functions  having  the  character  of  the  functions  i//(x,  a;  z,  clt  ...,  cp), 
E  (x,  z),  Qr  i  have  been  given  by  Weierstrass,  in  lectures.  Unfortunately  these  expressions  have 
not  yet  (August,  1895)  been  published,  so  far  as  the  writer  is  aware.  Indications  of  some  value 
are  given  by  Hettner,  Gotting.  Nachr.  1880,  p.  386;  Bolza,  Gotting.  Nachr.  1894,  p.  268; 
Weierstrass,  Gesamm.  Werke,  Bd.  ii.  p.  235  (1895),  and  in  the  Jahresbericht  der  Deuts.  Math.- 
Vereinigung,  Bd.  iii.  (Nov.  1894),  pp.  403—436.  But  it  does  not  appear  how  far  the  last  of  these 
is  to  be  regarded  as  authoritative  ;  and  it  has  not  been  used  here.  The  reader  is  recommended 
to  consult  the  later  volumes  of  Weierstrass's  works. 

t  This  notation  has  already  been  used  (§  45).     It  will  be  adhered  to. 

B.  12 


178  ALGEBRAICAL   EXPRESSION   OF   THE   FUNCTIONS.  [130 

jit 

(£,  x)  -~ ,  wherein  t  is  the  infinitesimal  at  the  place  z,  is  finite*  ;  if  we  denote 

(MI 

dz 

this   limit   by  (z,  x)  -j- ,  and  introduce   a   similar   notation   for   the   places 
uit 

Cj,  . ..,  cp,  we  obtain  the  expression 
i/r  0,  a ;  z,  d,  . . . ,  Cp)  =  [(z,  x)  -  (z,  a)]  ^  -  2   a)r  (z} .  [(a,  x)  -  (a,  a)]  ~  , 

which,  as  in   §  49,  has   the  necessary  behaviour,  for  all  finite  positions  of 
z,  d,  GI , . . . ,  Cp. 

From  this  expression  we  immediately  obtain  (§  45) 


131.     In  a  precisely  similar  way  it  can  be  seen  (see  §  127)  that 
^  (x,  a ;  z,  c)  =  [(z,  x)  -  (z,  a)]  ^  -  2  <*>r  (z)  D*J~l  j[(c,  as)  -  (c,  a)]  ^4  , 

wherein  DkJ~l  |[(c,  x)  -  (c,  a)]  ^|  =  limit^  [(^J^  {[(£  *)  ~  (S  «)]  §}]  5 

for  this  expression  can  be  written  as  the  quotient  of  two  determinants,  in 
the  manner  of  §  49,  and  the  integrands  f^  (z),  . . . ,  £lp(z)  are  linear  functions 
of  the  p  integrands 

<£j  (z)  dz    z<f>-i  (z)  dz          z*1*1  <f>!  (z)  dz    </>2  (z)  dz 
/'(«)#'  T7!?  dt'  ""     f  («)      dt'  f(s)  di' ' 

these  latter  quantities  can  therefore  be  introduced  in  the  determinants  in 
place  of  Hj  (z),  . . . ,  £lp  (z),  the  same  change  being  made,  at  the  same  time, 
for  the  quantities  ^(c),  ...,  Op(c),  throughout.  Then  it  can  be  shewn 
precisely  as  in  §  49  that  the  expression  is  not  infinite  when  x  is  at  infinity. 
In  regard  to  finite  places,  it  is  clear  that  the  expression 

Tfr-1  it(r    <r\-(r   a\\  —  I  -  7)**  P°'y 
U9       \ [\c,  x)      \c,  a)]   ,  f,  -  uc   jrXt a , 


regarded  as  a  function  of  x,  has  the  same  character,  when  x  is  near  to  c,  as 
the  function  Dfcr~1ra;'a. 

c  c 

Hence,  also,  it  follows  that  E(x,  z)  has  the  form 


*  /'  M,  when  r)  is  very  nearly  s,  vanishes  to  order  i  +  w,  and  dfldt  to  order  w  (see  Chap.  VI. 
§  87).     Or  the  result  may  be  seen  from  the  formula 


(Chap.  IV.  §  45). 


132]  EXAMPLES. 

132.     Ex.  i.     For  the  case  (p  =  1)  where  the  surface  is  associated  with  the  equation 

f  =  (x,  1)4, 

if  the  values  of  the  variables  x,  y  at  the  place  a  be  respectively  a,  b,  and  the  values  at  the 
place  q  be  ct,  dv  respectively,  then 


d,  dz     .        .         s+y 
(a)  when  (cls  d\)  is  not  a  branch  place  CDI(S)  =  -  ^  ,  ft,  ^)  =  2s(2_ 


and 


r    s+y            s  +  b__~\dz  _djdzr  _d1+y__  dt  +  b 

('r'  a  '•  *>  ci)  =  \Zs(z-x}  ~  2s  (z-a)]  dt      s  ~dt  [.2^  (c,  -  x)  2^  (ct  -  a)  J 

_  J.  dz  rs+y  _  s  +  b  _  d^+y     d± 
~ 


z-a 


(/3)  when  (ct,  d\)  is  a  branch  place,  in  the  neighbourhood  of  which 

M--  —    C      a?^  =  limit  of  — ^^—  .2*=  — ^— 


and 

•fy  (so,  a ; 


_?±b_~\(k_^(!lz(__y__  b      } 

2*  (z  -  a)  J  dt      2s  dt  \A  (q  -  x}     A  (^  -  a)  j 


_  _!  dz  (s+y  _  s  +  b  _     y  b    | 

~  2s  dt  [z  -  x     z-a     c-^  —  x     c^  —  a) 

If  (s,  2)  be  not  a  branch  place,  ^  jf  =  ^  ;  if  (5,  2)  be  a  branch  place,  in  the  neighbour- 

1  dz        ..     .,     ,,     1    ,,.        1 
hood  of  which  x=z+t\  y  =  Bt  +  ... ,  ^  ^  ,  =  limit  of  ^  2«,  =-g. 

Ex.  ii.  For  the  case  (/>  =  2)  where  the  surface  is  associated  with  the  equation  y2  =/(#), 
where  f(x}  is  an  integral  function  of  x  of  the  sixth  order,  we  shall  form  the  function 
^(x,  a;  z,  cn  02)  for  the  case  where  clt  c2  are  branch  places,  so  that /(c1)=/(c.2)  =  0,  and 
shall  form  the  function  \ff(x,a;  z,  c)  for  the  case  when  c  is  a  branch  place,  so  that/(c)=0. 

When  c1;  c2  are  branch  places,  in  the  neighbourhood  of  which,  respectively,  0;=^+^, 
y  =  Altl  +  ...,  andtf=c2+«22,  y  =  Afa  +  ...,  so  that  Al2=f'(c1~),  A<?=f'(c2),  we  have 

and 


r    s+y  s  +  b    "1  dz  _  l_  dz  /_g^c2  (  J/_         b    \ 

^a;*C|>^"ia«(«-*)    2s(2-«)J^    sUfftK-^V^-*    q-«/ 


When  c  is  a  branch  place,  in  the  neighbourhood  of  which  .r=< 
so  that  A*=f  (c),  the  numbers  klt  k2  are  1,  3  respectively  (Chap.  V.  §  58,  Ex.  ii.).  In  the 
definition  of  the  forms  ^(z),  o>2(2)  (§  127)  we  may,  by  linear  transformation  of  the  2nd, 
3rd,  ...,  (/)  +  l)th  columns  of  the  numerator  determinant,  and  the  same  linear  transforma 
tion  of  the  columns  of  the  denominator  determinant,  replace  Ql(z),  ...,  Qp(z)  by  the 
differential  coefficients  of  any  linearly  independent  integrals  of  the  first  kind.  In  the  case 
now  under  consideration  we  may  replace  them  by  the  differential  coefficients  of  the 

integrals   I  —  ,    1-5-  .     Hence  the  denominator  determinant  becomes 

12—2 


180 
limit, =e 


HYPERELLIPTIC   CASE. 


[132 


dt 


x  dx          =  limits =c 
2w  dt 


'  \dt 


c5\ 
4J! 


Hence 


=  limit,.  = 


•\_dz 

2s  dt 


z  dz 


. 


'"A* 


and 


1  dz      z  dz 
2s  dt'    2*  dt 

I  dx      xdx 


1  dzc  —  z 
2s  eft  ^T 


Hence 


1  dz 


Further 


but 


Hence  the  function  ^  (a?,  a  ;  s,  c)  is  given  by  the  expression 

s+b 


_2«(f  -*)     2s  (2 


b  ~]dz  - 

-  a)  J  dt 


A  2s  dt  \c-x 

z  —  c 


1  dz(A-B(x-c)        A-B(a-c}    \ 
2s  ^\     (^--c)2      y         (a-c)2        /' 


JKr.  iii.  Apart  from  the  algebraical  determination  of  the  function  ^(x,  a;  z,  cls  ...,  cp) 
which  is  here  explained,  it  will  in  many  cases  be  very  easy*  to  determine  the  function  by 
the  methods  of  Chapter  VI.  It  is  therefore  of  interest  to  remark  that,  when  the  function 
VT  (a?,  a  ;  z,  clf  ...  ,  ep)  is  once  obtained  the  forms  of  independent  integrals  of  the  first  and 
second  kinds  can  be  immediately  obtained  as  the  coefficients  in  the  first  few  terms  of  the 
expansion  of  the  function  in  the  neighbourhood  of  its  poles,  in  terms  of  the  infinitesimals 
at  these  poles. 


*  An  adjoint  polynomial  *  of  grade  (n-l)<r  +  n-2  which  vanishes  in  the  p  +  1  places 
z,  clt  ....  cp  will  vanish  in  n+p-3  other  places.  The  general  adjoint  polynomial  of  grade 
(n-1)  ff  +  n-2  which  vanishes  in  these  n+p-3  places  will  be  of  the  form  \*  +  /*e,  where  X  and 
/t  are  constants.  The  function  f(x,  a  ;  z,  clt  ....  c,)  is  obtained  from  X  +  /t0/*,  by  determining 
X  and  yu  properly.  Cf.  Noether  (toe.  cit.)  Math.  Annal.  xxxvii, 


132]  THE   FUNCTION   i|r   IS   FUNDAMENTAL.  181 

In  fact,  if  tj,  be  the  infinitesimal  in  the  neighbourhood  of  the  place  ci}  arid  Mr,  ;  denote 

Ci,  x) 


D<\_(C"  'i) 


the  expansion  of  >/<•(#,  a;  z,  c1?  ...,  cp),  as  a  function  of  x,  in  the  neighbourhood  of  the 
place  Ci,  has,  as  the  coefficient  of  ti~l,  the  expression  o>i  (z),  which  is  one  of  a  set  of  linearly 
independent  integrands  of  the  first  kind,  while  the  coefficient  of  ^  is 


Now  the  elementary  integral  of  the  second  kind  obtained  in  Chap.  IV.  (§§  45,  47) 

with  its  pole  at  a  place  c,  when  z  is  the  current  place,  is  E^  a  =  I  dzDc(z,  c),  whether  c  be 

J  a 
a  branch  place  or  not,  and  when  z  is  near  a  branch  place  this  must  be  taken  in  the  form 


Hence  the  coefficient  of  ^  in  the  expansion  of  ^(x,  a;  z,  cl}  ...,  c^,),  when  x  is  near  to  cit 
is  equal  to 

DtEla  -  S  «,(*)*•„„ 

*         r=\ 

This  is  the  differential  coefficient  of  an  integral  of  the  second  kind,  with  its  pole  at  cf  , 
the  current  place  being  z.  We  shall  see  that  the  integral  of  the  second  kind  with  its  pole 
at  any  place  2  can  be  expressed  by  means  of  the  functions  Ee  ,  ...,  Ee  (§135,  Equation  x.). 

Ex.  iv.  Similar  results  hold  for  the  expansion  of  the  function  ^  (x,  a  ;  z,  c),  as  a  func 
tion  of  x,  when  x  is  in  the  neighbourhood  of  the  place  c.  If  tc  be  the  infinitesimal  at  this 
place,  the  terms  involving  negative  powers  are 


of  which  the  coefficients  of  the  various  powers  of  tc  are  differential  coefficients  of  linearly 
independent  integrals  of  the  first  kind  ;  the  terms  involving  positive  powers  are 


where  Piy  k  is  the  limit,  when  the  place  .v  approaches  the  place  c  of  the  expression 


Among  the  coefficients  of  these  positive  powers  of  te,  only  those  are  important  for 
which  t  is  one  of  the  numbers  ^  ,  .  .  .,{;„.  This  follows  from  the  fact  that  Dek  ~  l  r*'  a,  when 
k  is  not  one  of  the  numbers  *lf  ...,  kp,  is  expressible  by  those  of 


of  which  the  indices  ^-  1,  kz-  1,  ...,  are  less  than  k-  1,  together  with  a  rational  function 
of  x  (Chap.  III.  §28). 


COMPARISON    OF   THE   TWO    REPRESENTATIONS  [132 

Ex.  v.     In  the  expansion  of  the  function  ^  (x,  a  ;  «,  c)  whose  expression  is  given  in 
Example  ii.,  the  terms  involving  negative  powers  are 


,-     A        _. 
2s          di  '  Tc       2s       clt't3' 


and  the  terms  involving  positive  powers  are 


where  the  quantities  A,  B,  ...,  E  are  those  occurring  in  the  expansion  of  y  in  the  neigh 
bourhood  of  the  place  c ;  this  expansion  is  of  the  form  y  =  At  +  Bt3  +  Ct»  +  Df  +  Et*  + . . . . 

Ex.  vi.     If  in  Ex.  v.  the  integrals  of  the  coefficients  of  t,  t3  and  t5  be  denoted  by 
FI,  F3Z,  FZ,  find  the  equation  of  the  form 

Fi=\Fi+p.F3*  +  integrals  of  the  first  kind  +  rational  function  of  (s,  2) 
which  is  known  to  exist  (Chap.  III.  §§  28,  26  ;  Chap.  V.  §  57,  Ex.  ii.),  X  and  p.  being 
constants. 

Prove,  in  fact,  if  the  surface  be  associated  with  the  equation 

7/2  =  (x  -  cf  +pl  (X  -  C)5  +  pz  (X  -  C)4  +p3  (X  -  C)3  +Pt  (X  -  Cf  +pb  (X  -  c) 

that 

^  +  2^?2  +Pi  (z  -  c)J  =  -  ^~Y  +  constant. 

133.  We  pass  now  to  a  comparison  of  the  two  forms  we  have  obtained 
for  each  of  the  rational  functions  -^  (as,  a;  z,  GI,  ...,  cp),  ty(x,  a;  z,  c),  one 
of  which  was  expressed  by  the  Riemann  integrals,  the  other  in  explicit 
algebraical  form. 

The  cases  of  the  two  functions  are  so  far  similar  that  it  will  be  sufficient 
to  give  the  work  only  for  one  case  ijr  (x,  a ;  z,  clf  ...,  cp),  and  the  results  for 
the  other  case. 

From  the  two  equations  (§§  122,  130) 

•\Jr  (x,  a ;  z,  GI,  . . . ,  Cp)  =  F*' a  —  2,  o)i  (z)  Tc'.  , 

i=\ 

^(X,a:  z,Cl,...,cp)  =  [(z,x)-(z,a)]-£-i  «<(*)[(*,  as)-  (d,  a)]  £ , 

Ujli          {,=1 

we  infer,  denoting  the  function 


byff*'a,  that 


1=1 


133]  OF   THE   FUNCTION    A/r.  183 

The   function  H*'a  is  not   infinite  at  the  place  z,  but  is  algebraically 
infinite  at  infinity;  it  has  the  same  periods  as  F*'  a.     The  equation  (ii)  shews 

that  Hx'a  I  -y-  is  a  rational  function  of  z,  while  the  equation 

/  at 

x  a  dz        P 

at     j-=i  ci 


*'  a 


gives  the  form  of  F*' a  /  -^-  as  a  rational  function  of  z. 

I  at 

Integrating  the  equation  (iii)  in  regard  to  z,  we  obtain 

p 

nx,  a,        -r)Z,  c    .     •*?     TT-2,  c  ux> a  /•    \ 

z,c   =Px,a+   ^    Vi      Hc,  (IV), 

i=l 

where  c  is  an  arbitrary  place,  and  P^  °a  is  the  integral  of  the  third  kind,  as  a 
function  of  z,  which  was  determined  in  Chap.  IV.  (§§  45,  46). 

Since  the  integral  of  the  second  kind  E^'a,  obtained  in  Chap.  IV. 
(§§  45,  46),  is  equal  to  DzP*^",  we  deduce  from  the  last  equation,  inter 
changing  x  and  z,  and  also  a  and  c,  and  then  differentiating  in  regard  to  z, 

T?x'a  _i_  f1    jrx>a  n  rjs'c       r>Tis>c          m-fx>a        ri21'0  /   \ 

&z      +2,     Kf       X>z/fCi     =  JJgU^a,    =DzIlZiC,  =Ta  (v), 

and  thence,  using  equation  (iii)  to  express  rx'a, 

E*z> a  =  [(z,  x}  -  (z,  a}}  |  +  £  [„,  (z)  H*  a-Vfa  DZH^ c]      (vi), 

which*  gives  the  form  of  £%'   /  -£  as  a  rational  function  of  ^. 

/   ott 

The  difference  of  two  elementary  integrals  of  the  second  kind  must  needs  be  a  function 
which  is  everywhere  finite,  and  therefore  an  aggregate  of  integrals  of  the  first  kind.  The 
equation  (v)  expresses  the  difference  of  E*' a  and  1^' a  in  this  way.  But  it  should  be 
noticed  that  the  coefficients  of  the  integrals  of  the  first  kind  in  this  equation,  which 
depend  upon  z,  become  infinite  for  infinite  values  of  z.  They  are  the  quantities 

D  ffz'c. 

Z         Cj 

From  the  equation  (iv)  we  have 

r,x,a_x,a        P     ^x.a.jZ.c 
^.c-^c-.f^i       Hc.     > 

wherein  the  coefficients  of  V?*  on  the  right  may  be  characterised  as  integrals  of  the 
second  kind.     From  this  equation  also,  if  the  periods  of  V?*  at  thejth  period  loops  of  the 

*  An  equation  of  this  form  is  given  by  Clebsch  and  Gordan.  Abel.  Functnen.  (Leipzig,  18G6) 
p.  120. 


184  ALGEBRAIC    FORM   OF   INTERCHANGE  [133 

first  and  second  kind  be  denoted  by  C^j  and  C'i,j  respectively,  we  obtain,  as  the  corre 
sponding  periods  of  P^'  * 


from  these  equations  the  periods  of  E*'  a  are  immediately  obtainable.  These  equations 
may  be  used  to  express  the  integrals  H*]  °  in  terms  of  the  periods  of  f^  "  at  the  period 
loops  of  the  first  kind. 

134.  But  all  these  equations  are  in  the  nature  of  transition  equations; 
they  connect  functions  which  are  algebraically  derivable  with  functions  whose 
definition  depends  upon  the  form  of  the  period  loops.  We  proceed  further 
to  eliminate  these  latter  functions  as  far  as  is  possible,  replacing  them  by 
certain  constants,  which,  in  the  nature  of  the  case,  are  not  determinable 
algebraically. 

The  function  of  x  expressed  by  H*'a  is  not  infinite  at  the  place  z. 
Hence  we  may  define  p2  finite  constants  A^  r  by  the  equation 

A          D    fTCr>  c 

A-iir  —  UCr  O.  c      , 

where  c  is  an  arbitrary  place.  And  if,  as  in  §  132,  Ex.  in.,  we  use  the 
algebraically  determinable  quantities  given  by 

,.         _.    F,        ,  dot]       ,,          (r.   [,       ^dc{     1 
Mi>r  =  DCr  \(ci,cr) 

we  have 

Mi, 

and 


Then,  from  equation  (v),  putting  therein  cr  for  z, 

,  a      r-,x,a      r,         ^      ,          .-.dcr       -nXya      r/          x      /          ,  -,  CtCr       ^,      .         -TT-X,  a      /    ••\ 

r  =rcr  -[(Cr,x)-(cr,a}]-~=ECr  -  [(cr,#)-(cr,a)]  -^  +  2^  Ait  r  V\        (vn) 


and  thence,  since  Exc'r  a  =  I    dx  DCr  (x,  cr) 

J  a 

D*Hla  =  Der  \(x,  cr)  d4\  -  Dx  \(cr, 
at  j  )_ 


1=1 


If  in  this  equation  we  replace  as  by  z  and  i  by  r  and  then  substitute 
in  equation  (v),  we  obtain 


135]  OF   ARGUMENT  AND   PARAMETER.  185 

and  thus,  if  we  define  an,  algebraically  determinable,  integral  by  the  equation 

ST.X,  a      r,x,  a       JJ    i  r<r, 

Gz    =EZ    +  SF 


t=l 

—  \  2  (M r<  i  —  Mir)  &)r  (z)  \      (viii), 

r=l  ) 

we  have 

rxz'a  =  Gxz'a  +  2  7j'a  2  (^r)i  +  p/r  f  -  p/t- r)  &v  (z), 

i=l  r=l 

or 

•n*.  a 


\         /\  /    •  •  •  \> 

.)^^).  (vm)> 

i=l  r=l 

from  which,  by  integration  in  regard  to  z,  we  obtain  an  equation 

^.x,a        fz  ~x,  a   7.         rrX,  a        ,   r^"^.p  /  A  A      N  T7-x,  a  Trz,  e  ,.    x 

&,C  =    ^2   ^=nZ)C-^  ss  (Ar<i  +  Ai>r)Vi    v;      (ix), 
*«  f=i...p 

either  of  these  expressions  being,  by  equation  (viii),  also  equal  to 

WE,  a-        £    vj-x^l^ZtC       r,          v      ,          ,n  dc 

Pz,  c  +      F,     j(5;  -  [(a,  z)-(Ci,  c)] 


P       P  x  a,        - 

i=l  r=l 

The  equation  (ix)  shews  that  the  integral  Qx' a  is  such  that 

2t  C  %>  & 

while  every  term  of  (ix)'  is  capable  of  algebraic  determination. 

135.     From  the  equation  (ix),  when  none  of  the  places  x,  z,  d,  ...,  cp  are 
branch  places,  we  obtain 


dxdz      dz^        "^i    '    ' 
^    -^ 

i=l  r=l 

and  hence,  from  the  characteristic  property  ^— ^-  Q*'*  =  ^-^-Q^l.  we  infer 

r~P)  ^  ~i  r^  ci  ~i^ 

c)  [^'c<)-^i'  ^r^t^^'^^Jl 


f=l  r=l 


wherein   every  quantity  which   occurs  is   defined   algebraically.     The   form 
when  some  of  the  places  are  branch  places  is  obtainable  by  slight  modi- 


186  CANONICAL   INTEGRAL  [135 

fications.  This  is  then  the  general  algebraic  relation  underlying  the  funda 
mental  property  of  the  interchange  of  argument  and  parameter,  which  was 
originally  denoted,  in  this  volume,  by  the  equation  fiff  *  =  II*'  cft. 

The  relation  is  of  course  independent  of  the  places  clt  ...,  cp.  For  an  expression  in 
which  these  places  do  not  enter,  see  §  138,  Equation  17. 

The  equation  (xi)  can  be  obtained  in  an  algebraic  manner  (§  137,  Ex.  vi.).  The  method 
followed  here  gives  the  relations  connecting  the  Riemann  normal  integrals  and  the  particular 
integrals  obtained  in  Chap.  IV.,  with  the  canonical  integrals  G^'a,  Q*'". 

It  should  be  noticed,  in  equation  (xi),  that  in  the  last  summation  each  term  occurs 
twice.  By  a  slight  change  of  notation  the  factor  £  can  be  omitted. 

The  interchange  of  argument  and  parameter  was  considered  by  Abel  ;  some  of  his 
formulae,  with  references,  are  given  in  the  examples  in  §  147. 

136.     From  the  equation  (viii)'  we  have 

r*»=0«.»  +  i  |(^ii  +  ^i8)vf«. 

C8  %  i  =  l 

From  this  equation,  and  the  equation  (viii)',  we  infer  that 


8=1  S=l 

=  ty(x,  a;  z,  c1}  ...,  cp)  (xii), 

which  result  may  be  regarded  as  giving  an  expression  of  the  function 
ty  (x,  a  ;  z,  d,  ...  ,  Cp)  in  terms  of  the  integrals  G  ;  but,  written  in  the  form 

Gx'  a  =  2  a>s  (z)  Yx'  a  +  [(z,  x)  -  (z,  a)]  —  -  2  a>i  (z)  [(ci}  x)  -  (a,  a)]  -rr  , 

S  =  l  t*C          i  =  l  (Mi 

the  equation  (xii)  has  another  importance;   if  we  call  Q*'"  an  elementary 

canonical  integral  of  the  third  kind,  and  fl^  .,  =DzQ*'",  an  elementary 
canonical  integral  of  the  second  kind,  we  may  express  the  result  in  words 
thus  —  The  elementary  canonical  integral  of  the  second  kind  with  its  pole  at 
any  place  z  is  expressible  in  the  form 

Z,  ODS  (z)  Gx>  a  +  (rational  function  of  x,  z,  C1}  .  .  .  ,  cp)   -r  , 
s=i  c»  I  &t 

wherein  the  elementary  canonical  integrals  occurring,  have  their  poles  at  p 
arbitrary  independent  places  c1}  .  .  .  ,  cp. 

Further,  by  equation  (xii)  the  function  E  (x,  z),  of  §  124,  can  be  written 
in  the  form 

nx'  a  -  2  V''  c  Gx'  " 

E(x,z)  =  e^'c    -i         c'  (xiii). 


137]  AS    FUNCTION   OF   ITS   POLE.  187 

If  we  put 

K*'a=Gxz'a-[(Z,x}-(Z,a)}d^  /;"      (xiv), 

the  equation  following  equation  (xii)  gives 

p 

rrX,  a         i?  /    \    rrX,  a  /        \ 

K  '    =  2  <Oi(z)K'  (xv), 

i=i  ci 

and  therefore,  also 

Q*'°=P*'0+i    VX'aK''e  (xvi), 

Z,  C  2,  C          ^_i         i  Ct 

and 


which  is  another  form  of  equation  (xi). 
It  is  easy  to  see  that 


137.  Ex.  i.  Prove  that  the  most  general  elementary  integral  of  the  third  kind,  with 
its  infinities  at  the  places  z  and  c,  and  vanishing  at  the  place  «,  which  is  unaltered  when 
x,  z  are  interchanged  and  also  a  and  c,  is  of  the  form 


.c., 

z=l  r=l 

wherein  a,,  r  are  constants  satisfying  the  equations  0$,  r=ar,  f. 

.Er.  ii.     If  the  integral  of  Ex.  i.  be  denoted  by  ^  ",  and  Z),  $£•"  be  denoted  by  Gx;  a  , 
prove  that 


iii.    If,  in  particular,  (£'  a  be  given  by 


t,  0 


.. 

i=l  r=l 

prove  that 


This  is  the  integral,  in  regard  to  z,  of  the  coefficient  of  ^  in  the  expansion  of 
\lr(x,  a;  z,  c1}  ...,  cp),  as  a  function  of  x,  in  the  neighbourhood  of  the  place  ct  (§  132, 
Ex.  iii.). 

The  integral  ^'"  is  algebraically  simpler  than  the  integral  <^'ca,  of  this  example,  in 
that  its  calculation  does  not  require  the  determination  of  the  limits  denoted  by  M^  ;. 

Ex.  iv.     For  the  case  p  =  1,  when  the  fundamental  equation  is  of  the  form 


188  CALCULATION    OF   CANONICAL   INTEGRAL.  [137 

if  the  variables  at  the  place  ct  be  denoted  by  x  =  clyy  =  dly  the  place  not  being  a  branch 
place,  prove  that 


and  calculate  §f  '  a  ,  from  the  equation  xi,  in  the  form 

#i  C 

*  °^  *      1  "  dx    •  dz 


where,  if  y*=f(x)  =  a()xi+4alx3  +  6a2x2  +  <ia3x  +  ai,  the  symbol  f(xyz)  denotes  the  sym 
metrical  expression 

a;2  («022  +  2a12+a2)  +  2#  («1^2  +  2a2z-f  a3)  +  («2z2  +  2a32  +  a4). 
Prove  also  that  in  this  case  Mlt  1=  —f  (c1)/4/(c1). 

Calculate  the  integral  Qx"  a  when  the  place  c:  is  a  branch  place,  and  prove  that  in  that 
case  Mltlt  =limitt=0(^      -     +-),  wherein  x=cl  +  t2,  y  =  At  +  Bt3+  ...,  vanishes. 

\-£i  Ci  —  30        t  / 

Ex.  v.     For  the  case  (p  =  2)  in  which  the  fundamental  equation  is 

2 


where  f(x)  is  a  sextic  polynomial,  taking  cly  c2  to  be  the  branch  places  (cly  0),  (c2,  0),  in 
the  neighbourhood  of  which,  respectively,  x  =  c1  +  t1yy  y  =  A1tl  +  B1t13  +  ...  ,  and  o;= 
y  —  Azt2  +  B2t23+...,  prove  that 


and  infer  that 

.        .   1  dz  1 


Supposing  ^  and  z  have  general  positions,  deduce  from  equation  (ix)  that 


where  ^x2,  ^22  have  been  replaced  by  /'  (c^,  /  (ca)  respectively. 

Prove  that  this  form  leads  to 

Q*,*=  f  fsy+f^^dxdz      {*  fx^dz  M  + 

z'c      Jcja    2(j«7-z)a     y    «      JcJa2y2sL 
where,    if  /(a?)  be  a0^  +  6a1^  +  15a2^4  +  20a3^3  +  15a4A-2  +  6a5^-|-a6,  /(^,  2)   denotes   the 


expression 


and  Z,  JS/,  ^V  are  certain  constants  depending  upon  ct  and  c2. 

.Er.  vi.     Let  R  (x]  be  any  rational  function.     By  expressing  the  fact  that  the  value  of 
the  integral  $R(x)dx  taken  round  the  complete  boundary  of  the  Riemann  surface,  is  equal 


137]  UTILISATION    OF  THE   FUNCTION   \/r.  189 

to  the  sum  of  its  value  taken  round  all  the  places  of  the  surface  at  which  the  integral  is 
infinite,  we  shall  (cf.  also  p.  232)  obtain  the  theorem 


where  the  summation  extends  to  all  places  at  which  the  expansion  of  R  (x)  -7-  ,  in  terms  of 

Cbt 

[dx~\ 
R(x}~r-     _l  means  the  coefficient  of 

t~l  in  the  expansion.  If  all  the  poles  of  R  (x)  occur  for  finite  values  of  x,  this  summation 
will  contain  terms  arising  from  the  fact  that  -j-  contains  negative  powers  of  t  when  x  is 
infinite,  as  well  as  terms  arising  at  the  finite  poles  of  R  (x).  If  however  R  (x}  be  of  the 
form  U(x)  ^r  V(x\  wherein  U(x),  V(x)  are  rational  functions  of  x,  whose  poles  are  at 

finite  places  of  the  surface,  there  will  be  no  terms  arising  from  the  infinite  places  of  the 
surface. 

Now  let  £  denote  the  current  variable,  and  x,  z  denote  fixed  finite  places  :  prove,  by 
applying  the  theorem  to  the  case*  when 

&(€)  =  +(&  «;  z,cit  ...,cp)^ 
that 

D*  f  (xt  z)-Dz  +  (z,  x}  =  2  {«,  (x)  |>  (x, 

<  =  1  C{  ct 

where  ^(x,  z)  is  written  for  shortness  for  ^(x,  a;  z,  en  ...,  cp),  and  ty(x,  z)]*  denotes  the 

'* 

coefficient  of  tc.  in  the  expansion  of  ^  (x,  z},  regarded  as  a  function  of  x,  in  the  neighbour 
hood  of  the  place  c$. 

Shew,  when  all  the  involved  places  are  ordinary  places,  that  this  equation  is  the  same 
as  equation  (xii)  obtained  in  the  text. 

Prove  also  that 


Hence,  as  the  forms  a>f  (.r)  are  also  obtainable  by  expansion  of  the  function  ty  (z,  x),  eveiy 
term  on  the  right  hand  is  immediately  calculable  when  the  form  of  the  function  ^  (x,  z) 
is  known  ;  then  by  integrating  the  right  hand  in  regard  to  x  and  z  we  obtain  an  integral 
of  the  third  kind  for  which  the  property  of  the  interchange  of  argument  and  parameter 
holds.  (Cf.  Ex.  iii.  p.  180.) 

Ex.  vii.  By  comparison  of  the  two  forms  given  for  the  function  ^(x,  a;  z,  c)  (§§  126, 
131),  we  can  obtain  results  analogous  to  those  obtained  in  §§  133—136  for  the  function 
+  (x,a;  z,cl}  ...,cp). 

Putting,  as  before,  H*  a  -  I^1  °  -  [(z,  x)  -  (z,  a)]  -^  ,  and,  when  z  is  a  branch  place,  under 
standing  by  Z)*'1  H*  a  the  expression  D*z  (n*'"  -  Pj  cfl),  and,  further,  putting 


Gunther,  Crelle,  cix.  p.  206. 


190  MODIFICATION  [137 

wherein  m  is  an  arbitrary  place  and  tc  the  infinitesimal  at  the  place  c,  so  that 

^^-^B,,^^^^^:^^^ 

prove,  in  order,  the  following  equations,  which  are  numbered  as  the  corresponding  equa 
tions  in  §§  133—136  ; 

<fl=  JiW^"1^"  (ii), 


(vi), 


wherein,  when  c  is  a  branch  place,  the  first  term  of  the  right  hand  is  to  be  interpreted  as 

rff  i  px<  a  _  pc>  m\  . 
c    \    c,  m         x,  a)  ' 

also  the  equations 


,m        -     '  i       ~c        HC 
i— i 


+  I  I 

t'=l  r=l 


and  thence,  that  the  algebraically  determinable  integral 

<r^"+j,  T  ^r  [A  (M  *)-/>,  (fe,)* 


p      p  x  a 

•t=lr=l  '"        * 

is  equal  to 

I?*-|£    1    V^'\r(z}(Br,i  +  Bi,r} 
i=lr=l 

and,  finally,  that  the  integral 

_a;,  a          x,  a  P      P     ,.x,a  ,,s,m 

which,  clearly,  is  such  that  &?**&mj  can  be  algebraically  defined  by  the  equation 


x,  a       J-.X,  a 


(     i         *r  r          i       '   **rii  (lx)'- 

i  r 

Further  shew  that  the  function  ^  (x,  a  ;  z,  c)  can  be  written  in  the  form 

>//•  (.r,  a  ;  z,  c)  =  G*' '  -   2  «»g  (z)  D*      ff^'  "  (xii). 


137]  OF  THE  RESULTS  OBTAINED.  191 

The  algebraical  formula  expressing  the  property  of  interchange  of  argument  and  parameter 
is  to  be  obtained  from  the  equation 

r>    n    f\x<  a        r»    //         \  °^\          2         /    \    rfi'1   (  r»   //        \  d>Z\        -    /.        .  dc 

DXD,  ^  m=D.         z)         +       „,  (x)  Zy        A        c)        -  A    (',  *) 


+  \  22  [a>i  (a?)  «,.  (z)  -  <ar  (a?)  o^  (z)]  JT,  ,  r  (x). 

Lastly,  if  Lk(z)  denote  the  coefficient  of  tk/\k  (k  positive)  in  the  expansion  of  the  function 
•^  (x,  a  ;  z,  c)  as  a  function  of  x  in  the  neighbourhood  of  the  place  c,  so  that  (Ex.  iv.  §  132) 


where  Pt,  k  denotes  a  certain  constant  such  that  P*,^  is  Ni)r,  prove,  by  equating  to  zero 
the  sum  of  the  coefficients  of  the  first  negative  powers  of  the  infinitesimals  in  the  expan 
sions  of  the  function  of  £,  >//•  (£,  a  ;  z,  c)  D%  ^  (£,  a  ;  x,  c),  at  all  places  where  negative 
powers  occur,  that 

p 
Dx  ^  (x,  a  ;  z,c)-D^(z,a;  a?,  c)  =  2  [«<  (a?)  Lk.  (z)  -  ^  (z)  Lk.  (x)]  (A), 

wherein,  on  the  right,  only  functions  Lk(z)  occur  for  which  k  is  one  of  the  p  numbers 
^n  ^2>  •••»  kp)  and  that 

thus  an  elementary  integral  of  the  third  kind,  permitting  interchange  of  argument  and 
parameter,  is  obtained  immediately  from  the  function  ty(x,  a;  z,  c)  by  integrating  the 
right  hand  of  equation  (B)  in  regard  to  x  and  z. 

Prove  also,  that  if 

we  have  the  formulae 

p 

•]lfi-lK^a  (XV) 


^r.  viii.     To  calculate  the  integral  Q*'^  for  the  case  (p  =  2)  where  the  fundamental 
equation  is 

2/2=/H, 
wherein/^)  is  a  sextic  polynomial  divisible  by  x-c,  which  is  expansible  in  the  form 

•f(x}  =  A*(x-c}  +  Q(x-c?  +  R(x-cf  +  ..., 
we  may  use  the  equation  (xi)  of  Ex.  vii.     When  x,  z  are  near  the  place  c,  putting 


prove  that 


D'  \*  ^  ^~t)  ~  DX    ^  x^  Jt    =  A*  (**  ~  ^2)  +  cubes  and  hiSher  powers  of  «,  and  «2, 


192  GENERAL   STATEMENT  [137 

and  thence  (see  Ex.  ii.  §  132)  that 

v    r     i  \      i  \         i  \      ,  \-<    R(x  —  z)dxdz 

Kn  [«!  (*)  0>2  (Z)  -  o>2  (X)  <*!  (Z)]  =       V^     >   -^  jt  . 

Also,  when  z  is  not  a  branch  place,  if  Cj  be  a  place  near  to  c,  and  the  expansion  of  the 
function  ^-  (z,  c^-^fa,  2)  -^  in  powers  of  the  infinitesimal  at  c,  contain  the  terms 
M+  .  +  JVP  +  ...  ,  so  that 


prove  that 


substituting  these  results  in  the  formula  (xi)  of  Ex.  vii.,  prove  that 


_ 

z)z      240 

where  /(#,  0)  has  the  same  signification  as  in  Example  v.     The  part  within  the  brackets 
{     }  is  of  the  form  ys^'2ai,r<ai(x)a>r(z),  where  ai,r  =  ar,i. 

Obtain  the  same  result  by  the  formula  (B)  of  Ex.  vii.,  using  the  form  of  ^  (#,  a  ;  z,  c) 
found  in  Ex.  ii.  §  132. 

138.  The  formulae  in  §§  133  —  136  enable  us  to  express  the  form  of  a 
canonical  integral  of  the  third  kind,  in  the  most  general  case  ;  and  to 
calculate  the  integral  for  any  fundamental  algebraic  equation,  when  the 
integral  functions  are  known.  But  they  have  the  disadvantage  of  presenting 
the  result  in  a  form  in  which  there  enter  p  arbitrary  places  c1}  ...  ,  cp.  We 
proceed  now  to  shew  how  to  formulate  the  theory  in  a  more  general  way  ; 
though  the  results  obtained  are  not  so  explicit  as  those  previously  given, 
they  are  in  some  cases  more  suitable  for  purposes  of  calculation. 

Let  u*'  a,  ...  ,  ux'a  denote  any  p  linearly  independent  integrals  of  the  first 
kind  ;  denote  Dxuf  °  by  /^  (#).  Let  the  matrix  whose  (i,  j)th  element  is 
Hj  (Ci)  be  denoted  by  p,  c1}  ...,  cp  being  the  places  used  (§  121)  to  define 
the  quantities  wl  (x),  ...,  wp(x).  Let  i/ij  denote  the  minor  of  the  (i,j)ih 
element  in  the  determinant  of  the  matrix  /A,  divided  Jby  the  determinant 
of  /*;  so  that  the  matrix  inverse  *  to  p  is  that  whose  (i,  j)ih  element  is  Vjt{. 
Then  we  clearly  have 

o>i  0)  =  Vi,  i  /*i  O)  +  ......  +  vi>PnP(x)  (i=l,  2,  ...,  p). 


*  Since  «*'",  ...,  «*'"   are  linearly  independent,  and  the  places  clt  ...,cp  are   independent 
(see  §§  23,  121),  the  matrix  /j.-1  can  always  be  formed. 


138]  FOR   FUNDAMENTAL    INTEGRALS   OF   THE    SECOND   KIND.  193 

Let  a  denote    any  symmetrical   matrix  of  p2  quantities,  a,-j,  in  which 
aiij  =  Uji  i.     Then  we  define  p  quantities  by  the  p  equations 


and  call  them  fundamental  integrals  of  the  second  kind  associated  with  the 
integrals  u*'a,  ...  ,  u^".  For  instance  when  m  (x)  =  &>;  (x\  Vjj  =  Q  unless 
i=j,  in  which  case  *>,-,;=!.  Thus  by  taking  ait  ;  =  £  (Ait  }  +  A  jti),  the 
integrals  K*'a,  ...,  Kx'a  (p.  187.  xiv.)  are  a  fundamental  system  associated 
with  the  set  V*'a,  ...,  V*'a. 

It  will  be  convenient  in  what  follows  to  employ  the  notation  of  matrices 
to  express  the  determinant  relations  of  which  we  avail  ourselves  *.  We  shall 
therefore  write  the  definition  given  above  in  the  form 

L*'*=vH*'a-2au*-", 

wherein  Lx'a  stands  for  the  row  of  p  quantities  Lx'a,  ...  ,  Lx'a,  H'r'a  stands 
for  the  row  of  p  quantities  Hx'a,  ...  ,  Hx'a,  and  v  denotes  the  matrix  obtained 

by  changing  the  rows  of  v  into  its  columns,  and  is  in  fact  equal  to  the 
matrix  denoted  by  /z"1,  so  that  we  may  also  write 

Lx'  a  =  ^Hx'  a 
where  (§137) 

TT-t,  a  jr  X.(t.tf*/t  t          ..    TT%>  ffl 

Hci      =  Kc-      +  2    S  (Ar>  i  +  Ai}  r)  Vr     . 


t 

r=l 


Explicit  forms  of  the  integrals  K*'a  have  been  given  (§§  134,  136). 
Then,  from  the  equations  defining  the  integrals  Lx.' a,  we  have 

2  m  (z)  L?  a  =  2  Hxc'.  a  2  i>j, ,:  &  (z)  -  2  2    2  ar> ,  M *'  "  ps  (z\ 

i=s\  *  —  i  *•»'  —  i  -n  —  i    « _  i 


,   x  TJ,  n  , 

=  Z  &>j  (3rJ  ±T;     -  2  2    2  ar,  g  ur    p*  (z\ 

j=l  r=l   ,i=l 

UX'a        O    <£      4>  a;'a         /    \ 

=  •"«     —22    2  ar) ,  wr     ^,  (2)  ; 

r=l  s=l 

and  this  is  an  important  result.  For,  putting  for  z  in  turn  any  p  independent 
places,  the  p  functions  Lx'a  are  determined  by  this  equation.  Thus  the 
functions  L^  a,  ...  t  Lx' a  do  not  depend  upon  the  places  c1 ,  c2,  . . . ,  cp. 

See  for  instance  Cayley,  Collected  Works,  vol.  ii.  p.  475,  and  the  Appendix  II.  to  the  present 
volume,  where  other  references  are  given. 

B-  13 


194  CANONICAL   INTEGRAL   OF   THE  THIRD   KIND.  [138 

Also,  from  this  equation  we  infer 
~    |~         .  dz~\       j^   [,       v<fe|       n  ITZ>C      n  TTx>a 

x  (*'  X^~dt\~   *  I      ^  «8j      *  "  ~ 

=  I  [^  (x)  D,i?  "  -  ^-  (5)  0,1?  a]      (17), 

1=1 

c  being  any  arbitrary  place.     Now  it  is  immediately  seen  that  if  -Ri(#),  ...  , 
Rp  (x)  be  any  rational  functions  of  x  such  that 


then  Ri  (x)  can  only  be  a  form  of  DXL?  a,  obtained  from  DXL*'  a  by  altering 
the  values  of  the  constant  elements  of  the  symmetrical  matrix  a.  Hence 
the  equation  (17)  furnishes  a  method  of  calculating  the  integrals  Lf",  when 
ever  it  is  possible  to  put  the  left-hand  side  into  the  form  of  the  right-hand 
side. 

The  equation  (17)  shews  that  the  expression 

r>  //       \  da>\  ,    v        /  \  n  r*-  c 
Dz  ((x,z)  -T.    +  2  fit  (x)  DzLi    , 
\  at/      i=i 

is  unaltered  by  the  interchange  of  x  and  z.  This  expression  is  also 
equal  to 

D,  ((*,  z)  tg)  +  DZHX'C-  2  I    iar^iir  (*)  ^  (z} 
\          at/  r=\  s=i 

and,  -therefore,  to 


Hence,  the  formula  (§  134,  ix.) 


z>  c 


,.x,  a         r>x,  a  ,       x,arz,c        -f-fX,  a       o  .        nl 

Rg,c,=Pz,c  +  ^  ut    Li     =HZ|C  -2  Z    i  ar>gw 

i=l  r=l  s=l 

_  a;  «  £,      Ji    /  \   TT  z.  a  TT-Z>  c        r»    vr>      ^  je,  a    z,  c 

=  Qz  c    +  k    2      2   (4r,  ,  +  -4,,  r)  7r'     F,       -  2    2      S   ar>  sUr      Us 
r=l   s=l  r=l   s=l 

gives  us  a  form  of  canonical  integral  of  the  third  kind  not  depending  upon 
the  places  cl}  ...  ,  cpt  and  immediately  calculable  when  the   forms   of  the 

functions  Li     are  found. 


The  formula 


If  "  =  [(*,  as)  -  (z,  a)]      +  2  fit  (z)  L*'a  +  2  a,,  .  if  *  p.  (z) 

Clt       ^=i  r=\  s=l 

serves  to  express  any  integral  of  the  second  kind  in  terms  of  the  integrals 
LI  .....  Lv 


139]  EXAMPLE   OF   HYPERELLIPTIC   CASE.  195 


Ex.  i.     For  the  surface  y2  =/(#)»  where  /(#)  is  a  rational  polynomial  of  order  2p  +  2, 
the  function 

^L_      d  (       9       N       .    *    f       f(&  2/tf) 

' 


wherein  s2=f(z),  »;2  =/(£),  is  a  rational  function  of  £  (without  17).     Prove  by  applying  the 
theorem,  2  fj2(f)  ^1      =0,  (Ex.  vi,  §  137)  that 


where  i;  k'  represent  in  turn  every  pair  of  unequal  numbers  from  0,  1,  2,  ...,  2p,  whose 
sum  is  not  greater  than  2p,  V  being  greater  than  k,  and  the  coefficients  X  are  given  by  the 
fact  that 


Hence,  a  set  of  integrals  of  the  second  kind  associated  with  the  integrals  of  the  first  kind 

/Q3C         i     OOQf\K  t     • 

T7  '     /    "17" »    '     / 
a,  !/        J  a    3  J  a 


y 

is  given  by 


x  a         fx  dx  fc  =  2p+l-»' 

Lfa=  2         Xt  +  l  +  f(*+l-i)«*f 

J  a  *</          k  =  i 

and  a  canonical  integral  of  the  third  kind  is  given  by 


This  is  equal  to 

p+i 


aJcZsfy  (X-ZY 

which  is  clearly  symmetric  in  x  and  z. 

O  o 

The  value  of  5-  (z,  x}  —  ^-  (x,  z)  used  in  this  example  is  given  by  Abel,  (Euvres  Completes 
(Christiania,  1881),  Vol.  i.  p.  49. 

Ex.   ii.     Shew   in   Ex.    i.,    for    »=1,    that    the    integral    associated   with     I    —    is 

J*  y 

fx  X  x  -4-  2X  x~ 

—  dx ;  and  express  these  in  the  notation  of  Weierstrass's  elliptic  functions 
J  a       *y 

when  the  fundamental  equation  is  y2=4.r3— gtfc-gy 

139.     Suppose  now  that  the  integrals  u*'n,  ...,u*'"  are  connected  with 
the  normal  integrals  Vi'a,  ...  ,  v*'a  by  means  of  the  equations 

which,  since  H4-  (x)  =  ZirHh*' n,  are  equivalent  to 


x,a 
Ur        = 


Then  the  periods  of  the  integral  «*'  a,  at  the  first  p  period  loops,  form  the 
rth  row  of  a  matrix,  2\,  and  the  periods  of  the  integral  ?^'  "  at  the  second 

13—2 


196  PERIODS    OF    FUNDAMENTAL    INTEGRALS.  [139 

p  period  loops  form  the  rib.  row  of  a  matrix  2Xr  ;  we  shall  write  &>  =  X  and 
W'  =  XT,  so  that  (t}jj=\ij.  The  two  suffixes  of  the  quantities  ta^j  will 
prevent  confusion  between  them  and  the  differential  coefficients  o>i  (x). 

Let  the  periods  of  L^  at  thejth  period  loops  of  the  first  and  second  kind 
be  denoted  by  —  2^  j  and  —  Zrj'^  j  respectively.  The  matrix  whose  t'th  row 
consists  of  the  quantities  77^  i  ,  ...  ,  77^  p  will  be  denoted  by  77  ;  similarly  the 
matrix  of  the  quantities  77'.^  will  be  denoted  by  77'.  The  matrix  of  the 

periods  of  the  integrals  H^a,  ...  ,  H^a  at  the  first  period  loops  is  zero;  the 
(i,  j)th  element  of  the  matrix  at  the  second  period  loops  is  the  jth  period  of 
HC.'  a,  namely  ft,-  (Cj).  We  shall  denote  this  matrix  by  A. 

By  the  definitions  of  the  integrals  Lj'a  we  therefore  have 


and  all  these  equations  are  contained  in  the  equations 

77  =  2a<u, 

77'  =  2am'  -  %v&  =  2aw'  -  ^/t-1  A. 
Now  from  the  equations  connecting  f*,r  (a)  and  fi,  (as),  we  obtain 

TTt'/i,.  (Cj)  =  X,.,  !  f^!  (C»)  +  ......  +  \r,  p  Op  (Ci), 

wherein  /j,r  (d)  is  the  (i,  r)ih  element  of  the  matrix  /A,  and  the  right  hand  is 
the  (i,  r)th  element  of  the  matrix  AX  ;  hence  we  may  put 

Trt'/i.  =  AX. 
If  then  we  denote  the  matrix  ^/*-1A  by  h,  we  have 

2AXA  =  27ri/j.h  =  Tn'A  =  Avri, 
and  infer  that  2XA  =  7rt,  and  thence  that  2/iX  =  iri.     Thus  2hu>=Tri,  2ha)'=7rir. 

A  i          ,  i         •     ,  ••          *,  a  x,  a  x,  a  x,  a  ,11  i 

Also   tne   integrals   u-i    ,  ...  ,  up    ,  ...  ,  vi    ,  ...  ,  vp      are   connected    by   the 


equation  AM*-  a  =  2h\vx>  a  =  Triif-  a. 
140.     The  four  equations 

2hw  =  iri,     2ha>'  =  TTIT,     77  =  2a&>,     77'  =  2aay'  —  h  (A) 

will  prove  to  be  of  fundamental  importance  in  the  theory  of  the  theta 
functions.  They  express  the  periods  77,  77'  independently  of  the  places 
d,  ...  ,  cp,  used  in  defining  L*'a. 

If  beside  the  symmetrical  matrix  T,  and  the  arbitrary  symmetrical  matrix 
a,  we    suppose    the    matrix   h,   which    is    in    general    unsymmetrical,  to    be 


141]  RELATIONS   CONNECTING   THE    PERIODS.  197 

arbitrarily  given,  the  integrals  Ui'  ,  ...  ,  up'  being  then  determined  by  the 
equation  hu*< a  =  7rvix>  a,  the  first  equation,  2Ao>  =  TTI,  gives  rise  to  p2  equations 
whereby  the  p*  quantities  wit  j  are  to  be  found,  and  similarly  the  other 
equations  give  rise  each  to  p2  equations  determining  respectively  the  quantities 
o>'i,j,  rii,j,  rfij-  But,  thereby,  the  4p2  quantities  thus  involved  are  deter 
mined  in  terms  of  less  than  4>p2  given  quantities.  For  the  symmetrical 
matrices  a,  T  involve  each  only  ^p(p  +  I)  quantities,  and  the  number  of 
given  quantities  is  thus  only  p  (p  +  1)  +p2.  There  are  therefore,  presumably, 

4p2  —  [pz  +p  (p  +  1)],    =  2p*  —p, 

relations  connecting  the  4p2  quantities  (0,-j,  co'ij,  77^-,  ?/,;( j\  we  can  in  fact 
express  these  relations  in  various  forms. 

One  of  these  forms  is 

corj  =  770),     W'TJ'  =  rj'o)',     rjta'  —  wv)  =  ^TTI  =  rn'ij  —  TJ'CO,  (B) 

of  which,  for  instance,  the  first  equation  is  equivalent  to  the  %p(p  —  1) 
equations 

(wr,  i  IJr,  j  —  tjr,  i  &>  r,  j)  =  0, 


r=l 


in  which  i  =  1,  2,  . .. , p,  j  =  1,  2, ... , p,  and  i  is  not  equal  to  j.  The  second 
equation  is  similarly  equivalent  to  ^p  (p  —  1)  equations,  and  the  third  to  p- 
equations.  The  total  number  of  relations  thus  obtained  is  therefore  the 
right  number  p-  +p  (p  —  1),  In  this  form  the  equations  are  known  as 
Weierstrass's  equations. 

Another  form  in  which  the  2p-  —  p  relations  can  be  expressed  is 

wo)' =&)'&>,     7777'  =  r}'rj,     0/77  —  0)77'  =  ^7ri  =  ijm'  —  t]'(a  (C) 

These  equations  are  distinguished  from  the  equations  (A)  as  Riemanu's 
equations. 

141.  The  equations  (B)  and  (C)  are  entirely  equivalent;  either  set  can  be  deduced 
from  the  equations  (A)  or  from  the  other  set.  A  natural  way  of  obtaining  the  set  (B)  is 
to  use  the  equation  (17).  A  natural  way  of  obtaining  the  set  (C)  is  to  make  use  of  the 
Riemaun  method  of  contour  integration. 

The  equations  (A)  give,  recalling  that  a  =  a,  a>'  =  a>7-,  f  =  r, 

o)ij  =  2wa&)  ,=/3,  say,  a  symmetrical  matrix, 
<o»j'  =  2u>r/o/  —  w/i  = 

Hence  ^ft)'  =  ^wr==^r=^T 

and  because  w'  =  rw, 

<5  V  =  TVTJ'  =  r/3r  — 
and  thus,  as  r^r  =  T^T,  \ve  have 


198  PROOFS   OF   THE    RELATIONS  [141 

which  are  the  equations  (B).     And  it  should  be  noticed  that  these  results  are  all  derived 
from  the  three  a>'  =  «r,  urj  =/3,  &>;/=/3r  —  ^TTJ,  assuming  only  that  ft  and  T  are  symmetrical. 

From  the  equations  (B),  putting  »»;=£,   uTj'=y,  so  that  $  and  y  are  symmetrical 
matrices,  we  obtain* 

?;  =  («5)~1jS,  ^'=y(<o')~1,  and  thence  ^'(w)"1^  —  y(u)~1u  =  $ni, 
Henue,  if  <O~IU>'  =  K,  HO  that  O>K  =  O>',  O>'  =  KO>,  «'  («)  ~  1  —  *,  and  >c~1  =  (a>')~1t<),  we  have 

K/3  —  yK~1  =  ^7rl,   or  K/3K  —  y  =  ^7ri»c, 
and  therefore,  as  the  matrices  K/SK  and  y  are  symmetrical,  so  also  is  the  matrix  <c  ;  and  thus 

a>  ~  l  w'  =  a>'  (o>)  ~  *,  and  therefore  ow'  =  <w'<o, 
which  is  one  of  the  equations  (C). 
Further 

Wlf  =  tyw'  —  ^TTt  =  IJWK  —  ^Trt  =  /3K  —  JfTTZ, 

and  therefore  q'w  =  icji  -  £TTI  =  K/3  -  %iri\ 

leading  to  w^'w  =  £*£  -  ^Trtft 

and  the  right  hand  is  a  symmetrical  matrix,  and  therefore  equal  to  w^'/jtu  ;   thus  also 

W'|"9'f> 

which  is  the  second  of  the  equations  (C). 

r  inally  (o>  rj  —  w^')  w  =  a)'jja)  —  <a((o'r]  —  ^TTI)  —  eo'tbjj 

=  ^-TT  la), 
and  thus 

to'^  -<»^'  =  ^7ri,  =  ,  therefore,  r)H'  —  rj'oi, 
which  is  the  third  of  equations  (C). 

We  have  deduced  both  the  equations  (B)  and  (C)  from  the  equations  (A).     A  similar 
method  can  be  used  to  deduce  the  equations  (B)  from  the  equations  (C). 

Other  methods  of  obtaining  the  equations  (B)  and  (C)  are  explained  in  the  Examples 
which  follow  (§  142,  Exx.  ii—  v). 

142.     Ex.  i.     Shew  that  the^>  integrals  given  by  the  equation 

.x,  a      .         fjx,a.          ..         Tix,a 
Ai       =tl>iHc,     +---  +  tPJi-acp    > 

where  titj  is  the  minor  of  Q,-^)  in  the  determinant  of  the  matrix  A  (§  139),  divided  by  the 
determinant  of  A,  namely  by  the  equation 

A*.«  =  A  -!#*'", 

are  a  set  of  fundamental  integrals  of  the  second  kind  associated  with  the  set  of  integrals 
of  the  first  kind  2nivi'  a,  ...  ,  ^irivf  a,  and  are  such  that 

' 


=  1 


. 

^UWB.**')*  1  (ai(x)D,Kl°  -<*>(,)  DtK*'* 

/      i=l  \  J* 


i=\ 


*  The  determinant  of  the  matrix  w,  =  X,  cannot  vanish,  because  u'",    ..,?/'"  are  linearly 

i  /* 

independent.  The  determinant  of  the  matrix  T  does  not  vanish,  since  otherwise  we  could  deter 
mine  an  integral  of  the  first  kind  with  no  periods  at  the  period  loops  of  the  second  kind 
(cf.  Forsyth,  Theory  of  Functions,  §  231,  p.  440). 


142]  CONNECTING   THE   PERIODS.  199 

Prove  that  the  function  A*' a  has  only  one  period,  namely  at  the  ith  period  loop  of  the 
second  kind,  and  that  this  period  is  equal  to  1.  For  the  sets 

_     .  x,  a  _     .  x,  a        .x,a  .x,a 

2mv:     ,  ...,  2mvp'    ,   A,'    ,  ...,  A;)     , 

we  have  in  fact  <a=iri,  <a'  =  Trir,  f?  =  0,  rj'=—^. 

Shew  that  these  values  satisfy  the  equations  (B)  and  (C). 

Ex.  ii.     From  Ex.  i.  we  deduce 

a     •  £•   /  '-'•  a  .  *•  c        z,cx,a.         &    ,    x,  a  rz,  c         x,c  Tx,  a. 
fcrt  1  (»<       Aj      -V.      A«     )=    I  («!      Lt     -Ut     Li     ). 
i=\  i=\ 

Hence,  supposing  x  and  z  separately  to  pass,  on  the  dissected  Riemann  surface,  respec 
tively  from  one  side  to  the  other*  of  the  rth  period  loop  of  the  first  kind,  and  from  one 
side  to  the  other  of  the  sth  period  loop  of  the  first  kind,  we  obtain,  for  the  increment  of 
the  right-hand  side 

p 

-4  2  (&>i,ri7t,«-»7i,r<»t>«)> 
i=i 

which  is  the  (r,  s)th  element  of  the  matrix  —  4  (GM;  —  i;a>).  For  the  functions  on  the  left- 
hand  side  the  matrix  wrj  —  rjm  vanishes  (Ex.  i.).  Hence  the  same  is  true  for  those  on  the 
right  hand. 

Supposing  x  to  pass  from  one  side  to  the  other  of  the  rth  period  loops  of  the  first  kind, 
and  z  from  one  side  to  the  other  of  the  sth  period  loop  of  the  second  kind,  we  similarly 
prove  that  5»;'  —  ij<o'  has  the  same  value  for  the  functions  on  the  two  sides  of  the  equation, 
and  therefore,  as  we  see  by  considering  the  functions  on  the  left  hand,  has  the  value  —  fari. 

While,  if  both  x  and  z  pass  from  one  side  to  the  other  of  period  loops  of  the  second  kind 
we  are  able  to  infer  u'r)'  =  ^'<a'. 

We  thus  obtain  Weierstrass's  equations  (B). 

Ex.  iii.  If  Uf  ",...,  U*'  a  be  any  integrals,  the  periods  of  Uf  a  at  thejth  period  loops 
of  the  first  and  second  kind  be  respectively  &„-,  f'f)>,  and  the  matrices  of  these  elements 
be  respectively  denoted  by  £,  f ' ;  and  W*'a  ,  ...,  W%  a  be  other  integrals  for  which  the 

corresponding  matrices  are  £  and  f ,  prove  that  the  integral  lU^d  W*' a,  taken  positively 
round  all  the  period-loop-pairs  has  the  value 


which  is  the  (i,j)th  element  of  the  matrix  &'-  f'f 

Ex.  iv.     If  #(  (#)  denote  the  rational  function  of  x  given  by 

p  (fa 

Ri  (x)=    2    vr , »  [(cr ,  a?) -  (cr,  a)]  -^ , 
r=l 

the  function  Zj**+jg|(*)  is  infinite  only  at  c1?  ...,cp,  and  has   the  same  periods 
Zr*'  °  ,     Denote  this  function  by  Ya>  a  . 

To  that  side  for  which  the  periods  count  positively  (see  the  diagram,  §  18). 


200  SERIES   REPRESENTING   AN    UNIFORM   FUNCTION  [142 

Prove  that  if  the  expansion  of  the  integral  Y*'  "  in  the  neighbourhood  of  the  place  ct 
be  written  in  the  form 


then 

</i,i  =  "i,i(^ 

where  Ai,  s,  Mit  t  are  as  denned  in  §  134,  and  are  such  that  Aitt  +  Mit  t=Atti+Mtt  t. 

Hence  shew  that  the  sum  of  the  values  of  the  integral  J  r*'"  dYf*  taken  round  all 
the  places  cx  ,  .  .  .  ,  cv  is  zero. 

Ex.  v.     Infer  from  Exs.  iii.  and  iv.,  by  taking 

/    \       71^,0,      ,.x.  a       iJT  x,  a    ,-\     , 

(a)      U.      =u.'    =W.'   ,  that  cow  =  «  w, 

fo\      frx,a-yx,a      firx,a         x,  a     ,-,      ,       _.         .          , 

(P)     U.      =  Y.     ,    W.      =u.'  ,  that  riS'-T)'5  =  $iri, 

/    \       Trx,a       -irx,  a       Tirana   fUr.4-   v~'        /- 

(y)     ™    =Y.         W.'     that  777  =J?'7. 
These  are  Riemann's  equations. 

Ex.  vi.  If  instead  of  the  places  cl}  ...,  cp  and  the  matrix  p.,  we  use  a  matrix  depending 
only  on  one  place  c,  the  t'th  row  being  formed  with  the  elements  D^~  ^  (c),  ...  ,  ZT'  ^,(c), 
we  can  similarly  obtain  a  set  Lf  ",...,  ^'  a  associated  with  the  set  «*'  "  ,  ...  ,  u*'  a  . 

Shew  that  the  periods  of  Lx'a  ,  ...  ,  Zf'  a  thus  determined  are  independent  of  the  posi 
tion  of  the  place  c. 

Ex.  vii.  If  the  differential  coefficients  ^  O),  ...  ,  /*,,O),  be  those  derived  from  a  set  of 
p  independent  places  bly  b.^,  ...  ,  bp,  just  as  ^  (x),  ...  ,  <ov(x)  are  derived  from  c^,  ...  ,  cp,  so 
that  /*i(6i)  =  l,  /ui(6,.)  =  0,  prove  that  i/,.,  i  =  co,.  (6f)  and  that 


143.  We  conclude  this  chapter  with  some  applications*  of  the  functions 
•^r(x,  a;  z,  c),  E(x,  z)  to  the  expression  of  functions  which  are  single-valued 
on  the  (undissected)  Riemann  surface.  Such  functions  include,  but  are 
more  general  than,  rational  functions,  in  that  they  may  possess  essential 
singularities. 

Consider  first  a  single-valued  function  which  is  infinite  only  at  one  place  ; 
denote  the  place  by  m,  and  the  function  by  F  (x). 

dz 
Since  -\|r  (x,  a  ;  z,  c)    -^  is  a  rational  function  of  z,  the  integral 

/  CLt 

\F(z}\^r  (x,  a  •  z,  c)  I  -j-    dz,  or  \F(z)-ty  (x,  a  ;  z,  c)  dtz, 

taken  round  the  edges  of  the  period-pair-loops,  has  zero  for  its  value.     But 
this  integral  is  also  equal  to  the  sum  of  its  values  taken  round  the  place  m, 

*  Appell,  Acta  Math.  i.  pp.  109,  132  (1882),  Giinther,  Crelle  cix.  p.  199  (  1892). 


143]  NEAR   AN    ESSENTIAL   SINGULARITY.  201 

where  F(z}  is  infinite,  and  the  places  x  and  a  at  which  -ty  (x,  a;   z,  c)  is 
infinite. 

fJz 

Now,  when  z  is  in  the  neighbourhood  of  the  place  m,  since  ilr  (#,  a  ;  z,  c)  I  -=- 

/  at 

is  a  rational  function  of  z,  we  can  put 

00        jf 

^(x,a;  z,c)-  2  J?  Dr  ty(x,a\  m,  c), 

r-O  lr 

where  tm  is  the  infinitesimal  at  the  place  m. 

Thus  the  integral  I  F(z)ty(x,  a  ;  z,  c)dtz,  taken  round  the  place  m,  gives 

oo      Ar 

Zjri  2   -i-f  Drm  -f  O,  a  ;  m,  c\ 

?'  =  0     |_ 

1     f 
where  J.r  is  the   value   of  the  integral      —  .  \trmF(z}dtz  taken  round  the 

place  m. 

When  2  is  in  the  neighbourhood  of  the  place  x,  i/r  (x,  a;  z,c)  is  infinite 

like  tx  ,  tx  being  the  infinitesimal  at  the  place  as,  and  therefore,  taken  round 
the  place  x,  the  integral 

J  F(x)^f  (x,  a;  zt  c)dtz 
gives 


Similarly  round  the  place  a,  the  integral  gives  —  27riF(a). 
Hence  the  function  F(x)  can  be  expressed  in  the  form 

F(x)  =  ^(a)  -  J^  T^'  Drm  ^  (x,  a  ;  m,  c), 

the  places  a  and  c  being  arbitrary  (but  not  in   the   neighbourhood  of  the 
place  m). 


For  example,  when  p  =  0,  ^  (x  a;  z,  c)=  -  (  —  ---  L  \ 

\&  —  z     a-zj 


an(J 


wherein 

1     /" 
^r  =  2nri  /  (2  —  m)r  f(z}  dz,  the  integral  being  taken  round  the  place  m. 

A  similar  result  can  be  obtained  for  the  case  of  a  single  valued  function  with  only  a 
finite  number  of  essential  singularities.  When  one  of  these  singularities  is  only  a  pole, 
say  of  order  M,  the  integral  /£  F(z)  dz,  taken  round  this  pole,  will  vanish  when  r5M,  and 
the  corresponding  series  of  functions  Dr  ^  (.>-,  a  •  m,  c)  will  terminate. 


202  MITTAG  LEFFLER'S  THEOREM  [144 

144.  We  can  also  obtain  a  generalization  of  Mittag  Leffler's  Theorem. 
If  c1;  c2,  ...  be  a  series  of  distinct  places,  of  infinite  number,  which  converge* 
to  one  place  c,  and  f±  (x),  f2  (a), ...  be  a  corresponding  series  of  rational 
functions,  of  vnuca/V(0)  is  infinite  only  at  the  place  Cj,  then  we  can  find  a 
single  valued  function  F  (x),  with  one  essential  singularity  (at  the  place  c), 
which  is  otherwise  infinite  only  at  the  places  cit  C2>  ...,  and  in  such  a  way 
that  the  difference  F(x)  —J\  (x)  is  finite  in  the  neighbourhood  of  the  place  Cf. 

Since  fi(x)  is  a  rational  function,  infinite  only  at  the  place  C{,  and 
•fy(x,a;  x,  c)  does  not  become  infinite  when  z  comes  to  c,  we  can  put 

ft  («)  =/*  (a)  ~  2    -f  Dl  +  (x,  a  •  a,  c),  (A) 

r=0    ;_L 

wherein  a  is  an  arbitrary  place  not  in  the  neighbourhood  of  any  of  the 
places  Cj,  c2, ...,  c,  and  \  is  a  finite  positive  integer,  and  Ar  a  constant. 

Also,  when  z  is  sufficiently  near  to  c,  and  x  is  not  near  to  c,  we  can  put 

«,      tk 

TJT  (as,  a  ;  z,  c)  =  2     «  [D^  ^r  (ar,  a  ;  s,  c)]z=c, 

fc=0    \K 

wherein  tc  is  the  infinitesimal  at  the  place  c.     Thus  also,  when  z  is  near  to  c, 
17  ^  (x,  a  •  z,  c)  m  |o  tkc  Rk  (as),  (B), 

wherein  Rk  (x}  is  a  rational  function,  which  is  only  infinite  at  the  place  c. 
There  are  p  values  of  k  which  do  not  enter  on  the  right  hand ;  for  it  can 
easily  be  seen  that  if  &!,...,  kp  denote  the  orders  of  non-existent  rational 
functions  infinite  only  at  the  place  c,  each  of  the  functions 

[D*'->O,  a;  z,  cXU, ,  [JOf-1  ^ (*,  a  ;  z,  c],=c 

vanishes  identically.  Let  the  neighbourhood  of  the  place  c,  within  which  z 
must  lie  in  order  that  the  expansions  (B)  may  be  valid,  be  denoted  by  M. 

Of  the  places  Cj ,  c2 ,  . . . ,  an  infinite  number  will  be  within  the  region  M ; 
let  these  be  the  places  cs+l,  cs+.2,  ...:  then  s  will  be  finite  and,  when  i  >  s, 
we  have 

oo        £ 

&'.  ty  (*',  a;  Ci,c)=  S   <<  ^  *  (as), 

k=0 

wherein  ti  is  the  value  of  tc,  in  the  equation  (B),  when  z  is  at  c;.  Hence  also, 
from  the  equation  (A),  wherein  there  are  only  a  finite  number  of  terms  on 
the  right  hand,  we  can  put 

fi(x}-fi(a)=  I  £$,*(*),  (C), 

k  =  Q 

wherein  S^k  is  a  rational  function,  i  >  s,  and  a;  is  not  near  to  the  place  c. 

*  so  that  c  is  what  we  may  call  ike  focus  of  the  series  c1}  c3,  ...  (Haufungsstelle). 


144]  FOR   ANY    UNIFORM    FUNCTION.  203 

It  is  the  equation  (C)  which  is  the  purpose  of  the  utilisation  of  the 
function  ty  (x,  a  ;  z,  c)  in  the  investigation.  The  functions  S^k  (#)  will  be 
infinite  only  at  the  place  c.  The  series  (C)  are  valid  so  long  as  x  is  outside 
a  certain  neighbourhood  of  c.  We  may  call  this  the  region  M'. 

Let  now  eg+i,  eg+2,  ...  be  any  infinite  series  of  real  positive  quantities,  such 
that  the  series 

C8+l  H~  e«+2  +  €S+3  +   •  •  • 

is  convergent  ;  let  ^  be  the  smallest  positive  integer  such  that,  for  i  >  s,  the 
terms 

00          k 

2      ti  $,:,  jfc  (x), 
fc=c*i+l 

taken  from  the  end  of  the  convergent  series  (C),  are,  in  modulus,  less  than  et-, 
for  all  the  positions  of  x  outside  M  '  ;  then,  defining  a  function  gt  (x),  when 
i  >  s,  by  the  equation 

^    k 
9i  O)  =/i  OB)  ~fi  (a)  ~  2  tt  Si,  k  (a;), 

fc=0 

we  have,  tor  i  >  s, 


Thus  the  series 


2  [/((*)-/<(«>]  +    2 

t=l  i=s+l 


is  absolutely  and  uniformly  convergent  for  all  positions  of  x  not  in  the 
neighbourhood  of  the  places  c,  clt  c2,  ...,  and  represents  a  continuous  single 
valued  function  of  x.  When  a;  is  near  to  cit  the  function  represented  by  the 
series  is  infinite  like  /f  (#). 

The  function  is  not  unique  ;  if  i/r  (x)  denote  any  single-valued  function 
which  is  infinite  only  at  the  place  c,  the  addition  of  ty  (x)  to  the  function 
obtained  will  result  in  a  function  also  having  the  general  character  required 
in  the  enunciation  of  the  theorem.  As  here  determined  the  function 
vanishes  at  the  arbitrary  place  a  ;  but  that  is  an  immaterial  condition. 

For  instance  when  p  =  0,  and  the  place  m  is  at  infinity,  the  places  mlt  m2,  «ia,  ..., 
being  0,  1,  w,  l+a,  ...  ,  p  +  qa>,  ...  ,  wherein  o>  is  a  complex  quantity  and  pt  q  are  any 
rational  integers,  let  the  functions  f^x),  /,(#),  ...  be  x~\  (x-l}~\  (x-m)-\  ...  , 

He,  B       c= 


when  z  is  great  enough  and  |  x\  <  \  z  |,  |  a  \  <  \  z  |. 
Also 


1      _  ix-a 
a-nti     \mS 


when  im  is  great  enough,  and  |  x  \  <  \  m <  | ,  |  a  \  <  \  m^  \ . 


204  FORMATION   OF   AN    UNIFORM   FUNCTION  [144 

Now  the  series 

2     ^    =22 
mf 

is  convergent.     Hence  when  x  and  a  are  not  too  great 


' 


where  et  is  a  term  of  a  convergent  series  of  positive  quantities.     This  equation  holds  for 
all  values  of  i  except  i  =  l,  in  which  case  mi  =  0. 

Hence  we  may  write 


x-mi     a-mi      mf 
and  obtain  the  function 


i  r —     i    i  x~a  i 

=-ao  \_x-p-qo     a-p-qe>      (p  +  qu^J* 


*       «•     p=  —  oo    q 

which  has  the  property  required.     This  function  is  in  fact  equal,   in  the  notation  of 
"VVeierstrass's  elliptic  functions,  to  f(.t-  1,  a>)  — f(a  1,  «). 

145.     We  can  always  specify  a  rational  function  of  x  which,  beside  being 
infinite  at  the  place  c,  is  infinite  at  a  place  d  like  an  expression  of  the  form 

T-°  +  -2-1+ + 

tci       % 
ci 

namely,  such  a  function  is 


and  this  may  be  used  in  the  investigation  instead  of  the  function  fi  (x}  —fi  (a). 

Hence,  in  the  enunciation  of  the  theorem  of  §  144,  it  is  not  necessary 
that  the  expressions  of  the  rational  functions  fi  (x)  be  known,  or  even  that 
there  should  exist  rational  functions  infinite  only  at  the  places  Cj  in  the 
assigned  way.  All  that  is  necessary  is  that  the  character  of  the  infinity 
of  the  function  F,  at  the  pole  C;,  should  be  assigned. 

Conversely,  any  single-valued  function  F  whose  singularities  consist  of 
one  essential  singularity  and  an  infinite  number  of  distinct  poles  which 
converge  to  the  place  of  the  essential  singularity,  can  be  represented  by 
a  series  of  rational  functions  of  x,  which  beside  the  essential  singularity  have 
each  only  one  pole. 

146.  Let  the  places  c1}  c2,  ...,  c  be  as  in  §  144.  We  can  construct  a 
single-valued  function,  having  the  places  c1;  c2,  ...,  as  zeros,  of  assigned 
positive  integral  orders  Xj,  X2,  ...,  which  is  infinite  only  at  the  place  c,  where 
it  has  an  essential  singularity. 


147] 


WITH    GIVEN    ZEROS. 


205 


For  the  function 


E  (x,  z}  - 


is  zero  at  the  place  z  and  infinite  only  at  the  place  c.     When  z  is  near  to  c 
we  can  put 

-    tr 
Dz  log  E  (x,z)  =  2  f  [DJ  ^  (*,  a  ;  *,  c)]z=c, 


r=0 


and  therefore,  when  c4-  is  near  to  c,  and  #  is  not   near  to  the  place  c,  we 
can  put 

\t\ogE  (a,  a)  =  2  tJJBi,*(*), 

fr=o 

wherein  R^jg^ae)  is  a  rational  function  of  x   which   is  infinite  only  at  the 
place  c,  and  ti  has  the  same  significance  as  in  §  144. 

Let  the  least  value  of  i  for  which  this  equation  is  valid  be  denoted  by 
s+  I,  and,  taking  e,+1,  es+2,  ...  any  positive  quantities  such  that  the  series 


is  convergent,  let  /*t-  be  the  least  number  such  that,  for  i  >  s, 

00  Jf- 

2*          vi  JTVV    Jf  \^ )       ^   ^1* 

Then  the  series 

*  00  /  V-f 

2  Xi  log  E  (x,  d)  +2    ( \i  log  E  (x,  mi)  —  2  ti  R^  k  (x. 

i=l  i=s-fl  \  fr  =  0 

consists  of  single-valued  finite  functions  provided  x  is  not  near  to  any  of 
GI,  c2,  ...,  c,  and,  by  the  condition  as  to  the  numbers  //*,  is  absolutely  and 
uniformly  convergent. 

Hence  the  product 

«  00 

n  \E  (x  col**  n 

represents  a  single-valued  function,  which  is  infinite  only  at  c  where  it  has 
an  essential  singularity,  which  is  moreover  zero  only  at  the  places  c1}  C2,  ... 
respectively  to  the  orders  \lt  \2, 

With  the  results  obtained  in  §§  144 — 146,  the  reader  will  compare  the 
well-known  results  for  single-valued  functions  of  one  variable  (Weierstrass, 
Abhandlungen  aus  der  Functionenlehre,  Berlin,  1886,  pp.  1 — 66,  or  Mathem. 
Werke,  Bd.  ii.  pp.  77,  189). 

147.  The  following  results  possess  the  interest  that  they  are  given  by  Abel ;  they 
are  related  to  the  problems  of  this  chapter.  (Abel,'  (Euvres  Completes,  Christiania,  1881, 
vol.  i.  p.  46  and  vol.  ii.  p.  46.) 


206          INTERCHANGE  OF  ARGUMENT  AND  PARAMETER.          [147 

Ex.  i.     If  $  (x)  be  a  rational  polynomial  in  x,  =n 

and  /  (.r)  be  a  rational  function  of  x,  = 

then 

-/(»)  <6  (a?)  , 


The  theorem  can  be  obtained  most  directly  by  noticing  that  if  0  (#,  2)  = 


<p  (z)  (x  —  z) 
then 


is  a  rational  function  of  X     Denoting  it  by  R(X}  and  applying  the  theorem 


we  obtain  Abel's  result. 

Ex.  ii.     With  the  same  notation,  but  supposing  f(x}  to  be  an  integral  polynomial, 
prove  that 


wherein  Akt1c't  is  a  certain  constant,  and  \^  (x)  is  the  product  of  all  the  simple  factors  of 
This  result  may  be  obtained  from  the  rational  function 

as  in  the  last  example. 

Ex.  iii.     Obtain  the  theorem  of  Ex.  ii.  when  f(x)=Q,  and  0  (x)  =  ty  (.>•)]'"•     In  the 
result  put  »i=— £,  and  obtain  the  result  of  the  example  in  §  138. 

These  results  are  extended  by  Abel  to  the  case  of  linear  differential  equa 
tions.  Further  development  is  given  by  Jacobi,  Crelle  xxxii.  p.  194,  and  by 
Fuchs,  Crelle  Ixxvi.  p.  177. 


.148] 


CHAPTER   VIII. 

ABEL'S  THEOREM;  ABEL'S  DIFFERENTIAL  EQUATIONS. 

148.  THE  present  chapter  is  mainly  concerned  with  that  theorem  with 
which  the  subject  of  the  present  volume  may  be  said  to  have  begun.  It  will 
be  seen  that  with  the  ideas  which  have  been  analysed  in  the  earlier  part  of 
the  book,  the  statement  and  proof  of  that  theorem  is  a  matter  of  great 
simplicity. 

The  problem  of  the  integration  of  a  rational  algebraical  function  (of  a 
single  variable)  leads  to  the  introduction  of  a  transcendental  function,  the 
logarithm  ;  and  the  integral  of  any  such  rational  function  can  be  expressed 
as  a  sum  of  rational  functions  and  logarithms  of  rational  functions.  More 
generally,  an  integral  of  the  form 


\ 


dxR(x,y,  y,,  ...,  yk), 


wherein  x,  y,  yl}  yz,  ...  are  capable  of  rational  expression  in  terms  of  a  single 
parameter,  and  R  denotes  any  rational  algebraic  function,  can  be  expressed 
as  a  sum  of  rational  functions  of  this  parameter,  and  logarithms  of  rational 
functions  of  the  same.  This  includes  the  case  of  an  integral  of  the  form 


\dx  R  (x,  Vatf2  +  bx  +  c). 
But  an  integral  of  the  form 

\dx  R  (x,  Vow?4  +  bxs  +  cx2  +  dx  +  e) 

cannot,  in  general,  be  expressed  by  means  of  rational  or  logarithmic  functions ; 
such  integrals  lead  in  fact  to  the  introduction  of  other  transcendental  func 
tions  than  the  logarithm,  namely  to  elliptic  functions ;  and  it  appears  that 
the  nearest  approach  to  the  simplicity  of  the  case,  in  which  the  subject 
of  integration  is  a  rational  function,  is  to  be  sought  in  the  relations  which 
exist  for  the  sums  of  like  elliptic  integrals.  For  instance,  we  have  the 
equation 

I"*1  j dx      jx*  dx_ [x* (/.'.'  _  ., 

h   */(l-tf\(1—tMf\        o    A/H  -.7? VI  -kW      Jo    \/Cl  -ar'Ul  -  k*a*) 


208  INTRODUCTORY.  [148 

provided 


On  further  consideration,  however,  it  is  clear  that  this  is  not  a  complete 
statement  ;  and  it  is  proper,  beside  the  quantity  x,  to  introduce  a  quantity  y, 
such  that 


and  to  regard  y,  for  any  value  of  x,  as  equally  capable  either  of  the  positive 
or  negative  sign  ;  in  fact  by  varying  x  continuously  from  any  value,  through 

one  of  the  values  x=±\,  x=±j,  and  back  to  its  original  value,  we  can 

K 

suppose  that  y  varies  continuously  from  one  sign  to  the  other.  Then  the 
theorem  in  question  can  be  written  thus  ; 

/•<*-  0>>  dtKi      [<*"  ^  dx2      [<**•  y^dxs_ 

l(o,  i)     2A      J(o,  i)     2/2      J  (o,  i)      2/3 

where  the  limits  specify  the  value  of  y  as  well  as  the  value  of  x.  The 
theorem  holds  when,  in  the  first  two  integrals  the  variables  (x,  y)  are  taken 
through  any  continuous  succession  of  simultaneous  values,  from  the  lower  to 
the  upper  limits,  the  variables  in  the  last  integral  being,  at  every  stage  of 
the  integration,  defined  by  the  equations 


ys  (1  -  l&xfxff  =  S/iJ/2  (1  +  AfteiW)  -  XjX%  (I  -  &asfaif     1  -   2. 

The  quantity  y  is  called  an  algebraical  function  of  x\  and  the  notion  thus 
introduced  is  a  fundamental  one  in  the  theorems  to  be  considered  ;  its 
complete  establishment  has  been  associated,  in  this  volume,  with  a  Riemann 
surface. 

In  the  case  where  y2  =  (1  —  #2)  (1  —  &2#2)  we  have  the  general  theorem 
that,  if  R  (x,  y}  be  any  rational  function  of  x,  y,  the  sum  of  any  number,  m, 
of  similar  integrals 


f(*i,  I/,)  r^m'  2/m> 

M  (a,  y)  dx  +  ......  +  1 

J«-..*0  ** 


R(x,y)dx 


can  be  expressed  by  rational  functions  of  (x1}  y^,  ...,  (xm,  ym),  and  logarithms 
of  such  rational  functions,  with  the  addition  of  an  integral 


X*m+i.  y«+i> 

R  (x,  y}  dx. 

•/(««+!>   ZWl) 


Herein  the  lower  limits  (c^,  b^,  ...,  (am,  bm)  represent  arbitrary  pairs  of 
corresponding  values  of  x  and  y,  and  the  succession  of  values  for  the  pairs 
(a?i,  2/j),  ...,  (xm,  ym)  is  quite  arbitrary;  but  in  the  last  integral  a'm+1,  yM+i  are 
each  rational  functions  of  (scl}  y^,  ...,  (xm,  ym),  which  must  be  properly  deter- 


loO] 


INTRODUCTORY  STATEMENT. 


209 


mined,  and  it  is  understood  that  the  relations  are  preserved  at  all  stages  of 
the  integration,  so  that  for  example  am+l,  bm+1  are  respectively  taken  to  be 
the  same  rational  functions  of  (a1}  6j),  ...,  (am,  bm).  The  question  of  what 
alteration  is  necessary  in  the  enunciation  when  this  convention  is  not 
observed,  is  the  question  of  the  change  in  the  value  of  an  integral 

+l>  ?/m+l> 

R  (x,  y)  dx 

+l>  &m+l> 

when  the  path  of  integration  is  altered.  This  question  is  fully  treated  in  the 
consideration  of  the  Riemann  surface,  with  the  help  of  what  have  been  called 
period  loops. 

149.  Abel's  theorem  may  be  regarded  as  a  generalization  of  the  theorem 
just  stated,  and  may  be  enunciated  as  follows  :  Let  y  be  the  algebraical 
function  of  x  defined  by  an  equation  of  the  form 

f(y,  x)  =  yn+A}yn->  +  ......  +  An  =  0, 

wherein  Aly  .  ..,  An  are  rational  polynomials  in  cc,  and  the  left-hand  side  of 
the  equation  is  supposed  incapable  of  resolution  into  the  product  of  factors  of 
the  same  rational  form  ;  let  R  (x,  y)  be  any  rational  function  of  x  and  y  ; 
then  the  sum  of  any  number,  m,  of  similar  integrals 


r(*i,3/i>  n 

I          R(x,y)dx  +  ......  +  I 


R  (x,  y)  dx, 


with  arbitrary  lower  limits,  is  expressible  by  rational  functions  of  (xlt  ;?/,),  ..., 
(xm,  2/m)>  and  logarithms  of  such  rational  functions,  with  the  addition  of  the 
sum  of  a  certain  number,  k,  of  integrals, 


—  I          R  (x,  y)  dx  — —  I 


R  (x,  y)  dx, 


wherein  zl}  . ..,  zk  are  values  of  x,  determinable  from  xlt  yl}  ...,  xm,  ym  as  the 
roots  of  an  algebraical  equation  whose  coefficients  are  rational  functions  of 
x\>  y\>  •••,  ®m,  ym,  and  sl}  ...,  Sfc  are  the  corresponding  values  of  y,  of  which 
any  one,  say  S{,  is  determinable  as  a  rational  function  of  zt,  and  aelt  ylt  ..., 
xm,  ym-  The  relations  thus  determining  (zl}  s^,  ...,  (zk,  sk)  from  (x1}  y^,  ..., 
(xm,  ym}  may  be  supposed  to  hold  at  all  stages  of  the  integration ;  in 
particular  they  determine  the  lower  limits  of  the  last  k  integrals  from  the 
arbitrary  lower  limits  of  the  first  m  integrals.  The  number  k  does  not 
depend  upon  m,  nor  upon  the  form  of  the  rational  function  R  (x,  y} ;  and  in 
general  it  does  not  depend  upon  the  values  of  (#,,  y^,  ...,  (>„,,  ?/,„),  but  only 
upon  the  fundamental  equation  which  determines  y  in  terms  of  x. 

150.     In  this  enunciation  there  is  no  indication  of  the  way  in  which  the 

equations  determining  zly  sl}  ...,  zk,  sk  from  xlt  ylt  ...,  xm,  ym  are  to  be  found. 

Let  6  (y,  x)  be  an  integral  polynomial  in  x  and  y,  wherein  some  or  all  of  the 

coefficients   are   regarded   as    variable.      By   continuous   variation    of  these 

B.  14 


210  STATEMENT   OF   ABEL'S   THEOREM.  [150 

coefficients  the  set  of  corresponding  values  of  x  and  y  which  satisfy  both 
the  equations  f(y,  x)  =  0,  6  (y,  x)  =  0,  will  also  vary  continuously.  Then,  if 
m  be  the  number  of  variable  coefficients  of  6  (y,  x},  and  m  +  k  the  total 
number  of  variable  pairs  (x,  y}  which  satisfy  both  the  equations  f(y,  x}  =  0, 
Q(y,  x)  =  0,  the  necessary  relations  between  (x^,  y^),  ...,  (xm,  ym),  (zl}  s^),  ..., 
(zjf,  Sk)  are  expressed  by  the  fact  that  these  pairs  are  the  common  solutions  of 
the  equations  /(y,  x)  =  0,  6  (y,  x)  =  0.  The  polynomial  6  (y,  x}  may  have  any 
form  in  which  there  enter  m  variable  coefficients  ;  by  substitution,  in  6  (y,  x}, 
of  the  m  pairs  of  values  (xlt  y^,  ...,  (xm,  ym),  we  can  determine  these  variable 
coefficients  as  rational  functions  of  xlt  y1}  ...,  xm,  ym\  by  elimination  of  y 
between  the  equations  6  (y,  x}  =  0,  f(y,  x)  =  0,  we  obtain  an  algebraic  equa 
tion  for  x,  breaking  into  two  factors,  P0  (x)  P  (x)  =  0,  one  factor,  P0  (x),  not 
depending  on  xlt  ylf  ...,  xm,  ym,  and  vanishing  for  the  values  of  x  at  the 
fixed  solutions  of  f(y,x)  =  Q,  0(y,x)  =  0,  which  do  not  depend  on  x,,ylt 
..-,  xm,  ym,  the  other  factor,  P  (x),  having  the  form 

(x-xj  ...(x-xm)(xk  +  R^-1  +  ...  +  Rk), 

where  Rly  ...,  RK  are  rational  functions  of  x1}  ylt  ...,  xm,  ym.  Finally,  from 
the  equations  /(>;,  zi)  =  Q>  0(si,  z^  =  Q  we  can  determine  s-i  rationally  in 
terms  of  zit  xlt  yly  ...,#,»,  ym.  As  a  matter  of  fact  the  rational  functions  of 
#1,  2/i>  •••  >  xm,  ym,  which  appear  on  the  right-hand  side  of  the  equation  which 
expresses  Abel's  theorem,  are  rational  functions  of  the  variable  coefficients  in 


151.  When  0(y,x)  is  quite  general  save  for  the  condition  of  having 
certain  fixed  zeros  satisfying  f(y,  x)  =  0,  the  forms  of  (zly  sj,  ...,  (zky  sk)  as 
functions  of  (xlt  y^,  ...,(xm>  ym)  are  independent  of  the  form  of  6  (y,  x}.  This 
appears  from  the  following  enunciation  of  the  theorem,  which  introduces 
ideas  that  have  been  elaborated  since  Abel's  time,  and  which  we  regard  as  the 
final  form  —  Let  (a1;  6j),  ...,(aQ,  bQ)  be  any  places  of  the  Riemann  surface 
whatever,  such  that  sets  coresidual  therewith  have  a  multiplicity  q,  and  a 
sequence  Q  —  q=p  —  r—l,  where  r  +  I  is  the  number  of  0  polynomials 
vanishing  in  the  places  (a^  6j),  ...,  (aQ,  bQ);  let  (a?,,  y^,  ...,  (xq,  yq}  be  q 
arbitrary  places  determining  a  set  coresidual  with  (alt  6j),  ...,  (aQ,  6C),  and 
(z1}  Si),  ...,  (ZP-T-I,  SP-T-I)  be  the  sequent  places  of  this  set*  ;  then,  R  (x,  y) 
being  any  rational  function  of  (x,  y),  the  sum 

n*uj/i)  /•(*«•  v,)  _ 

R(x,y)dx+  ......  +  R(x,y)dx 

J  (a,,  V  1  (a?,  6«) 

is  expressible  by  rational  functions  of  (xlt  y^,  ...,  (xq,  yq},  and  logarithms  of 
such  rational  functions,  with  the  addition  of  a  sum 

/•<?!,  «i>  riv-i.^-T-i) 

—  R(x,y}dx—  ......  —  R  (x,  y)  dx 

•  '  («»+i,  b«+i)  J  (as,  b^ 

*  See  Chap.  VI.  §  95. 


152]  REDUCTION    TO    TWO    SIMPLE    CASES.  211 

herein  it  is  understood  that  the  paths  of  integration  are  such  that  at  every 
stage  the  variables  form  a  set  coresidual  with  (alt  6j),  ...,  (aQ,  bQ). 

The  places  (aly  b^,  ...,(cig,  bQ)  may  therefore  be  regarded  as  the  poles,  and 
(a?i,  ^j),  ...,  (xq,  yq),  (X,  Sj),  ...,  (^p_T_j,  .Sp_T_!)  as  the  zeros,  of  the  same  rational 
function  Z  (x)  ;  if  dl  (y,  x)  denote  the  form  of  the  polynomial  0  (y,  x)  when  it 
vanishes  in  (a1}  bj,  ...,  (aQ,  bq),  and  0%(y,  x}  denote  its  form  when  its  zeros 
are  (xlt  y^,  ...,  (zlt  s^,  .  ..,  the  function  Z  (x)  may  be  expressed  in  the  form 
#2  (y,  x}jdi(y,  x}.  If  the  polynomials  0i(y,  x},  0%(y,  x)  are  not  adjoint,  the 
function  will  be  of  the  kind,  hitherto  regarded  as  special,  which  takes  the 
same  value  at  all  the  places  of  the  Riemann  surface  which  correspond  to  a 
multiple  point  of  the  plane  curve  represented  by  the  equation  f  (y,  x)  =  0  ; 
this  fact  does  not  affect  the  application  of  Abel's  theorem  to  the  case. 

152.  To  prove  the  theorem  thus  enunciated,  with  the  greatest  possible 
definiteness,  we  shew  first  that  it  may  be  reduced  to  two  simple  cases. 

In  the  neighbourhood  of  any  place  of  the  Riemann  surface,  at  which  t  is 
the  infinitesimal,  we  can  express  R  (x,  y)-r.  in  a  series  of  positive  and 

negative  powers  of  t,  in  which  the  number  of  negative  powers  is  finite.  Let 
the  expression  at  some  place,  £,  where  negative  powers  actually  enter,  be 
denoted  by 


then,  if  P£  £  denote  any  elementary  integral  of  the  third  kind,  with  infinities 
at  f,  7,  and  E*'  c  denote  the  differential  coefficient  of  P^'  c  in  regard  to  the 
infinitesimal  at  £,  the  places  7,  c  being  arbitrary,  the  difference 


wherein  D^  denotes  differentiation  in  regard  to  the  infinitesimal  at  £,  is  finite 
at  the  place  £     The  number  of  places,  £,  at  which  negative  powers  of  t  enter 

•  dec 

in  the  expansion  of  R  (x,  y)  -=-  ,  is  finite  ;  dealing  with  each  in  turn  we  obtain 

an  expression  of  the  form 


wherein  7,  c  are  taken  the  same  for  every  place  £  ;  this  is  finite  at  all  places 
of  the  Riemann  surface,  except  possibly  the  place  7.  If  ty  be  the  infinitesi 
mal  at  this  place  the  function  is  there  infinite  like  (2AJ  log  ty.  But  in  fact 
S4,  is  zero  (Chap.  II.  §  17,  Ex.  (S):  Chap.  VII.  §  137,  Ex.  vi.).  Hence  the 

14-2 


212  PROOF   OF   THE   THEOREM.  [152 

function  under  consideration  is  nowhere  infinite,  and  is  therefore  necessarily* 
a  linear  aggregate  of  integrals  of  the  first  kind,  plus  a  constant.  Hence 
if  ua>  a,  ...,  ua''  "  be  a  set  of  linearly  independent  integrals  of  the  first  kind,  a 
denoting  the  place  (a,  6),  and  (7j  ,  .  .  .  ,  Cp  be  proper  constants,  we  have 


The  consideration  of  the  sum 


r*i  r*u 

i    R(x,y}dx  +  ......  +  1     R(x,y)dx, 

J  tt  a 


wherein  a^,  ...,  aQ  denote  the  places  (al}  6j),  ...,  (a^,  bQ),  and  xlf  ...,  XQ  denote 
the  places  (xly  yj,  ...,  (xq,  yg),  (z1}  s^,  ...,  (zp^_lt  sp-^-^),  is  thus  reduced  to 
the  consideration  of  the  two  sums 


,,     ... 

Ex.  i.     By  the  proposition  here  repeated  from  §  20,  Chap.  II.,  it  follows  that  any 
rational  function  can  be  written  in  the  form 


+  (^,  I/-1'1  0B_1  (x,  y)]/f  (y) 
where  (cf.  §  45,  Chap.  IV.) 

n-l 

(x,  |)  =  [<^o  (^  y)  H-  2   0,.  (a?,  y)  gr  (£,  r,)]/(x  -  £)f  (y), 
i 

»;  being  the  value  of  y  at  the  place  £. 

.£"#.  ii.     Prove  also  that  any  rational  function  with  simple  poles  at  |1}  £2,  ...  can  be 
written  in  the  form 


Xj,  A2>"'  bein§  constants,  and  «  denoting  an  arbitrary  place  (cf.  §  130,  Chap.  VII.). 

153.  We  shall  prove,  now,  in  regard  to  these  two  sums,  under  the 
conventions  that  the  upper  limits  are  coresidual  with  the  lower  limits,  and 
that  the  Q  paths  of  integration  are  such  that  at  every  stage  the  variables  are 
at  places  also  coresidual  with  the  lower  limits,  a  convention  under  which  the 
paths  of  integration  may  quite  well  cross  the  period  loops  on  the  Riemann 
surface,  that  the  first  sum  is  zero  for  all  values  of  i,  and  the  second  equal  to 
log  Z(£)/Z(ry),  Z(oc)  being  the-}-  rational  function  which  has  alt  ...,  aQ  as 
poles  and  x1}  ...,  x^  as  zeros.  The  sense  in  which  the  logarithm  is  to  be 
understood  will  appear  from  the  proof  of  the  theorem.  If  we  suppose  the 
lower  limits  arbitrarily  assigned,  the  general  function  Z  (x),  of  which  these 

*  Forsyth,  Theory  of  Functions,  §  234. 

t  If  two  rational  functions  have  the  same  poles  and  the  same  zeros  their  ratio  is  necessarily 
a  constant. 


154]  PROOF   OF   THE   THEOREM.  213 

places  a1(  ... ,  aq  are  the  poles,  will  contain  q  4- 1  arbitrary  linear  coefficients, 
entering  homogeneously,  and  the  assignation  of  q  of  the  zeros,  say  x1,  ...,xq, 
will  determine  the  others,  as  explained. — The  equations  giving  the  determi 
nation  will  be  such  functions  of  a,,  ...,  aQ  as  are  identically  satisfied  by  these 
places,  Oj,  ...,  (tq.  Hence  the  general  form  of  Abel's  theorem  is 


where  Z'  (f )  =  D$Z  (£) ;  the  term  2-4j  log  Z  (7)  =  log  Z  (7)  2-4 1  can  be  omitted 
because  2^  =  0  (Chap.  II.  p.  20  (8)).     Herein  Z  '(£)  is  a  rational  function  of 

n  n      Q nn    'T*  o* 

lt/i  j     .   .  .   .    \AJQ    CvlJ.VA    lA/i  j      *  •  •  j    t^rt  • 

154.  In  carrying  out  the  proof  we  make  at  first  a  simplification — Let 
Z(x),  or  Z,  be  the  rational  function  having  a1}  ...,  aQ  as  simple  poles  and 
#!,  ...,  #c  as  simple  zeros,  these  places  being  supposed  to  be  all  different; 
trace  on  the  Riernann  surface  an  arbitrary  path  joining  at  to  x^  chosen  so  as 
to  avoid  all  places  where  dZ  is  zero  to  higher  than  the  first  order,  and  let  /j, 
be  the  value  of  Z  at  any  place  of  this  path  ;  then  there  will  be  Q  —  1  other 
places  at  which  Z  has  the  same  value  JJL  ;  the  paths  traced  by  these  Q  —  1 
places  as  /*  varies  from  oc  to  0  are  the  paths  we  assign  for  the  Q  —  1  integrals 
following  the  first.  The  simultaneous  positions  thus  defined  for  the  variables 
in  the  Q  integrals  are,  for  q  >  1,  not  so  general*  as  those  allowed  by  the  con 
vention  that  the  simultaneous  positions  are  coresidual  with  Oj,  ...,  UQ;  but  it 
will  be  seen  that  the  more  general  case  is  immediately  deducible  from  the 
particular  one. 

Consider  now,  for  any  value  of  JJL,  the  rational  function 

1      dl 
Z-fji  dx' 

I,  =  IR(x,  y)dx,  being  any  Abelian  integral  whatever.     In  accordance  with 

a  theorem  previously  used  (Chap.  II.  p.  20  (8) ;  Chap.  VII.  §  137,  Ex.  vi.)  the 
sum  of  the  coefficients  of  t~l  in  the  expansions  of  (Z  -  n)~ldlldt,  in  terms  of 
the  infinitesimal  t,  at  all  places  where  negative  powers  of  t  occur,  is  equal  to 
zero.  Of  such  places  there  are  first  the  Q,  places  where  Z  is  equal  to  //..  We 
shall  suppose  that  dl/dt  is  finite  at  all  these  places ;  then  the  sum  of  the 
coefficients  of  t~l  at  these  places  is 

(^          ;fdA  M 


*  Sets  coresidual  with  two  given  coresidual  sets  have  a  multiplicity  q;  but  sets  equivalent 
with  two  given  coresidual  sets  have  a  variability  expressible  by  one  parameter  only  (cf.  Chap.  VI. 
§§  94-96). 


214  PROOF   OF  THE   THEOREM.  [154 

provided  Z  —  //,  be  not  zero  to  the  second  order  at  any  of  the  places,  that  is, 
provided  dZ  be  not  zero  to  higher  than  the  first  order.  In  accordance  with 
the  convention  made  as  to  the  paths  of  the  variables  in  the  integrals,  we 
suppose  this  condition  to  be  satisfied. 

Hence  this  sum  is  equal  to  the  sum  of  the  coefficients  of  t~l  in  the 
expansions  of  the  function  -  (Z  -  /Lt)"1  dl/dt  at  all  places,  only,  where  dl/dt  is 
infinite;  this  result  we  may  write  in  the  form 


H 


we  may  regard  this  equation  as  a  convenient  way  of  stating  Abel's  theorem 
for  many  purposes;  and  may  suppose  the  case,  in  which  an  infinity  of  dl/dt 
coincides  with  a  place  at  which  Z  =  p,  to  be  included  in  this  equation,  the 
left  hand  being  restricted  to  all  places  at  which  Z  =  p  and  dl/dt  is  not 
infinite. 

In  this  equation,  in  case  I,  =  u*'a,  be  any  integral  of  the  first  kind,  the 
right  hand  vanishes;  then,  integrating  in  regard  to  //,  from  oo  to  0,  we 
obtain 


In  case  /  be  an  integral  of  the  third  kind,  =  Pf  c  say,  and  Z  be  not  equal  to 
fi  either  at  £  or  7,  the  right  hand  is  equal  to 


1  1 

to\  I 


hence,  integrating, 

Z>»1,  «i     ,  >pXQ'ali  -  rj..  -   lr>».  /m 

pt.    '  -d*-          +  '    g' 


while,  if  the  places  at  which  the  rational  function  Z  (x)  has  the  values  /JL,  v  be 
respectively  denoted  by 

•&!  }    ......  )  «£  Q) 

and 

&l>   ......  )  a  Q 

we  have 

pz,',  a/  p*tt,a'u        _  ["•    7      /  _L  __  _1 

^  5^      L*P\  ZM-^ZM- 


For  any  Abelian  integral  we  similarly  have 

/-  •  a>  +  ......  +  1**  ?• 


which  is  a  complete  statement  of  Abel's  theorem. 


155]  REMARKS.  215 

155.  In  the  equation  (B),  and  in  the  equation  which  follows  it,  the 
significance  of  the  logarithm  is  determined  by  the  path  of  /j,  in  the  integral 
expression  which  defines  the  logarithm  ;  we  may  also  define  the  logarithm  by 
considering  the  two  sides  of  the  equation  as  functions  of  f. 

There  is  no  need  to  extend  the  equation  (B)  to  the  case  where  one  of  the 
paths  of  integration  on  the  left  passes  through  either  £  or  7,  since  in  that 
case  a  corresponding  infinite  term  enters  on  both  sides  of  the  equation. 

But  it  is  clear  that  the  condition  that  no  two  of  the  upper  limits  xl,  ...  ,  #g 
should  be  coincident  is  immaterial,  and  may  be  removed.  And  if  two  (or 
more)  of  the  places  at  which  Z  takes  any  value,  /j,,  should  coincide,  the 
equations  (A)  and  (B)  can  be  formed  each  as  the  sum  of  two  equations  in 
Avhich  the  course  of  integration  is  respectively  from  Z  —  GO  to  Z=  /JL  and  from 
Z  =  fj,  to  Z  =  0,  and  the  final  outcome  can  only  be  that  the  order  in  which  the 
upper  limits  xl,  ...,  XQ  are  associated  with  the  lower  limits  a^  ,  .  .  .  ,  aQ  may 
undergo  a  change.  But  in  the  general  case  we  may  equally  put,  for  example, 
in  equations  (A),  (B), 

/•*i  fz2  r*2  f*i  C^       .       /•«,  rx2  rxl 

dl  +    dl,=    dl+    dl+    dr+    dl,=    dl+    dl, 

J  al  J  a2  J  a,  J  jr2  •*  x\  J  at  J  a,  •'  a2 

with  proper  conventions  as  to  the  paths  ;  hence  the  condition  that  dZ  shall 
not  be  zero  to  higher  than  the  first  order  at  any  stage  of  the  integration  may 
be  discarded  also,  with  a  certain  loss  of  definiteness.  The  most  general  form 
of  equation  (A),  when  each  of  the  Q  paths  of  integration  are  arbitrary,  is  of 
course 


iiP  +  Ml'»titl  +  ......  +  Mp'a>'i>p,    (C) 

where  w^,  ...,  w'i>p  are  the  periods  of  ufa  and  Mlf  ...,  Mp'  are  rational 
integers,  independent  of  i.  We  shall  subsequently  see  that  this  equation  is 
sufficient  to  prove  that  the  places  xl}  ...,  XQ  are  coresidual  with  the  set 
a,,  ...,  aQ. 

If,   in   equation   (B),  we   substitute   for   Z(x)   any   one   of  its   rational 
expressions,  say*  6z(x)ldl(x),  we  shall  obtain 


where,  now,  02(x),  O^x)  are  any  two  polynomials,  integral  in  x  and  y,  of 
which,  beside  common  zeros,  02(x)  has  xlt  ...,  xq  for  zeros,  and  6^(x)  has 
OL  •••,  «y  for  zeros.  If  in  this  equation  we  suppose  any  of  the  coefficients  in 
Q*  (x)  to  vary  infinitesimally  in  any  way,  such  that  the  common  zeros  of  02  (x} 

9  (x)  is,  for  shortness,  put  for  what  would  more  properly  be  denoted  by  9  (y,  x). 


CASE   IN    WHICH   THE   LOGARITHM  [155 

and  $!(&•)  remain  fixed,  #2(#)  changing  thereby  into  02  (x)  +  802  (x),  the  places 
AI,  ...,  xq  changing  thereby  to  xl  +  dxl}  ...,  XQ  +  dxQ>  we  shall  obtain 


=  S  log 


^-      , 
02  (7) 

Avhich  is  slightly  more  general  than  any  equation  before  given,  in  that  the 
places  Xi  +  dxi,  ...,  xQ+dxQ,  though  coresidual  with  xlt  ...,  XQ,  are  not 
necessarily  such  that"  the  function  0a  (#)/0,  (a;)  has  the  same  value  at  all  of 
them.  This  general  equation  is  obtained  by  Abel  in  the  course  of  his  proof 
of  his  theorem. 

For  any  Abelian  integral  we  have,  similarly,  the  equation 


which,  also,  may  be  regarded  as  a  complete  statement  of  Abel's  theorem. 

156.     In  equation  (B)  the  logarithm  of  the  right  hand  will  disappear  if 
=  z("t\  namely  if  the  infinities  of  the  integral  be  places  at  which  the 
function  Z  (x)  has  the  same  value. 

One  case  of  this  may  be  noticed  ;  if  ^  (?/,  x)  be  an  integral  polynomial  of 
grade  (•/*  -  1)  a  +  n  -  3  (cf.  Chap.  VI.  §§  86,  91),  which  is  adjoint  at  all  places 
except  those  two,  say  A,  A',  which  correspond  to  an  ordinary  double  point  of 
the  curve  represented  by  the  equation  f(y,  x)  =  0,  the  integral 


/•/  /  \    "**'> 

/  (y) 

will  be  an  integral  of  the  third  kind  having  A,  A'  as  its  infinities.  Hence,  if 
in  forming  the  function  Z(x),  =  02(x)/01(x),  the  places  A,  A'  have  been 
disregarded,  so  that  the  polynomials  0l(x},  02(x)  do  not  vanish  in  these 
places,  the  function  Z  (x)  will  take  the  same  value  at  A  as  at  A',  and 
we  shall  obtain 

yx»ai  +  ......  _j_  y*^  _  0 

Hence  we  obtain  the  result  :  if,  in  the  formation  of  the  integrals  of  the 
first  kind  for  a  given  fundamental  curve,  we  overlook  the  existence  of  a 
certain  number,  say  B,  of  double  points,  we  shall  obtain  p  +  8  integrals,  where 
p  is  the  true  deficiency  of  the  curve;  and  these  integrals  will  be  linear 
aggregates  of  the  actual  integrals  of  the  first  kind  and  of  8  integrals  of  the 
third  kind.  If  in  the  formation  of  the  rational  functions  also  we  overlook 
the  existence  of  these  double  points,  Abel's  theorem  will  have  the  same  form 
of  equation  for  the  p  +  8  integrals  as  if  they  were  integrals  of  the  first  kind 
(cf.  §§  83,  90,  and  Abel,  (Euvres  Camp.,  Christiania,  1881,  Vol.  I.  p.  167). 

For  example,  let  a1?  ...,  aQ  be  arbitrary  places  in  which  r  +  1  ^-poly 
nomials  vanish  (Chap.  VI.  §§101,  93).  Take  q(=Q-p  +  r+l)  arbitrary 


157J  DISAPPEARS    FROM    THE    EQUATION.  217 

places  d,  ...,  cq,  and  so  determine  the  set  d,  .  ..  ,  CQ  coresidual  with  alt  ...,  «y. 
A  rational  function,  f(#),  which  has  the  places  al}  ...,  aQ  for  poles  and  the 
places  d,  ...,  CQ  for  zeros  is  quite  determinate  save  for  a  constant  multiplier. 
Let  j,\,  .  .  .  ,  XQ  be  any  set  of  places  at  which  f  (x)  has  the  same  value,  A  say, 
so  that  #!,  ...  ,  XQ  are  the  zeros  of  £(#)  —  .4  ;  then,  as  a1}  ...  ,  ac  are  the  poles 
of  £  (#)  —  A  .  we  have 

p*.  ,  <*,  p,u,  «,,       ,        £(Ci)-VJ 

^,,2-f  ^r,,,,         10g£(Cs)_^> 

and  as  f(d)  =  £(c.,)  =  0,  the  right  hand  is  zero. 

Hence,  calling  the  places  where  a  definite  rational  function  has  the  same 
value  a  set  of  level  points  for  the  function,  we  can  make  the  statement  —  the 
level  points  of  a  definite  function  satisfy  the  equations 


c1}  c.,  being  any  two  of  the  zeros  of  the  function. 

In  particular,  when  q  =  l,  the  sets  of  level  points  are  the  most  general 
sets  coresidual  with  the  poles  or  zeros  of  the  function.  Hence,  if  xly  ...,xp+1 
be  any  set  of  places  coresidual  with  a  fixed  set  c,,  ca,  ...,cp+li  in  which  no 
^-polynomials  vanish,  we  have  the  equations 


157.     Ex.  i.     We  give  an  example  of  the  application  of  Abel's  theorem. 
For  the  surface  associated  with  the  equation 


the  integral 

f.rP4-/?-/rP-l_l-       _j_c 

dx 


y 

is  of  the  second  kind,  becoming  infinite  only  at  the  (single)  place  #  =  oo.     Consider  the 
rational  function 


which,  for  general  values  of  A,...,  L0,  is  of  the  (2jo  +  l)th  order,  its  zeros,  for  instance, 
being  given  by 


To  evaluate  the  expression 

(-      1 
\dt  Z- 

the  place  .*  =  «    l^ing  the  only  one  to  be  considered,  we  put  x  =  t~'>  and  obtain 


218  EXAMPLES.  [157 


~- 

dl         ^P^fip-aT  ......      _2 

dt~     2  ~*' 


and  therefore 

dl      1  1      1  •     ,   A  —  A0  1        cl 

wherein  the  coefficient  of  t~l  is  ^  (A -^  A0)  (1— /i)~3. 

Hence,  if  .1^,  ...,  ^'2,,  +  l  be  the  zeros,  and  «!,...,  «2P  +  1  be  the  poles  of  Z,  we  have 


Now  the  zeros  of  Z  are  zeros  of  the  polynomial 


denoting  the  values   of  y  by  yl,  ...  ,  y.iv  +  v   and   using  F(x)  for   (x~x^  ......  (^'-^p  +  i), 

where  (xlty^,...,  (xp  +  l,yp  +  l)  are  any  p  +  l  of  the  places  (x^y^...,  (xtj>+1,  y2,  +  1),  we 
have,  from  the  jt?  +  1  equations 


and  hence,  if  6^  62,  ...   be  the  values  of  y  when  .v=a1,  a2,  ...,  and  ^T0(^)  =  (^  —  «x)  ... 
(^-ap  +  1),  we  have 


7^'^+  ......  +/«*H-i'ffl^i=i  2  Fr  2  F7^)- 

i=l  *     ^*V          i  =  l      0  \M't'' 

If  in  the  integral  /  the  term  .vp  be  absent,  the  value  obtained  for  the  sura 

1*1  '«l+  ......  +  7*8^-1  '  "SH-I 

will  be  zero. 

The  reader  will  notice  that  for  p  =  l,  we  obtain  an  equation  from  which  the  equation 


can  be  deduced,  ult  u%,  u3  being  arguments  whose  sum  is  zero  ;  and  that  the  algebraic- 
equation  whose  roots  are  x1}...,  x2p  +  1  gives 


/p  +  l        y.       \2 

#„  +  ......  +^  +  i  =  J^2  =  i      2 


which  for     =  \  becomes 


Io7]  HYPKRELLIPTIC    CASE.  219 

Ex.  ii.     If  Y)  Z  be  any  two  rational  functions,  and  u  any  integral  of  the  first  kind, 
prove  by  the  theorem 


/  1 

\(Y-b}(Z 


du  dx 

~ 


-J)  dx 

that  the  sum  of  the  values  of  (Y—b)~l  dujdZ,  at  all  places  where  £=c,  added  to  the  sum 
of  the  valuer  of  (Z—  c)~l  du/dY  &i  all  places  where  F=6,  is  zero. 

It  is  assumed  that  all  the  zeros  of  the  functions  Y-  b,  Z—c  are  of  the  hrst  order. 
Hence  prove  the  equation 

2    T—  =   5   (du       Z(x}-n 
8 


where  a1(  ...,  ag  are  the  places  at  which  Z(x)  =  v,  x1,  ...,  XQ  the  places  at  which  Z(x)=p, 
and  the  suffix  on  the  right  hand  indicates  that  the  values  of  the  expression  in  the  brackets 
are  to  be  taken  for  the  n  places  of  the  surface  at  which  x=b. 

It  is  assumed  that  there  are  no  branch  places  for  x=b. 

Ex.  iii.     If  </>  (x)  be  any  integral  polynomial  in  .r,  y*  =  (x,  l)2p  +  2>  =/(•*•')  say.  and  M  (x), 
N(x]  be  any  two  integral  polynomials  in  x  of  which  some  coefficients  are  variable,  and 

f(x)  .  M^(x}-^(x)  =  K(x-xl}  ......  (x-xgl 

where  K  is  a  constant  or  an  integral  polynomial  whose  coefficients  do  not  depend  upon 
the  variable  coefficients  in  M(x],  N  (x\  and  yi,...,ys  be  determined  by  the  equations 
yiM(Xi)  +  N(xi)  =  0,  then,  on  the  hypothesis  that  s  is  not  one  of  the  quantities  xlt  ...,  XQ> 
and  is  not  a  root  of/(#)  =  0,  prove  that 


(* 
J 


- 


where  C  is  a  constant,  and  R  is  the  coefficient  of  -  in  the  development  of  the  function 

)        !      N 
* 


in  descending  powers  of  x  ;  herein  the  signs  of  Jf(x)  ,  */f(zj  are  arbitrary,  but  must  be 
used  consistently. 


Shew  that  the  statement  remains  valid  when  f  (x)  is  of  order  2p  +  l  (in  which  case  the 
development  from  which  r  is  chosen  is  to  be  regarded  as  a  development  in  powers  of  */x)  • 
prove  that  r  is  zero  when  <£  (a?)  is  of  order  p,  or  of  less  order.  Obtain  the  corresponding 
theorem  when  2  is  a  root  of  f(x)  =  0. 

Ex.  iv.  The  result  of  Ex.  iii.  is  given  by  Abel  ((Euvres  Compl.,  Vol.  i.  p.  445),  with  a 
direct  proof.  We  explain  now  the  nature  of  this  proof,  in  the  general  case.  Let/  (y,  x)  =  0 
be  the  fundamental  equation,  and  let  6  (y,  x)  be  a  polynomial  of  which  some  of  the 
coefficients  are  variable  ;  if  y^  ...  ,  yn  be  the  n  conjugate  roots  of  /  (y,  x)  =  0  corresponding 
to  any  general  value  of  .r,  the  equation 

r  (x)  =  e  (#!,  .»)  6  (y2,  x}  ......  B  (yu,  .»:)  =  0, 

gives  the  values  of  x  at  the  finite  zeros  of  the  polynomial  6  (y,  x).  Suppose  that  the 
left-hand  side  breaks  into  two  factors  F0  (.v)  and  F  (x),  of  which  the  former  does  not 
contain  any  of  the  variable  coefficients  of  6  (y,  x}.  Let  £  be  a  root  of  F(x)  =  0,  and 
Vu  ••-,  in  be  the  corresponding  values  of  ij  ;  then  one  or  more  of  the  places  (£,  ^j),  ......  , 


220  EXPLANATION   OF   ABEI/S   PROOF.  [157 

(£>  »7n)  are  zeros  of  6  (y,  x)  ;  fix  attention  upon  one  of  these,  and  denote  it  by  (£,  rj).  Then 
if,  by  a  slight  change  in  the  variable  coefficients  of  6  (y,  x\  whereby  it  becomes  changed 
into  6  (y,  x)  +  80  (y,  x\  F  (x)  become  F  (x)  +  8F  O),  the  symbol  8  referring  only  to  the 
coefficients  of  6  (y,  x\  and  £  become  £  +  o?£,  we  have  the  equations 

"  (£)<*£=<>, 


8,-  (|)=  20  Oh,  £)  ......  5  fo.,,  £)  e  (,i  +  1,  |)  ......  <9  (,n,  ^)  80  fa,  £), 

i  =  l 

where  /*'  (g)  =  dF((;)/dg.     Denote  now  by  U  (x)  the  rational  function  of  x,  given  by 

U(x)  =  2  d  (y1?  x)  ......  6  (#_!,  #)  0  (yi  +  1,  a,-)  ......  0  (yn,  x)  W  (y4,  *•); 

»=i 

then  if  /i  (a-',  y)  be  any  rational  function  of  x  and  y,  we  have 


where,  on  account  of  ^  (r/,  ^)  =  0  we  can  write 


and 


=  0  (I),  say, 

0  (£)  being  a  rational  function  of  £  only.     Taking  the  sum  of  the  equations  of  this  form, 
for  all  the  zeros  of  6  (y,  x},  we  have 


herein  the  summation  on  the  right  hand  can  be  carried  out,  and  the  result  written  as  the 
perfect  differential  of  a  function  of  the  variable  coefficients  of  6  (y,  .r),  in  fact  in  the  form 


(#,  y)       *  log 
as  we  have  shewn. 

For  example,  when 

/  (y,  x)  =y3  +  x3  -  3ayx  -I,  6  (y,  x)  =y  -  mx  -  n,  we  have  F0  (x)  —  1, 

F  (x}  =  x3  +  (mx  +  n)3  —  Sax  (mx  +  n)  —  1  , 
and 

&<%  _  _  3£,8f  (|)_  _  _  3^rW(ga«i  +  a>Q  _  _  3g(mg  +  ?Q(gam  +  an)         >H|)    ( 

7s  -«l     /T^^'Tl)"        /'(«7)^«)  *"(£)  ^(f)' 

Now  ^^)_ 

- 


,  ,  „  cnwc          xw  (x)      3xm8m\  „. /«l»— a\ 

and  hence  2  -— — —„  =      „,  /  +  ^-  ,  =  -  38    ^ 5    , 

•7      a^     L*-W        l+m3Jx=cc  \l+m3/ 

as  is  easily  seen.     From  this  we  infer 

n  —  a        fmn  -  cA  ^  A'J  -  ^2 


2    I     .-^^.=  -3 
» = 


157]  ABEL'S  FORM  OF  THE  RESULT.  221 

In    this    example    it    is  easily   seen   that  the  integral  is  only   infinite  when  x   is 

infinite;  putting  x^t~\  the  equation  f  (y,  #)  =  0  gives  y=  -a>t~  l-au*  +  At  +  Bt*  + , 

where  «  =  1,  or  (-l±V^3)/2;    then   log  6  (y,  x)  dl/dt,    =\og  (y  -  m,r  -  n)  \xyl(yz-ax)} 
dxjdt,  has  (a»*+n)  a>2/(«  +  m)  for  coefficient  of  t~\  and  we  easily  find 


a+n        a>  2       a>  _ 

m  +  I       TO  +  O)  &      m  +  o)2" 


.Ek.  v.  If  Y,  Z  denote  any  two  rational  functions  (in  x  and  y\  such  that  there  is  no 
finite  value  of  x  for  which  both  have  infinities,  and  2  (YZ)  denote  the  sum  of  the  n 
conjugate  values  of  YZ  for  any  value  of  x,  and  [2  (YZ}\x_ay,  denote  the  sum  of  the 
coefficients  of  (x-  a)'1  in  the  expansions  of  the  rational  function  of  x,  2  (YZ),  for  all  finite 
values  of  x  for  which  Y  is  infinite,  and  [S  (YZ)^  denote  the  coefficient  of  x~l  in  the 
expansion  of  2  (YZ)  in  descending  powers  of  x,  it  is  easy  (cf.  §  162  below)  to  prove  that 


wherein,  on  the  left  hand,  the  dash  indicates  that  the  sum  is  to  be  taken  only  for  the 
finite  places  at  which  Z  is  infinite.  Hence  if  7  be  any  Abelian  integral,  =  \R(x,y)  d.v, 
we  have 

S  log  I  (a  ,))^-[.  (£«  log  0  (y,  • 

Hence,  if  we  assume  that  0  (y,  x)  has  no  variable  zeros  at  infinity,  we  can  obtain 
Abel's  theorem  in  the  form 


wherein  the  summation  on  the  left  refers  to  all  the  zeros  of  6  (y,  x). 

This  is  the  form  in  which  the  result  is  given  by  Abel  ((Euvres  Compl.,  Christiania,  1881, 
Vol.  i.  p.  159,  and  notes,  Vol.  ii.  p.  296),  the  right  hand  being  obtained  by  actual 
evaluation  of  the  summation  which  we  have  written,  in  the  last  example,  in  the  form 

_,    ^M_ 


*  (&**(&' 

The  reader  is  recommended  to  study  Abel's  paper*,  which,  beside  the  theorem  above, 
contains  two  important  enquiries  ;  first,  as  to  the  form  necessary  for  the  rational  function 
dl/dx,  in  order  that  the  right-hand  side  of  the  equation  of  Abel's  theorem  may  reduce  to  a 
constant,  next,  as  to  the  least  number  of  the  integrals  in  the  equation  of  Abel's  theorem, 
of  which  the  upper  limits  may  not  be  taken  arbitrarily  but  must  be  taken  as  functions 
of  the  other  upper  limits.  Though  the  results  have  been  incorporated  in  the  theory  here 
given  (§§  156,  151,  95),  Abel's  investigation  must  ever  have  the  deepest  interest. 

K.I:  vi.     Obtain  the  result  of  Ex.  i.  (§  157)  by  the  method  explained  in  Ex.  iv. 

*  Which  was  presented  to  the  Academy  of  Sciences  of  Paris  in  Oct.  1826,  and  published  by 
the  Academy  in  1841  (Mi'moirc*  par  dirfrx  xavants,  t.  vii.).  During  this  period  many  papers  were 
published  in  Crelle's  Journal  on  Abel's  theorem,  by  Abel,  Minding,  Jiirgensen,  Broch,  Richelot, 
Jacob!  and  Rosenhain.  (See  Crelle,  i — xxx.  I  have  not  examined  all  these  papers  with  care. 
Jiirgensen  uses  a  method  of  fractional  differentiation.) 


222  CONVERSE   OF   ABEL'S   THEOREM.  [157 

Ex.  vii.     Prove  that  the  sum  of  the  values  of  the  expression 

U.v 
J    ' 

wherein  v  is  any  linear  expression  in  the  homogeneous  coordinates  x,  y,  z,  U  is  any 
integral  polynomial  of  degree  m  +  n  —  3,  J  is  the  Jacohian  of  any  two  curves  /=0,  0  =  0, 
of  degrees  n  and  m,  and  the  line  v  =  0,  and  the  sum  extends  to  all  the  common  points 
of/=0  and  0  =  0,  vanishes,  multiple  points  of/=0,  0  =  0  being  disregarded. 

Hence  deduce  Abel's  theorem  for  integrals  of  the  first  kind. 

(See  Harnack,  Alg.  Diff.  Math.  Annal.  t.  ix.  ;  Cay  ley,  Amer.  Journ.  Vol.  v.  p.  158  ; 
Jacobi,  theoremata  nova  algebraica,  Crelle,  t.  xiv.  The  theorem  is  due  to  Jacobi  ;  for 
geometrical  applications,  see  also  Humbert,  Liouville's  Journal  (1885)  Ser.  iv.  t.  i.  p.  347)*. 

Ex.  viii.     For  the  surface 

ya=tf>  (*)*(*),     =/(*), 
wherein  0  (#),  ^  (x]  are  cubic  polynomials  in  #,  prove  the  equation 


wherein  .vlt  #2,  |  and  ml5  m2,  y  are  coresidual  with  the  roots  of  0  (#)=0,  and  |,  y  are  the 
places  conjugate  to  £  and  y  ;  conjugate  places  being  those  for  which  the  values  of  x  are 
the  same. 

158.  When  the  places  xl)...,xq  are  determined  as  coresidual  with 
the  fixed  places  an  ...  ,  aq,  p  —  r  —  l  of  the  places  xl}  ...,xq  are  fixed  by 
the  assignation  of  the  others.  Hence  the  p  +  1  relations,  Avhich  are  given  by 
Abel's  theorem, 


cannot  be  independent.  We  prove  now  first  of  all  that  the  last  may 
be  regarded  as  a  consequence  of  the  other  p  equations.  In  fact,  if  x\,  ...  ,  Xq 
and  alt  ...,  aqbe  any  two  sets  of  places,  sucJi  that,  for  any  paths  of  integration  , 


(i  =  l,2,  ...,p),  wherein  u*\a,  ...,u*'a  are  any  set  of  linearly  independent 
integrals  of  the  first  kind,  &>,-(1  ,  ...  ,  a>'i>p  are  the  periods  of  the  integral  u{'  ,  and 
M-i,  ...,  M'p  are  rational  integers  independent  of  i,  then  there  exists  a  rational 
function  having  the  places  a^,  ...,  aq  for  poles  and  the  places  ti\,  ...,  Xq  for 
zeros. 

For  if  vXi'a,  ...,  vl'n  be  the  normal  integrals  of  the  first  kind,  so  that  we 
have  equations  of  the  form, 

x,  a       f-i         x,  a  ,-i         x,  a 

Vi       =  C'j(  j  Wj       +  ......  +  Ci<p  Up     , 

*  Further  algebraical  consideration  of  Abel's  theorem  may  be  found  in  Clebscb-Lindemann- 
Benoist,  Lecona  sur  la  Geometrie  (Paris  1883)  Vol.  iii.  Geometrical  applications  are  given  by 
Humbert,  Liouville's  Journal,  1887,  1889,  1890  (Ser.  iv.  t.  iii.  v.  vi.). 


158]  THE    INDEPENDENT    AND   SUFFICIENT    EQUATION.  223 

wherein  C^,  ...,  Ciip  are  constants,  and  therefore,  also, 

Cit  j  ta^j  +  ......  +  Gi>  p  copi  j  =  0  or  1,  according  as  i  ^=j,  or  i  =j, 

and 

@i,  I  m'\,j  +  ......  +  Ci,P(0'p,j  =  ri,}> 

we  can  deduce 

v?'ai  +  ......  +v?'aa  =  Mt  +  Ml'Titt  +  ......  +M'pTitp. 

Consider  now  the  function 


«//    x         Uxa   +  ......  +  nx°a  -2"i(M\vx'c+  ......  +M'vx'°) 

Z(x)  =  e    "  '  xQ>aa  PP  ' 

c  being  an  arbitrary  place. 

Herein  an  integral,  Tix\,a,>  suffers  an  increment  2jri  when  a;  makes  a 
circuit  about  the  place  ^  ;  but  this  does  not  alter  the  value  of  Z  (#).  And 
in  fact  Z(x)  is  a  single-valued  function  of  x;  for  the  functions  11%  aa  have 
no  periods  at  the  first  p  period  loops,  while,  if  x  describe  a  circuit  equivalent 
to  crossing  the  t-th  period  loop  of  the  second  kind,  the  function  Z(x)  is  only 
multiplied  by  the  factor 


or  eiwlMi,  whose  value  is  unity. 

Further  the  function  Z  (x)  has  no  essential  singularities;  for  it  has  poles 
at  the  places  alt  ...  ,  ay,  and  is  elsewhere  finite. 

Since  the  function  has  zeros  at  xl ,  . . . ,  XQ  and  not  elsewhere,  the  state 
ment  made  above  is  justified. 

Ex.  i.     It  is  impossible  to  find  two  places  y,  £  such  that  each  of  the  p  integrals  wf-  f  is 
zero.     For  then  there  would  exist  a  rational  function,  given  by 


having  only  one  pole,  at  the  place  y.     (Of.  §  6,  Chap.  I.)     It  is  also  impossible  that  the 
equations 


wherein    3flt  ...,  Mp,  M\,  ...,  M'v   are    rational    integers    independent    of   i,    should   be 
simultaneously  true. 

Ex.  ii.     If  p  equations,  of  the  form 


exist,  y,  and  y2  are  the  poles  of  a  rational  function  of  the  .second  order,  and  the  surface 
hyi>erelliptic.     (Chap.  V.  §  52.) 


224  THE   NUMBER   OF   INDEPENDENT   EQUATIONS.  [159 

159.     In  regard  now  to  the  equations 


11. 


which  express  that  the  places  a?1}  ...,XQ  are  coresidual  with  the  places 
alt  .  .  .  ,  O,Q,  if  r  +  1  be  the  number  of  (^-polynomials  which  vanish  in  the  places 
al}  ...,aQ  (Chap.  VI.  §  93),  or  (Chap.  III.  §§  27,  37)  the  number  of  linearly 
independent  linear  aggregates  of  the  form 


wherein  C1,...,GP  are  constants,  which  vanish  in  these  places,  then, 
Q  —  p  +  r  +  1  of  the  places  xl,...,Xq  can  be  assumed  arbitrarily,  and  the 
equations  are  therefore  equivalent  to  only  p  —  r  —  1  equations,  determining 
the  other  places  of  xl  ,  .  .  .  ,  XQ  in  terms  of  those  assumed.  This  can  be  stated 
also  in  another  way  :  the  p  differential  equations 


express  that  the  places  oc1,  ...,XQ  are  coresidual  with  the  places  #j  +  dx^  ,  .  .  .  , 
XQ  +  dxq  ;  if  the  places  xly  ...,XQ  have  quite  general  positions  these  equations 
are  independent  ;  if  however  T  +  1  linearly  independent  linear  aggregates,  of 
the  form, 

~  du^  ~  dup 

Cld^c  +  ......  +^^-°' 

wherein  Clt  ...,CP  are  constants,  vanish  in  the  places  xlt  ...,Xy,  then  the  p 
differential  equations  are  linearly  determinable  from  p  —  r  —  1  of  them. 

Ex.  i.  A  rational  function  having  .r1}  ...,  .%  as  poles  of  the  first  order,  and  such  that 
Xu  ...,  Xp  are  the  coefficients  of  the  inverses  of  the  infinitesimals  in  the  expansion  of 
the  function  in  the  neighbourhood  of  these  places,  can  be  written  in  the  form 

\    r-*'  f  >     T>X"  c  • 

—  AT  1          —  ......  —  \o  1  ; 

i      /r  f 

X,  Xy 

the  conditions  that  the  periods  be  zero  are  then  the  p  equations 

A1Qi(#i)  +  ......  +XBOi(A'B)=0,     (i=l,  2,  ...,p). 

But,  if  we  take  consecutive  places  coresidual  with  xl,  ...,  .ry,  and  tl,...,t(l  be  the 
corresponding  values  of  the  infinitesimals  at  .vlt  ...,  ,re,  we  also  have 


thus,  if  the  first  q  (  =  Q  —  f>  +  r  +  1)  of  tlt  ...,  tu  be  taken  proportional  to  X,,  ...,  X,,  we  shall 
have  the  equations 

'iAi=  ......  =*«/*«• 

Ex.\\.  When  the  set  .r1,...,x(!,  beside  being  coresidual  with  o^,  ...,afi,  has  other 
specialities  of  position,  Abel's  theorem  may  be  incompetent  to  express  them.  For  instance, 
in  the  case  of  a  Riemann  surface  whose  equation  represents  a  plane  quartic  curve  with 
two  double  points,  there  is  one  finite  integral  ;  if  al9  ...,  «4  represent  any  4  rollinear  points, 
and  .r1?  ...,.r4  represent  any  other  4  collinear  points,  the  equation  of  Abel's  theorem  is 


1GO]  ABEL'S  DIFFERENTIAL  EQUATIONS.  225 

but  this  equation  does  not  express  the  two  relations  which  are  necessary  to  ensure  that 
xlt  ...,%i  are  collinear  ;  it  expresses  only  that  #l}  x2,  x3,  x±  are  on  a  conic,  S,  passing 
through  the  double  points,  or  that  x^,  .v2,  xa,  x±  are  the  zeros,  and  ax,  ...,«4  are  the  poles 
of  the  rational  function  S/LL0,  where  L=Q  is  the  line  containing  aly...,at  and  L0=Q  is 
the  line  joining  the  double  points. 

100.     From  these  results  there  follows  the  interesting  conclusion    that 
the  p  simultaneous  differential  equations 


have  algebraical  integrals,  Q  being  >  p,  and  «,,  ...,up  being  a  set  of  p  linearly 
independent  integrals  of  the  first  kind.  The  problem  of  determining  these 
integrals  consists  only  in  the  expression  of  the  fact  that  #,,  ...,  ary  con 
stitute  a  set  belonging  to  a  lot  of  coresidual  sets  of  places. 

The  most  general  lot  will  consist  of  the  sets  coresidual  with  Q  arbitrary 
fixed  places  a,,  ...,aQ,  in  which  no  (^-polynomials  vanish.  But  the  lot  does 
not  therefore  depend  on  Q  arbitrary  constants;  for  in  place  of  the  set 
a,,  ....  nQ  we  can  equally  well  use  a  set  Alt  ...,  AQ,  whereof  q,  =Q-pt  places 
have  positions  arbitrarily  assigned  beforehand  ;  in  other  words,  all  possible 
lots  of  sets  of  Q  places  with  multiplicity  q  can  be  regarded  as  derived  from 
fundamental  sets  of  Q  places  in  which  q  places  are  the  same  for  all.  A  lot 
depends  therefore  on  Q-q,=p}  arbitrary  constants,  and  this  number  of 
arbitrary  constants  should  appear  in  the  integrals  of  the  equations  (Chap  VI 
§96). 

We  may  denote  the  Q  arbitrary  places,  with  which  xlt...,x(i  are  coresidual, 
by  A1,...,Aq,al,...,ap,  so  that  A1,...,Aq  are  arbitrarily  assigned  before 
hand,  in  any  way  that  is  convenient,  and  the  positions  of  «,,  ...,ap  are  the 
arbitrary  constants  of  the  integration. 

Then  one  way  in  which  we  can  express  the  integrals  of  the  equations  is 
as  follows:  form  the  rational  function  with  poles,  of  the  first  order,  in  the 
places  #1,  ...,  xQi  and  determine  the  ratios  of  the  q  +  1  homogeneous  arbitrary 
coefficients  entering  therein,  so  that  the  function  vanishes  in  A^^^Aq. 
Then  the  function  is  determined  save  for  an  arbitrary  multiplier,  and 
must  vanish  also  in  a,,  ...,ap.  The  expression  of  the  fact  that  it  does  so 
gives  p  equations,  each  containing  one  of  ctj,  ...,  ap  as  an  arbitrary  constant. 

From  these  p  equations  we  may  suppose  p  of  the  places  aslt  ...,XQ,  say 
*i,...,  «P,  to  be  expressed  in  terms  of  o^....^  and  xp+l,  ...,XQ  (and 
Al,...,Aq).  The  resulting  equations  may  be  derived  also  by  forming  the 
general  rational  function  with  its  poles  in  a,,...,  ap>  A,  ,...,  Aq  and  eliminating 
the  arbitrary  constants  by  the  condition  that  this  function  vanishes  in 
xii  ®p+i,  tfp+2,  ...,acQ,i  being  in  turn  taken  equal  to  1,  2,  .  .  .  ,  p. 

B-  15 


226 


EXAMPLES   OF 


[160 


For  example,  for  Q=p  +  1,  if  ty  (as,  a;  z,  cl5  ...,  cp)  denote  the  definite 
rational  function  which  has  poles  of  the  first  order  in  the  places  z,cl,...,cp, 
the  coefficient  of  the  inverse  of  the  infinitesimal  at  the  place  z  being 
taken  =  —  1,  which  function  also  vanishes  at  the  place  a  (Chap.  VII.  §  122), 
then  a  complete  set  of  integrals  is  given  by 


;  #p+1,  #!,...,  #p)  =  0  =  ......  =  ^(ap,A;  xp+lt  x1}  ...,  xp\ 

and  a  complete  set  is  also  given  by 

^  (®I,XP+I',  A,  alt  ...,  ap)  =  0  =  ......  =  i/r  (xp,  xp+1  ;  A,  a,,...,  ap). 

The  first  of  these  integrals  is  in  fact  the  equation 


dup     dup 
dxl '    dxz ' 

dP     dP 


dxri 


du 


dx 


p+l 
dP 


=  0, 


wherein  P  =  P^'^,  and  may  be  regarded  as  derived  by  elimination  of 
dx1} ...,  dxp+l  from  the  p  given  differential  equations  and  the  differential  of 
the  equation  (§  156) 


,  and  (J.,  tt:,  ...,  <%,)  are  coresidual 


-    a,,  A 

which  holds  when  (a?1}  ...,  ^+1),  (c^ 
sets. 

^r.  i.     For  p  =  l,  the  fundamental  equation  being  yi  =  (x^  1)4=X2.^4  +  ...,  shew  that  the 

differential  equation 

ofei     c^2  =  0 

y\     yz 

has  the  integral 


where  62  =  (a,  1)4.     (Here  the  place  A  has  been  taken  at  infinity.) 

Shew  also  that  this  integral  expresses  that  the  places  (#1}  T/J),  (.r2,  y2)>  (#>  —  &)>  are  the 
variable  zeros  of  the  polynomial  —  y+jo  +  ^-X^2,  when  p  and  <?  are  varied. 

Ex.  ii.  For  jo  =  2,  the  fundamental  equation  being  3/2  =  (#,  l)c  =  X2^i6  +  ...,  using  the 
form  of  the  function  ty  (xi  a>  z>  ci>  •••>  CP)  given  in  Ex.  ii.  §  132,  Chap.  VII.,  and  putting 
the  place  A  at  infinity,  obtain,  for  the  differential  equations 


the  integral 


\Ai3C-t  \Aj3Cn  \AtJ(j  o  _. 

_J+  _2  +  _3  =  0j 
2/1  3/2 


3/i 


<i       z^  _ 

—    T  ,    —  "« 

3/2          3/3 


3/3 


to  -  a)  F'  to)      to  -  a)  ^'  (*a)      (^3  -  «)  ^"  W      ^  (a) 
wherein  /ri(.r)  =  (^-^1)(.'r-,'r.j)  (.r  — .rs),  b2=(a,  l)c,  and  the  position  of  the  place  (a,  6)  is 


l(jl] 


ABEL'S  DIFFERENTIAL  EQUATIONS. 


227 


the  arbitrary  constant  of  integration.     By  taking  three  positions  of  (a,  6)  we  obtain  a 
system  of  complete  integrals. 

Shew  that  this  integral  is  obtained  by  eliminating  pt  q,  r  from  the  equations  which 
express  that  the  places  (xlty^)y  Cr2J  #2)1  (xa>  2/3)1  (a>  ^)  are  zeros  of  the  polynomial 
—y  —  \y?  +px2  +  qx+r. 


Ex.  iii.     For  the  case  (p  =  3)  in  which  the  fundamental  equation  is  of  the  form 


(x,  y)4  being  a  homogeneous  polynomial  of  the  fourth  degree  with  general  coefficients,  etc., 
prove  that  an  integral  of  the  equations 


is  given  by 


where 


(2,  3,  4)  ^  +  (3,  1,  4)  Uz  +  (l,  2,  4)  ^3-(l,  2,  3)  ^4  =  0, 


(2,  3,  4)  = 


:r2    xz    ,r4 

3^2      3/3      2/4 

1       1      1 


etc., 


and 


/(6,  a)  being  =0,  and  the  position  of  (a,  6)  being  the  arbitrary  constant  of  integration. 
A  complete  system  of  integrals  is  obtained  by  giving  (a,  6)  any  three  arbitrary  positions. 
To  obtain  these  equations  the  place  A  has  been  put  at  x=0,  y  =  Q. 


Ex.  iv.     When  the  fundamental  equation  is  «4+2/4  =  l,  shew,  putting  the  place  A  at 
a?=l,  ?/  =  0,  that,  as  in  Ex.  iii.,  we  have  integrals  of  the  form 

(2,  3,  4)  CT1  +  (3,  1,  4)  U2  +  (l,  2,  4)  U3-(l,  2,  3)  ^  =  0, 


wherein 


and 


„  _i 


161.  The  method  of  forming  the  integrals  of  the  differential  equations 
which  is  explained  in  the  last  article  may  also  be  stated  thus:  take  any 
adjoint  polynomial  ty  which  vanishes  in  the  Q  places  Alt  ...,  Aq,  aly  ...,  ap; 
let  Oi,  ...,  CK  be  the  other  zeros*  of  i/r;  let  the  general  adjoint  polynomial 
of  the  same  grade  as  t/r,  which  vanishes  in  C,,  ...,  CR,  be  denoted  by 


X,  Xj,  ...,\9  being  arbitrary  constants.  By  expressing  that  the  places 
xi>  xp+i,  #p+2>  •••,  %Q  are  zeros  of  this  polynomial  we  obtain  a  relation 
whereby  #;  is  determined  from  xp+l,  ...,  XQ  in  terms  of  the  arbitrary  positions 


Beside  those  where/'  (y)  or  F'  (77)  vanishes  (cf.  Chap.  VI.  §  86). 


15—2 


228 


METHODS   OF   EXPRESSING 


[161 


a1}  ...,  ap  (and  Alt  ...,  Aq).     By  taking  i  =  1,  2,  ...,  p  we  obtain  a  complete 
system*  of  integrals. 

Now  instead  of  regarding  the  set  Alt  ...,  Aq,  al}  ...,  ap  as  the  arbitrary 
quantities  of  the  integration,  we  may  regard  the  set  C1,...,CK  as  the 
arbitrary  quantities,  or,  more  accurately,  we  may  regard  the  p  quantities 
upon  which  the  lot  of  sets  coresidual  with  Clt  ...,  CR  depends,  as  the 
arbitrary  quantities.  To  this  end,  and  under  the  hypothesis  that  no 
^-polynomials  vanish  in  the  places  Clt...,  CR,  imagine  a  set  of  places 
Bl,...,BB-p,  bl}...,bp  determined  coresidual  with  G^,...,CR>  in  which 
BI,...,  BR-P  have  any  convenient  positions  assigned  beforehand,  so  that  the 
lot  of  sets  coresidual  with  C1  ,  .  .  .  ,  GR  depends  upon  the  positions  of  61,...,  bp. 
Let  a  general  adjoint  polynomial  with  Q  +  R  variable  zeros  be  of  the  form 


wherein  fj,,  ...,  ^  are  arbitrary  constants,  and  k  is  for  shortness  written  for 
Q  +  R  —  p.  Then  an  integral  of  the  differential  equations  under  con 
sideration  is  obtained  by  expressing  that  the  places 

JJl,  ...,  £>R—p,  Vif  ...,  Op,  OCi,  Xp+},  Xp+i,  ••',  %Q 

are  zeros  of  the  polynomial  ®  ;  and  a  complete  system  of  integrals  is 
obtained  by  putting  i  in  turn  equal  to  1,  2,  ...,  p. 

Similarly  a   complete   set   of  integrals  is  obtained  by  expressing  that 
the  places 

SS1}  ...,  Xp  ,  (Kp+i  ,  .  .  .  ,  Xq  ,  GI,  i>i  ,  .  .  .  ,  JJR—p 

are  zeros  of  the  polynomial  @,  i  being  taken  in  turn  equal  to  1,  2,  ...,  p. 

In  this  enunciation  there  is  no  restriction  as  to  the  value  of  R,  save  that 
it  must  not  be  less  than  p. 

Ex.  i.     For  the  general  surface  of  the  form 

/  (y,  x}  -  (#,  y\  +  (x,  y)3  +  (x,  y)z  +  (.r,  y\  +  constant  =  0, 
a  set  of  integrals  of  the  equations 


tlcAj  _ 

f/TyT0' 


4 

?/(y<) 


T  =  °. 


is  given  by 


y\ 


y 


^2    ^15 


A     B     I 


*  And  we  can  of   course  obtain   quite   similarly   a   set   of  p    integrals,   each   connecting 
xl ,  . . . ,  xg ,  Alt  ...,  Av,  and  one  of  the  arbitrary  positions  a, ,  . . . ,  a,> . 


1C1]  THE   SOLUTION    OF   THE   EQUATIONS.  229 

where  /((!>;,  «*)=(),  f  (B,  J)  =  0,  i=l,  2,  3,  mid  the  place  (.1,  B)   may  be  taken  at  any 
convenient  position. 


Ex.  ii.     Taking  as  before  (J  =/»  +  !,  and  considering  the  hyperelliptic  case,  the  funda 
mental  equation  being 


we  require  a  polynomial  having  R  -\-p  +  1  variable  zeros  :   such  an  one  is 

Q=-y  +  X.u" 
It  being  equal  to  p,  and  we  have 


where  /*  (a-)  =  (#  -  .^  ......  (*--^f)  +  1),  0  (.v)  =  (je-bl)  ......  (x-bp). 

An  integral  of  the  differential  equations  may  be  obtained  by  eliminating  F,  6-',...,  H 
from  the  equations  expressing  that  the  places 

0|,  ...,  Op,  #f,  #p  +  1 

are  zeros  of  the  polynomial  e,  or  from  the  equations  expressing  that 

•vn  ••••>  -Vp)  **;:>  +  1>  "» 

are  zeros  of  this  polynomial,  and  a  complete  system  of  integrals,  in  either  case,  by  taking 
i  in  turn  equal  to  1,  2,  ...,  p. 

Or  a  complete  system  of  p  integrals  may  be  obtained  by  eliminating  F,  G,  ...,  H  from 
the  2p  +  1  equations  obtained  by  equating  the  coefficients  of  the  same  powers  of  x  on  the 
two  sides  of  the  equation. 

We  may  of  course  also  take  e  in  the  form 


then  R=p  +  l,  and  the  places  Bl,  ...,  BR_V  are  not  evanescent  ;  putting  the  place  Bl  at 
infinity  we  obtain  E=\,  as  above. 

Ex.  iii.     The  integration  in  the  previous  example  may  be  carried  out  in  various  ways. 
By  introducing  again  a  set  of  fixed  places  «u  ...,  ap,  A,  coresidual  with  x^  ...,  xp,  xp  +  l, 
we  can  draw  a  particular  inference  as  to  the  forms  of  the  coefficients  F,  G,  ...,  H.     For  if 
U  (x)  denote  X.r"  +  l  +  Fx*  +  ...  +  G,  and  U0  (x)  denote  what  U  (x)  becomes  when  x1,...,xp  +  l 
take  the  positions  alt  ...,  op,  A,  the  coefficients  F,  G,  ...,  H  being  then  F0)  G0,  ...,  ff0, 
and    also    F0(x)  =  (x-a1)  ......  (x  -  a}>}  (x  -  A  ),    then,   because    each    of    the    polynomials 

-y+  U  (x\  -y+U(}(x)  vanishes  in  the  places  61}...,  bp,  the  polynomial   U(x)-U0  (x} 
must  divide  by  0  (#),  namely  U  (x}  =  170  (x)  +  1  <f>  (#),  where  t  is  a  variable  parameter; 
or,  if  we  write  0  (x)  =  x»  +  t1x*>-i  +  ......  +  tp,  tlt...,tp  being  then  regarded,  instead  of 

&!,...,  6P,  as  the  arbitrary  constants  of  the  integration,  we  have 


and  the  quantities  G-^  F,  ...,  Jf-t,,  F  are  constants  in  the  integration,  being  unaltered 
when  the  places  ^,  ...,  xp  +  l  come  to  alt  ...,  av,  A.  Hence  we  can  formulate  the  following 
result:  let  the  ^  +  1  quantities  F9,  G0,  ...,  ff0  be  determined  so  that  the  polynomial 
-y+U0  (x)  vanishes  in  the  fixed  places  at,  ...,  ap,  A.  Then  denoting  (^-^...(^-ap) 
(x-A)  by  F0(x),  the  fraction 


is  an    integral    polynomial;    denote   it   by  (p-2F9  X)  (jev  +  tl  x»~i+  ......  +  <„),   so  that 


230  THE   HYPERELLIPTIC   CASE.  [161 

<j>0,tl,...ytp   are    uniquely  determined    in   terms  of  the  places  a,,  ...,  ap,  A,  and  put 
F(x)  for  x»  +  t1xp~1  +  ......  +  tp.     Then  xlt  ...,  xp  +  l  are  the  roots  of  the  equation 

]}*==(»-2F»  X)  F,  (*)-*  U0  (*) 


and  the  set  x1}...txp  +  l  varies  with  the  value  of  t,  which  is  the  only  variable  quantity 
in  this  equation.  By  equating  the  coefficients  of  the  various  powers  of  x  in  the 
polynomial  on  the  left-hand  side  of  this  equation  to  the  coefficients  in  the  polynomial 
(n-2F0\)  F(x\  we  can  express  each  of  the  symmetric  functions 

MI  =  X^  T  ......  T  Xp  +  i 


as  rational  quadratic  functions  of  a  variable  parameter  t,  containing  definite  rational 
functions  of  the  variables  at  the  places  a15  ...,  ap,  A  ;  the  place  A  may  be  given  any 
fixed  position  that  is  convenient  ;  the  positions  of  the  places  a1?  ...,  ap  are  the  arbitrary 
constants  of  the  integration. 

Ex.  iv.  By  eliminating  t  between  the  p  +  l  equations  obtained  at  the  end  of  Ex.  iii. 
we  obtain  the  complete  system  of  p  integrals.  In  particular  any  two  of  the  quantities 
/*!,  /J2,  ...  are  connected  by  a  quadratic  relation,  and  any  three  of  them  are  connected  by 
a  linear  relation  (Jacobi,  Crelle,  t.  32,  p.  220). 

Ex.  v.    From  the  equation 


we  infer 


where  hl—x1  +  ...+xp  +  l  ;  hence  if  a  be  the  value  of  x  at  a  branch  place  of  the  surface, 
we  have  from  Ex.  ii. 


and  if,  herein,  a  be  put  in  turn  at  any  p  of  the  branch  places  of  the  surface,  the  resulting 
values  of  <f>  (a)  may  be  regarded  as  the  arbitrary  constants  of  the  integration,  and  the 
resulting  equations  as  a  complete  set  of  integrals  ;  and  if  X  =  0,  as  we  may  always  suppose 
without  loss  of  generality  (Chap.  V.),  we  thus  obtain  the  p  integrals 


Clt  ...,  Cp  being  the  constants  of  integration  (Richelot,  Crelle,  xxiii.  (1842),  p.  369.  In  this 
paper  is  also  shewn  how  to  obtain  integrals  by  extension  of  Lagrange's  method  for  the 
case  p  =  I.  See  Lagrange,  Theory  of  Functions,  Chap.  II.,  and  Cayley,  Elliptic  Functions, 
1876,  p.  337). 

Ex.  vi.     By  comparing  coefficients  of  x2p  in  the  equation  of  Ex.  ii.,  we  obtain 

v  -  (2X0  +  F*}  =  0*  - 
where  h1=x1  +  ...  +  xll  +  1;   hence  prove  that 


r-l 


162]  ABEL'S  THEOREM  FOR  A  CURVE  IN  SPACE.  231 

by  Ex.  ii.  the  right-hand  side  is  a  constant  in  the  integration  ;  hence  this  equation  is  an 
integral  of  the  differential  equations;  in  particular  if  X  =  0,  fi  =  4,  which  is  not  a  loss  of 
generality,  we  have  the  integral 


where  C  is  a  constant  ;  this  is  a  generalization  of  the  equation,  for  p  —  1, 


(cf.  Ex.  i.  §  157). 

Ex.  vii.     Shew  that  if  the  fundamental  equation  be 


then  another  integral  is 

,.,..,Vl  p«_*  -i'_£  (i+...+  _L)_  „  (L+...+  j_y=Coilst. 

Lr=i^*  wJ       Vi       XP+J      Vft       *+i/ 

(Richelot,  loc.  cit.) 

Ex.  viii.     If  a0,  0^  be  the  values  of  x  at  two  branch  places  of  the  surface,  obtain  the 
equations 


(Of-^)  ......  (0,  -Op)  (oo-J)  ......  (Oo-Op) 

wherein  the  quantities  .4,  ...,ap  are  the  values  of  ^  at  fixed  places  coresidual  with 
*'i,...,  *'P+I>  Pi  ^8  an  absolute  constant,  and  ^  is  a  parameter  varying  with  the  places 
#!,...,  Xp+i-  Take  i  in  turn  equal  to  1,  2,  ...,  (p  +  1),  and,  eliminating  /x,  we  obtain  a 
complete  set  of  integrals.  In  particular  if  the  left-hand  side  of  this  equation  be  denoted 
by  GI  we  have  such  equations  as 

(Gi  -  1)  PJ  pk  (PJ  -  pk)  +  (Gj  -  1)  Pk  Pi  (PA  -  Pi)  +  (Gk  -  1)  pi  PJ  (pi  -  PJ)  =0. 
(Weierstrass,  Collected  Works,  Vol.  I.  p.  267.) 

162.  The  proof  of  Abel's  theorem  which  has  been  given  in  this  chapter 
can  be  extended  to  the  case  of  an  algebraical  curve  in  space.  Taking  the 
case  of  three  dimensions,  and  denoting  the  coordinates  by  a,  y,  z,  we  shall 
assume  that  for  any  finite  value  of  x,  say  x  =  a,  the  curve  is  completely  given 
by  a  series  of  equations  of  the  form 


x  =  a  +  , 

y  =  Pl(tl)     ,    y  =  P2(t2)     ,  .........  ,y  =  P*(fe)     ,          (D) 


wherein  wl  +  I,  ...,  wk  +  I  are  positive  integers,  ^,...,^  are  infinitesimals, 
and  PI,  Q1}  ...,  Pk)  Qk,  denote  power  series  of  integral  powers  of  the  variable, 
with  only  a  finite  number  of  negative  powers,  which  have  a  finite  radius 
of  convergence.  The  values  represented  by  any  of  these  k  columns,  for  all 
values  of  the  infinitesimal  within  the  radius  of  convergence  involved,  are  the 
coordinates  of  all  points  of  the  curve  which  lie  within  the  neighbourhood 
of  a  single  place  (cf.  §  3,  Chap.  I.)  ;  the  sum 


232  PROOF    ENTIRELY   ANALOGOUS  [162 

is  the  same  for  all  values  of  x,  and  equal  to  n,  the  order  of  the  curve.     A 

similar  result  holds  for  infinite  values  of  x ;  we  have  only  to  write  -  for  x  —  a. 

x 

We  assume  further  that  any  rational  symmetric  function  of  the  n  sets 
of  values  for  the  pair  (y,  z),  which  are  represented  by  the  equations  (D),  is  a 
rational  function  of  x. 

Then  we  can  prove  that  if  R  (x,  y,  z)  be  any  rational  function  of  x,  y,  z, 

dx 

the  sum  of  the  coefficients  of  t~l  in  the  expression  R  (x,  y,  z)  -j.  ,  at  all  the 

k  places  of  the  curve  represented  by  the  equations  (D),  is  equal  to  the 

coefficient  of    in  the  rational  function  of  x, 

x  —  a 


5  (x,  ylt  zd  +  R(x,y2,  z2)  + +  R  (x,  yn,  zn}. 

And  further  that  the  sum  of  the  coefficients  of  t~l  in  R  (x,  y,  z)  -^  at  all 

the  places  arising  for  x  =  oo  is  equal  to  the  coefficient  of  —  in  the  expansion 
of  the  same  rational  function  of  x,  namely,  equal  to  the  coefficient  of  t'1  in 

U  (x)  -r  ,  when  x  =  -. 
d/t  t 

Hence,  the  theorem 


which  holds  for  any  rational  function,  U  (x),  of  a  single  variable  (as  may  be 
immediately  proved  by  expressing  the  function  in  partial  fractions  in  the 
ordinary  way),  enables  us  to  infer,  in  the  case  of  the  curve  considered,  that 
also 


By  this  theorem,  applied  to  the  case 

T ]_        d^  R       ^      .  dx 

\_R  (x,  y,  z)  dx         ' 

we  can  prove  that  the  number  of  poles  of  R  (x,  y,  z)  is  equal  to  the  number 
of  its  zeros,  and  therefore  also  equal  to  the  number  of  places  where  R  (x,  y,  z) 
has  any  assigned  value  /*,,  a  place  being  counted  as  r  coincident  zeros  when 
the  expression,  in  R  (x,  y,  z),  of  the  appropriate  values  for  x,  y,  z,  in  terms 
of  the  infinitesimal,  leads  to  a  series  in  which  the  lowest  power  of  t  is  tr ; 
similarly  for  the  poles. 


162]  TO   THAT    FOR   SIMPLER   CASE.  233 

Hence,  if  /  be  any  integral  of  the  form  j  R  (x,  y,  z)  dx,  we  can  apply 
this  theorem  in  the  form 


dt  Z- 

Z  being  any  rational  function  of  a?,  y,  z,  and  so  obtain,  as  before  (§§  154,  155), 
the  theorem 


and  if  Z  is  of  the  form  02  (x,  y,  z)/0i  (a,  y,  z},  where  B2,  @i  are  integral  poly 
nomials,  we  can  put  the  right-hand  side 


=          log          '  J' 
[dt     8ei(x,1J, 

wherein  xl , . . . ,  xk  are  the  places  at  which  Z  =  0,  or  02  (x,  y,  z)  =  0,  and 
ttj ,  . . . ,  ak  are  the  places  where  Z—<x>  or  01  (x,  y,  z)  =  0,  and  the  places 
to  be  considered  on  the  right  hand  are  the  infinities  of  dl/dt. 

The  reader  may  also  consult  the  investigation  given  by  Forsyth,  Phil.  Trans.,  1883, 
Part  i.  p.  337. 

Take  for  example  the  curve  which  is  the  complete  intersection  of  the  cylinders 


For  any  finite  value  of  .v,  except  x=0  or  x=  1,  we  have  4  places  given  by 

y=  ±*Jx  (1—  &•),     z=  ±\/x. 

For  infinite  values  of.*;,  putting  x  =  -„  we  have  two  places  given  by 
.  1  1 


For  x=l,  putting  x=l  +  f2,  we  have  two  places  given  by 

&  =  &  +  ...  ,  y  = 

z=+(l+W+t..),  a= 

For  .£  =  0,  putting  .v  =  f2,  we  have  two  places  given  by 

*-*(!-*«•-...)  I  yy=-<(l_i^_       )? 

«=<  ,  z=t 

and,  at  j,'  =  0,y=0,  2  =  0,    d.v  :  dy  :  dz  =  -2t  :  1  :  1  or  =2«  :-l  :  1=0  :  1  :  1  or  =0  :-  1  :  1 
so  that  there  is  a  double  point  with  x  =  Q,y=±z  for  tangents. 

Consider  now  if—  ,  from  the  intersections  of  z  +  ax  +  by~0  to  those  of  s  +  a'x  +  b'y  =  0. 


234  EXAMPLE.  [162 

Put  /=  /  —  ;  then  -=-  ,  =  --  j-  ,  when  x  is  near  to  0,  has,  for  one  value, 
J  yz  at'     yzdt 


.  -W  ...)    .      1+6' 

whlle       lo  °  Lr108  T+6 


+ 


and  the  contribution  to  the  sum  (  -=-  log       —     T     I      ,  is  2  log  --- 

\dt     6  z+ax  +  byjt~l  &  1  +  6 

If  we  take  the  other  place  at  x=Q  we  shall  get,  as  the  contribution  to 


dt 
the  quantity  —  2  log  -  —  j-  . 

Thus,  on  the  whole  we  get,  at  #=0, 


It  is  similarly  seen  that  no  contribution  arises  at  the  places  #=1,  x  =  oo. 
Thus  on  the  whole 


[  <**!  I      f 

J  ^  7T       J 


Now  from  the  equations  zl-\-axJ-\-by1  =  0,  z2  +  ax.2-\-by2  —  ^  we  find 

b  = 

and  thus 

— ==-Jlqg 


which  is  a  result  that  can  be  directly  verified. 


168]  235 


CHAPTER    IX. 

JACOBI'S   INVERSION   PROBLEM. 

163.  IT  is  known  what  advance  was  made  in  the  theory  of  elliptic 
functions  by  the  adoption  of  the  idea,  of  Abel  and  Jacobi,  that  the  value 
of  the  integral  of  the  first  kind  should  be  taken  as  independent  variable,  the 
variables,  x  and  y,  belonging  to  the  upper  limit  of  this  integral  being  regarded 
as  dependent.  The  question  naturally  arises  whether  it  may  not  be  equally 
advantageous,  if  possible,  to  introduce  a  similar  change  of  independent 
variable  in  the  higher  cases.  We  have  seen  in  the  previous  chapter  that,  if 
u*  l  a  ,  .  .  .  ,  ux'  a  be  any  p  linearly  independent  integrals  of  the  first  kind,  the 
p  equations 


justify  us  in  regarding  the  places  x1}  ...,  xp  as  rationally  determinable  from 
the  arbitrary  places  a^,  ...,  aQ,  xp+1,  ...,  x^  hence  is  suggested  the  problem, 
known  as  Jacobi's  inversion  problem*,  which  may  be  stated  thus:  if 
Ul}  ...,  Up  be  arbitrary  quantities,  regarded  as  variable,  and  ai}  ...,  ap  be 
arbitrary  fixed  places,  required  to  determine  the  nature  and  the  expression  of 
the  dependence  of  the  places  xlt  ...,  xp,  which  satisfy  the  p  equations 


upon  Hie  quantities  U1}  ...,  Up.  It  is  understood  that  the  path  of  integration 
from  ar  to  xr  is  to  be  taken  the  same  in  each  of  the  p  equations,  and  is  not 
restricted  from  crossing  the  period  loops. 

164.  It  is  obvious  first  of  all  that  if  for  any  set  of  values  U1}  ...,  Uv 
there  be  one  set  of  corresponding  places  xlt  ...,  xp  of  such  general  positions 
that  no  ^-polynomial  (§  101)  vanishes  in  them,  there  cannot  be  another  set 
of  places,  Xi,  ...  ,  Xp,  belonging  to  the  same  values  of  Ult  ...  ,  Up.  For  then 
we  should  have 


*  Jacobi,  Crelle  xin.  (1835),  p.  55. 


236  GENERAL    EXPLANATION  [104 

and  therefore  (§  158,  Chap.  VIII.)  there  would  exist  a  rational  function 
having  xl}  .  ..,  xp  as  poles  and  #/,  ...,  xp  as  zeros,  which  is  contrary  (§  37, 
Chap.  III.)  to  the  hypothesis  that  no  ^-polynomial  vanishes  in  xli  ...,  xp. 

But  a  further  result  follows  from  the  §  referred  to  (§  158,  Chap.  VIII.). 
Let  2(0iti,  ...,  %(0i,p,  2&)/(  n  ...,  2&>/)p  denote  the  periods  of  ux'a,  and 
m1}  .  ..,  mp,  m^',  ...,  mp'  denote  any  rational  integers  which  are  the  same  for 
all  values  of  i.  On  the  hypothesis  that  the  inversion  problem  is  capable  of 
solution  for  all  values  of  the  quantities  U1}  ...,  Up,  suppose  these  quantities 
to  vary  continuously  from  the  values  U1}  ...,  Up  to  the  values  Vlt  ...,  Vp, 
where 

Vi  =  Ui  +  Zrn^i,  l  +  ......  +  ZnipWi,  v  +  2W/&)/,  j  +  ......  +  2m/o>/>  p, 

(i  =  l,2,  ...,p), 
=  Ui+  2fli,  say, 

and  let  zlt  ...,  zp  be  the  places  such  that 

,,.«,,  «i  ,         ,  uzp<«p  =  y.  . 

U>i  ilt  V  I  > 

then  it  follows  from  §  158,  that  the  places  zlt  .  ..,  zp  are,  in  some  order,  the 
same  as  the  places  xl}  ...,xp.  For  this  reason  it  is  proper  to  write  the 
equations  of  the  inversion  problem  in  the  form 


where  the  sign  ==  indicates  that  the  two  sides  of  the  congruence  differ  by  a 
quantity  of  the  form  2Hj.  And  further,  if  the  set  xlt  ...,xp  be  uniquely 
determined  by  the  values  Ult  ...,  Up,  any  symmetrical  function  of  the  values 
of  x,  y  at  the  places  of  this  set,  must  be  a  single-valued  function  of 
Ui,  ...,  Up.  Denoting  such  a  function  by  <j)(Ul,  ...,  Up),  we  have,  therefore, 

</>(tr1  +  2n1,  u2+m,,  ...,  up  +  2ap)  =  <t>(Ul,  ...,  Up). 

The  functions  that  arise  are  therefore  such  as  are  unaltered  when  the 
p  variables  Ui,  ...,  Up  are  simultaneously  increased  by  the  same  integral 
multiples  of  any  one  of  the  2p  sets  of  quantities  denoted  by 

?Wj  pi     *^t  n     •••}  ^^p,  r 

2ft)/,  r,  2Q)/,  r,  .  .  .  ,  2ft)/,  ,..  (r  =  1,  2,  .  .  .  ,  p). 

165.  The  sign  =  will  often  be  employed  in  what  follows,  in  the  sense 
explained  above.  There  is  one  case  in  which  it  is  absolutely  necessary. 
In  what  has  preceded  the  paths  of  integration  have  not  been  restricted  from 
crossing  the  period  loops.  But  it  is  often  convenient,  for  the  sake  of 
definiteness,  to  use  only  integrals  for  which  this  restriction  is  enforced.  In 
such  case  the  problem  expressed  by  the  equations 


166]  OF  JACOBl'S   INVERSION   PROBLEM.  237 

may  be  incapable  of  solution  for  some  values  of  Ul}  ...,  Up.     This  can  be 
seen  as  follows  :  if  both  the  sets  of  equations 


were  capable  of  solution,  it  would  follow,  by  §  158,  that  the  set  zlt  ...,  zp  is 
the  same  as  the  set  xlt  ...  ,  xp.  And  thence,  as  the  paths  are  restricted  not 
to  cross  the  period  loops,  we  should  have 

i  i  i  i         ' 

and  thence 


i  p  +  2m/&)/)  ,  +  ......  +  2wp'a>i'>  p  =  0  ; 

but  these  equations  are  reducible  to 

mi  +  w/r^  j  +  ......  +  m/Tj,  p  =  0, 

and,  therefore,  there  would  exist  a  function,  expressed  by 


(where  v*'  a,  ...,  v^  a  are  Riemann's  elementary  integrals  of  the  first  kind), 
everywhere  finite  and  without  periods.  Such  a  function  must  be  a  constant  ; 
thus  the  conclusion  would  involve  that  v*'  a,  ...,  vx'  a  are  not  linearly  inde 
pendent,  which  is  untrue. 

Hence  when  the  paths  of  integration  are  restricted  not  to  cross  the  period 
loops,  the  equations  of  the  inversion  problem  must  be  written 


in  this  case  the  integral  sum  on  the  left-hand  side  is  not  capable  of  assuming 
all  values;  and  the  particular  period  which  must  be  added  to  the  right-hand 
side  to  make  the  two  sides  of  the  congruence  equal  is  determined  by  the 
solution  of  the  problem. 

166.  Before  passing  to  the  proof  that  Jacobi's  inversion  problem  does 
admit  of  solution,  another  point  should  be  referred  to.  It  is  not  at  first 
sight  apparent  why  it  is  necessary  to  take  p  arguments,  Ult  ...,  Up,  and 
p  dependent  places  xl}  ...,  xp.  It  may  be  thought,  perhaps,  that  a  single 
equation 

ux-  a  =  U, 

wherein  ux>*  is  any  definite  integral  of  the  first  kind,  suffices  to  determine  the 
place  a;  as  a  function  of  the  argument  U.  We  defer  to  a  subsequent  place 
the  enquiry  whether  this  is  true  when  the  path  of  integration  on  the  left 
hand  is  not  allowed  to  cross  the  period  loops  of  the  Riemann  surface  ;  it  is 
obvious  enough  that  in  such  a  case  all  conceivable  values  of  U  would  not  arise, 


238  JACOBl'S   INVERSION   PROBLEM.  [166 

for  instance  U  =  oo  would  not  arise,  and  the  function  of  U  obtained  would 
only  be  defined  for  restricted  values  of  the  argument.  But  it  is  possible 
to  see  that  when  the  path  of  integration  is  not  limited,  the  place  x  cannot  be 
definitely  determinate  from  U.  For,  then,  putting  x  =/(  U},  we  must  have 
f(U+  2ft)  =f(U),  wherein 


TOI,  ...,mp'  being  arbitrary  rational  integers,  and  2o>i,  .  ..,  2cop'  being  the 
periods  of  ux>  a  ;  and  it  can  be  shewn,  when  p  >  1,  that  in  general  it  is 
possible  to  choose  the  integers  TOJ,  ...,  mp'  so  that  H  shall  be  within  assigned 
nearness  of  any  prescribed  arbitrary  value  whatever.  Thus  not  only  would 
the  function  y(^0  have  infinitesimal  periods,  but  any  assigned  value  of  this 
function  would  arise  for  values  of  the  argument  lying  within  assigned  near 
ness  of  any  value  whatever.  We  shall  deal  later  with  the  possibility  of  the 
existence  of  infinitesimal  periods;  for  the  present  such  functions  are  excluded 
from  consideration. 

The  arithmetical  theorem  referred  to*  may  be  described  thus;  if  al}  a2 
be  any  real  quantities,  the  values  assumed  by  the  expression  ^(11+  JV2a2) 
when  Nlt  N2  take  all  possible  rational  integer  values  independently  of  one 
another,  are  in  general  infinite  in  number  ;  exception  arises  only  in  the  case 
when  the  ratio  a^a2  is  rational  ;  and  it  is  in  general  possible  to  find  rational 
integer  values  of  NI  and  Nz  to  make  Nlal+N2a2  approach  within  assigned 
nearness  of  any  prescribed  real  quantity.     Similarly  if  a1}  a2,  a3,  b1}  b2,  b3  be 
real   quantities,    of  the   expressions   N1a1  +  NzOi  +  Nsa3)  N^+N^  +  N^s, 
where  NI,  N2,  N3  take  all  possible   rational  integer  values  independently 
of  one   another,    there    are,    in  general,   values  which   lie  within   assigned 
nearness  respectively  to  two  arbitrarily  assigned  real  quantities  a,  b.     More 
generally,  if  alt  ...,  ak,  b1}  ...,bk,  ......  ,  clt  ...,ck  be  any  (k-1)  sets  each  of 

k  real  quantities,  and  a,  b,  ...,c  be  (k  —  1)  arbitrary  real  quantities,  it  is 
in  general  possible  to  find  rational  integers  N1}  ...,  Nk  such  that  the  (k  —  1) 
quantities 

N,a,  +  ......  +  Nkak-a,  N&  +  ......  +  Nkbk-b,  ...,  N.C.  +  ......  +Nkck-c, 

are  all  within  assigned  nearness  of  zero. 

Hence  it  follows,  taking  k  =  2j9,  that  we  can  choose  values  of  the  integers 
TOJ  ,  .  .  .  ,  mp',  to  make  p  —  1  of  the  quantities 

nr  =  TO!&)r)1  +  ......  +  mpwrip  +  m1'cor'tl+  ......  +mp'a>r',p, 

say  Ilj,  ...,  £lp-i,  approach  within  assigned  nearness  of  any  (p—  1)  prescribed 
values,  and  at  the  same  time  to  make  the  real  part  of  the  remaining  quantity 
£lp  approach  within  assigned  nearness  of  any  prescribed  value  ;  but  the 
imaginary  part  of  £lp  will  thereby  be  determined.  We  cannot  therefore 

*  Jacobi,  loc.  cit.  ;   Hermite,  CrclJe,  LXXXVIII.  p.  10. 


168]  EXISTENCE    OF   A   SOLUTION.  239 

expect  to  obtain  an  intelligible  inversion  by  taking  less  than  p  new  variables 
Ui,  U2,  ...  ;  and  it  is  manifest  that  we  ought  to  use  the  same  number  of 
dependent  places  asl  ,  x2,  ____  On  the  other  hand,  the  proof  which  has  been 
given  that  there  can  in  general  only  be  one  set  of  places  aslf  ...,xp  corre 
sponding  to  given  values  of  Ul,  ...,  Up  would  not  remain  valid  in  case  the 
left-hand  sides  of  the  equations  of  the  problem  of  inversion  consisted  of  a 
sum  of  more  than  p  integrals;  for  it  is  generally  possible  to  construct  a 
rational  function  with  p  +  1  assigned  poles. 

167.  It  follows  from  the  argument  here  that  when  p  >  1  an  integral  of  the  first  kind, 
ux>a,  is  capable,  for  given  positions  of  the  extreme  limits,  x,  a,  of  the  integration,  of 
assuming  values  within  assigned  nearness  of  any  prescribed  value  whatever.  Though  not 
directly  connected  with  the  subject  here  dealt  with  it  is  worth  remark  that  it  does  not 
thence  follow  that  the  integral  is  capable  of  assuming  all  possible  values.  For  the  values 
represented  by  an  expression  of  the  form 


for  all  values  of  the  integers  m1,  ...,  mp,  m^,  ...,  mp,  form  an  enumerable  aggregate  — 
that  is,  they  can  be  arranged  in  order  and  numbered  —  o>  ,  .  .  .  ,  -  3,  -2,  —  1  ,  0,  1  ,  2,  3,  .  .  .  ,  oo  . 
To  prove  this  we  may  begin  by  proving  that  all  values  of  the  form  m^  +  ragtog  form 
an  enumerable  aggregate  ;  the  proof  is  identical  with  the  proof  that  all  rational  fractions 
form  an  enumerable  aggregate  ;  and  may  then  proceed  to  shew  that  all  values  of  the  form 
Mj^+m^  +  TOgCBj  form  an  enumerable  aggregate,  and  so  on,  step  by  step.  Since  then  the 
aggregate  of  all  conceivable  complex  values  is  not  an  enumerable  aggregate,  the  statement 
made  is  justified. 

The  reader  may  consult  Harkness  and  Morley,  Theory  of  Functions,  p.  280,  Dini, 
Theorie  der  Functionen  einer  reellen  Orosse  (German  edition  by  Luroth  and  Schepp), 
pp.  27,  191,  Cantor,  Ada  Math.  II.  pp.  363  —  371,  Cantor,  Crelle,  LXXVII.  p.  258,  Rendiconti 
del  Circolo  Mat.  di  Palermo,  1888,  pp.  197,  135,  150,  where  also  will  be  found  a  theorem 
of  Poincare's  to  the  effect  that  no  multiform  analytical  function  exists  whose  values  are  not 
enumerable. 

168.     Consider  now*  the  equations 
(A)  <"*'  +  ......  +  u?"a»=Ui,  (i=l,2,...,p) 

wherein,  denoting  the  differential  coefficient  of  uf  a  in  regard  to  the  infini 
tesimal  at  #  by  fa  (x),  the  fixed  places  c^,  ...,  Op  are  supposed  to  be  such  that 
the  determinant  of  p  rows  and  columns  whose  (i,  j)ih  element  is  //,_,-  (af)  does 
not  vanish  ;  wherein  also  the  p  paths  of  integration  a1toa;li...,apioxpt  are 
to  be  the  same  in  all  the  p  equations,  and  are  not  restricted  from  crossing  the 
period  loops. 

When  a?!,  ...,  xp  are  respectively  in  the  neighbourhoods  of  a,,  ...,  ap  and 
l/i,  ...,  Up  are  small,  these  equations  can  be  written 


The  argument  of  this  section  is  derived  from  Weierstrass  ;   see   the  references  given   in 
connection  with  §  170. 


240  CONSTRUCTION   OF   SOLUTION  [168 

wherein  tf  is  the  infinitesimal  in  the  neighbourhood  of  the  place  ar,  and  //./(#) 
is  derived  from  ^r  (x)  by  differentiation.     From  these  equations  we  obtain 

*r=iV,iZ7i  +  ......  +  Vr,PUp+U?+  Uf}+  ......  ,         (r  =  l,2,  ...,j>), 


where,  if  A  denote  the  determinant  whose  (i,  j)ih  element  is  ^(di),  V{j 
denotes  the  minor  of  this  element  divided  by  A,  and  U^  denotes  a  homo 
geneous  integral  polynomial  in  Ult  ...,  Up  of  the  kih  degree.  These  series 
will  converge  provided  U1}  ...,  Up  be  of  sufficient,  not  unlimited,  smallness. 
Hence  also,  so  long  as  the  place  xr  lies  within  a  certain  finite  neighbourhood 
of  the  place  cr>  the  values  of  the  variables  xr,  yr  associated  with  this  place, 
which  are  expressible  by  convergent  series  of  integral  powers  of  tr,  are 
expressible  by  series  of  integral  powers  of  t/j  ,  .  .  .  ,  Up  which  are  convergent 
for  sufficiently  small  values  of  Uly  ...,  Up. 

Suppose  that  the  values  of  Ult  ...t  Up  are  such  that  the  places  xl}  ...,  xp 
thus  obtained  are  not  such  that  the  determinant  whose  (i,  j)ih  element  is 
/AJ  (xi)  is  zero  ;  then  if  [/"/,  .  .  .  ,  Up  be  small  quantities,  it  is  similarly  possible 
to  obtain  p  places  #/,  .  .  .  ,  xp,  lying  respectively  in  the  neighbourhoods  of 
X-L,  ...,  xp,  such  that 

fcf'-f  ......  +  <"''*"=£//,  (i-l,2,...,p); 

by  adding  these  equations  to  the  former  we  therefore  obtain 

<•'•"'  4-  ......  +U?''0*  =  Ui  +  Ut',      (i  =  I,  2,  ...,  p). 

Since  all  the  series  used  have  a  finite  range  of  convergence,  we  are  thus 
able,  step  by  step,  to  obtain  places  xl  ,  .  .  .  ,  xv  to  satisfy  the  p  equations 


for  any  finite  values  of  the  quantities  Ul}  ...,  Up  which  can  be  reached  from 
the  values  0,  0,  .  .  .  ,  0  without  passing  through  any  set  of  values  for  which 
the  corresponding  positions  of  xlt  ...,  xp  render  a  certain  determinant  zero. 

169.  The  method  of  continuation  thus  sketched  has  a  certain  interest; 
but  we  can  arrive  at  the  required  conclusion  in  a  different  way.  Let 
Ult  ...,  Uploe  any  finite  quantities  ;  and  let  m  be  a  positive  integer.  When 
m  is  large  enough,  the  quantities  UJm,  .  .  .  ,  Upjm  are,  in  absolute  value,  as 
small  as  we  please.  Hence  there  exist  places  zlt  ...,  zp,  lying  respectively  in 
the  neighbourhoods  of  the  places  alt  ...,  ap,  such  that 

M*"a'+  ......  +uz*'ap  =  -  Ui/m          (i=I,  2,  ...,p). 

In  order  then  to  obtain  places  x1}  ...,  ocp,  to  satisfy  the  equations 


169]  FOR  ALL   VALUES   OF  THE  ARGUMENTS.  241 

it  is  only  necessary  to  obtain  places  acl,  ...,xp>  such  that 


and  it  has  been  shewn  (Chap.  VIII.  §  158),  that  these  equations  express  only 
that  the  set  ofmp  +  p  places  formed  of  zl}  ...,  zp,  each  m  times  repeated  and 
the  places  xl}  ...,  xp,  are  coresidual  with  the  set  of  (m  +  l)p  places  formed  of 
Oj,  ...,  ap  each  (ra+  1)  times  repeated. 

Now,  when  (m  +  1)^>  places  are  not  zeros  of  a  ^-polynomial,  we  may 
(Chap.  VI.)  arbitrarily  assign  all  but  p  of  the  places  of  a  set  of  (m+  l)p 
places  which  are  coresidual  with  them;  and  the  other  p  places  will  be 
algebraically  and  rationally  determinable  from  the  mp  assigned  places. 

Hence  with  the  general  positions  assigned  to  the  places  al}  ...,  ap,  it 
follows,  if  Z  denote  any  rational  function,  that  the  values  of  Z  at  the  places 
#!,  ...,  xp  are  the  roots  of  an  algebraical  equation, 


whose  coefficients  El,...,Ep  are  rationally  determinable  from  the  places 
z\,  •••,  Zp,  and  are  therefore,  by  what  has  been  shewn,  expressible  by  series 
of  integral  powers  of  UJm,  ...,  Upfm,  which  converge  for  sufficiently  large 
values  of  m.  Thus  the  problem  expressed  by  the  equations 


is  always  capable  of  solution,  for  any  finite  values  of  Ult  ...,  Up. 

It  has  already  been  shewn  (§  164),  that  for  general  values  of  Ult  ...,  Up 
the  set  xl}  ...,scp  obtained  is  necessarily  unique;  the  same  result  follows 
from  the  method  of  the  present  article.  It  is  clear  in  §  164,  in  what  way 
exception  can  arise;  to  see  how  a  corresponding  peculiarity  may  present 
itself  in  the  present  article  the  reader  may  refer  to  the  concluding  result 
of  §  99  (Chap.  VI).  (See  also  Chap.  III.  §  37,  Ex.  ii.) 

In  case  the  places  alt  ...,  ap  in  the  equations  (A)  be  such  that  the  deter 
minant  denoted  by  A  vanishes,  we  may  take  places  blt  ...,bp,  for  which 
the  corresponding  determinant  is  not  zero,  and  follow  the  argument  of  the 
text  for  the  equations 

' 


in  which  Ff  =  Ut  +  ua*'  b>  +  .  .    .  .  +  ua.p>  bp. 

1  1 

We  do  not  enter  into  the  difficulty  arising  as  to  the  solution  of  the  in 
version  problem  expressed  by  the  equations  (A)  in  the  case  where  Ult...,  Up 
have  such  values  that  a?lf  ...,  xp  are  zeros  of  a  ^-polynomial.  This  point 
is  best  cleared  up  by  actual  examination  of  the  functions  which  are  to 
be  obtained  to  express  the  solution  of  the  problem  (cf.*  §  171,  and 
*  See  also  Clebsch  and  Gordan,  Abel.  Functnen.,  pp.  184,  186. 

B-  16 


242  EXPRESSION    OF   SOLUTION  [169 

Props,  xiii.  and  xv.,  Cor.  iii.,  of  Chap.  X.).  But  it  should  be  noticed  that 
the  method  of  §  168  shews  that  a  solution  exists  in  all  cases  in  which  the 
fixed  places  c^,  ...,  ap  do  not  make  the  determinant  A  vanish  ;  the  peculiarity 
in  the  special  case  is  that  instead  of  an  unique  solution  sclt  ...,  xp,  all  the 
GOT+I  sets  coresidual  with  xl}  ...,  xp  are  equally  solutions,  r+1  being  the 
number  of  linearly  independent  ^-polynomials  which  vanish  in  xl}  ...,xp. 
This  follows  from  §§  154,  158. 

170.  We  consider  now  how  to  form  functions  with  which  to  express  the 
solution  of  the  inversion  problem. 

Let  I*  *  denote  any  elementary  integral  of  the  third  kind,  with  infinities 
at  the  arbitrary  fixed  places  £  7.  Then  if  a1}  ...,  av,  xlt  ...,  asp  denote  the 
places  occurring  on  the  left  hand  in  equation  (A),  it  can  be  shewn  that  the 
function 

m_  pxl,a1,  pxp,ap 

*7t,V    '     ' +  -tl,y 

is  the  logarithm  of  a  single  valued  function  of  Ult  ...,  Up,  and  that  the 
solution  of  the  inversion  problem  can  be  expressed  by  this  function ;  and 
further  that,  if  /*> a  denote  any  Abelian  integral,  the  sum 

2*1 1  «i     i  i     jXp,  Op 

can  also*  be  expressed  by  the  function  T. 

It  is  clear  that  in  this  statement  it  is  immaterial  what  integral  of  the 
third  kind  is  adopted.  For  the  difference  between  two  elementary  integrals 
of  the  third  kind  with  infinities  at  £,  7  is  of  the  form 


x,  a   ,  .   -»      x,  a 

1  p   p 


where  \l}  ...,  \p,  \  may  depend  on  f,  7  but  are  independent  of  ar;  hence 
the  difference  between  the  two  corresponding  values  of  T  is  of  the  form 


and  this  is  a  single-valued  function  of  U1}  ....  Up. 

For  definiteness  we  may  therefore  suppose  that  Px'  a  denotes  the  integral 
of  the  third  kind  obtained  in  Chap.  IV.  (§  45.     Also  Chap.  VII.  §  134). 

Then,  firstly,  when  ae1}  ...,xp  are  very  near  to  al5  ...,  ap,  and  Ult  ...,  Up 
are  small,  T  is  given  by 


ij   r>          «-\         /  ^^i 

4      U  [(«,,  f)  -  (a,,  ,)]  -    + 


*  The  introduction  of  the  function  T  is,  I  believe,  due  to  Weierstrass.  See  Crelle,  LII. 
p.  285  (1856)  and  Mathem.  Werke  (Berh'n,  1894),  i.  p.  302.  The  other  functions  there  used  are 
considered  below  in  Chaps.  XL,  XIII. 


170]  BY   ABELIAN   INTEGRALS.  243 

where  ti  denotes  the  infinitesimal  in  the  neighbourhood  of  the  place  ait  c 
is  an  arbitrary  place,  and  the  notation  is  as  in  §  130,  Chap.  VII.  It  is 
intended  of  course  that  neither  of  the  places  £  or  7  is  in  the  neighbourhood 
of  any  of  the  places  aly  ...,ap.  Now  we  have  shewn  that  the  infinitesimals 
Zj,  ...,  tp  are  expressible  as  convergent  series  in  Ult  ...,  Up.  Thus  T  is  also 
expressible  as  a  convergent  series  in  Ult  ...,  Up  when  Ult  ...,  Up  are 
sufficiently  small. 

Nextly,  suppose  the  places  xly  .  .  .  ,  xp  are  not  near  to  the  places  al}  ...,ap; 
determine,  as  in  §  168,  places  to  satisfy  the  equations 


m  being  a  large  positive  integer;  then  we  shall  also  have  (§  158,  Chap.  VIII.) 


where  Z  (x)  denotes  the  rational  function  which  has  a  pole  of  the  (m  +  l)th 
order  at  each  of  the  places  a1}  ...,  ap,  and  has  a  zero  of  the  mth  order  at  each 
of  the  places  z1}  ...,  zp.  The  function  Z  (x)  has  also  a  simple  zero  at  each 
of  the  places  xl}  ...,xp,  but  this  fact  is  not  part  of  the  definition  of  the 
function. 

This  equation  can  be  written  in  the  form 
wherein  T0  denotes  the  sum 


a? 


It  follows  by  the  proof  just  given  that  T0  is  expressible  as  a  series  of 
integral  powers  of  the  variables  UJm,  ...,  Up/m,  which  converges  for 
sufficiently  great  values  of  m;  and  it  is  easy  to  see  that  the  expression 
^  (£)/<£  (7)  is  also  expressible  by  series  of  integral  powers  of  UJm,  ...,  Up/m. 
For  let  the  most  general  rational  function  having  a  pole  of  the  (m  +  l)th 
order  in  each  of  a1}  ...  ,  ap  be  of  the  form 

Z(x)=\1Z1(a;)+  ......  +\npZmp(x)+\, 

wherein  Z^x),  ...,  Zmp(x)  are  definite  functions,  and  \,  Xlf  ...,  \mp  are 
arbitrary  constants.  Then  the  expression  of  the  fact  that  this  function 
vanishes  to  the  mth  order  at  each  of  the  places  zlt  ...,zp  will  consist  of 
mp  equations  determining  \1}  ...,  \np  rationally  and  symmetrically  in  terms 
of  the  places  zlt  .  .  .  ,  zv.  Hence  (by  §  108)  \,  .  .  .  ,  X^  are  expressible  as  series 
of  integral  powers  of  UJm,  ...,  Up(m.  Hence  Z(g)/Z(y)  is  expressible 
by  series  of  integral  powers  of  UJm,  ...,  Up/m. 

16—2 


244  INTRODUCTION   TO   SOLUTION  [170 

Hence,  for  any  finite  values  of  U1}  ...,  Up  the  function  eT  is  expressible 
by  series  of  integral  powers  of  U1}  ...,  Up.  It  is  also  obvious,  from  the 
method  of  proof  adopted,  that  the  series  obtained  for  any  set  of  values  of 
£/!,  ...,  Up  are  independent  of  the  range  of  values  for  U1}  ...,  Up  by  which 
the  final  values  are  reached  from  the  initial  set  0,  0,  . . . ,  0  ;  so  that  the 
function  eT  is  a  single  valued  function  of  Ul}  ...,  Up.  The  function  eT 
reduces  to  unity  for  the  initial  set  0,  0,  . . . ,  0. 

171.  An  actual  expression  of  the  function  eT,  in  terms  of  Ul}  ...,  Up, 
will  be  obtained  in  the  next  chapter  (§  187,  Prop.  xiii.).  We  shew  here  that 
if  that  expression  be  known,  the  solution  of  the  inversion  problem  can 
also  be  given  in  explicit  terms.  Let  n£*  denote  the  normal  elementary 
integral  of  the  third  kind  (Chap.  II.,  §  14).  Then  if  K  denote  the  sum 


it  follows,  as  here,  that  eK  is  a  single  valued  function  of  U1}  ...,  UP1  whose 
expression  is  known  when  that  of  eT  is  known,  and  conversely.  Denote  eK  by 
V(UL,  ...,  Up;  ^,7).  Let  Z(x)  denote  any  rational  function  whatever,  its 
poles  being  the  places  y^,  ...,<yk;  and  let  the  places  at  which  Z(x)  takes 
an  arbitrary  value  X  be  denoted  by  £x,  ...,  %k.  Then,  from  the  equation 
(Chap.  VIII.,  §  154), 


we  obtain  * 


the  left-hand  side  of  this  equation  has,  we  have  said,  a  well  ascertained 
expression,  when  the  values  of  Ul,  ...,  Up.  the  function  Z(sc\  and  the  value 
X,  are  all  given  ;  hence,  substituting  for  X  in  turn  any  p  independent 
values,  we  can  calculate  the  expression  of  any  symmetrical  function  of  the 

quantities 

Z(acl),  ...,  Z(xp), 

and  this  will  constitute  the  complete  solution  of  the  inversion  problem. 

It  has  been  shewn  in  §  152,  Chap.  VIII.  that  any  Abelian  integral  Ix>a 
can  be  written  as  a  sum  of  elementary  integrals  of  the  third  kind  and  of 
differential  coefficients  of  such  integrals,  together  with  integrals  of  the  first 
kind.  Hence,  when  the  expression  of  V(U1}  ...,  Up\  g,  7)  is  obtained,  that 
of  the  sum 

r*n  «i    i  i    72*.  <h> 

can  also  be  obtained. 

*  Clebsch  u.  Gordan,  Abeh.  Functionen,  (1866),  p.  175. 


172]  BY  THETA  FUNCTIONS.  245 

172.     The  consideration  of  the  function 

TT\xi,O'\     i  i     f~\xP>  aP 

fc7  f,y    ' 

which  is  contained  in  this  chapter  is  to  be  regarded  as  of  a  preliminary 
character.  It  will  appear  in  the  next  chapter  that  it  is  convenient  to 
consider  this  function  as  expressed  in  terms  of  another  function,  the  theta 
function.  It  is  possible  to  build  up  the  theta  function  in  an  a  priori 
manner,  which  is  a  generalization  of  that,  depending  on  the  equation 


whereby,  in  the  elliptic  case,  the  a-function  may  be  supposed  derived  from 
the  function  g>  (it).  But  this  process  is  laborious,  and  furnishes  only  results 
which  are  more  easily  evident  a>  posteriori.  For  this  reason  we  proceed  now 
immediately  to  the  theta  functions  ;  formulae  connecting  these  functions 
with  the  algebraical  integrals  so  far  considered  are  given  in  chapters  X.  XI. 
and  XIV. 


[173 


CHAPTER    X. 
RIEMANN'S  THETA  FUNCTIONS.    GENERAL  THEORY. 

173.  THE  theta  functions,  which  are,  certainly,  the  most  important 
elements  of  the  theory  of  this  volume,  were  first  introduced  by  Jacobi  in 
the  case  of  elliptic  functions.  *  They  enabled  him  to  express  his  functions 
sn  u,  en  u,  dn  u,  in  the  form  of  fractions  having  the  same  denominator,  the  zeros 
of  this  denominator  being  the  common  poles  of  the  functions  sn  u,  en  u,  dn  u. 
The  ratios  of  the  theta  functions,  expressed  as  infinite  products,  were  also 
used  by  Abel  f.  For  the  case  p  =  2,  similar  functions  were  found  by  Gopelj, 
who  was  led  to  his  series  by  generalizing  the  form  in  which  Hermite  had 
written  the  general  exponent  of  Jacobi's  series,  and  by  Rosenhain  §,  who 
first  forms  degenerate  theta  functions  of  two  variables  by  multiplying  to 
gether  two  theta  functions  of  one  variable,  led  thereto  by  the  remark  that 
two  integrals  of  the  first  kind  which  exist  for  p  =  2,  become  elliptic  integrals 
respectively  of  the  first  and  third  kind,  when  two  branch  places  of  the  surface 
for  p  =  2,  coincide.  Both  Gopel  and  Rosenhain  have  in  view  the  inversion 
problem  enunciated  by  Jacobi  ;  their  memoirs  contain  a  large  number  of 
the  ideas  that  have  since  been  applied  to  more  general  cases.  In  the  form 
in  which  the  theta  functions  are  considered  in  this  chapter  they  were  first 
given,  for  any  value  of  p,  by  Riemann||.  Functions  which  are  quotients 
of  theta  functions  had  been  previously  considered  by  Weierstrass,  without 
any  mention  of  the  theta  series,  for  any  hyperelliptic  case  11.  These  functions 
occur  in  the  memoir  of  Rosenhain,  for  the  case  p  =  2.  It  will  be  seen  that 

*  Fundamenta  Nova  (1829)  ;  Ges.  Werke  (Berlin,  1881),  Ed.  i.  See  in  particular,  Dirichlet, 
Gediichtnissrede  auf  Jacobi,  loc.  cit.  Bd.  i.,  p.  14,  and  Zur  Geschichte  der  Abelschen  Trans- 
cendenten,  loc.  cit.,  Bd.  n.,  p.  516. 

t  (Euvres  (Christiania,  1881),  t.  i.  p.  343  (1827).  See  also  Eisenstein,  Crelle,  xxxv.  (1847), 
p.  153,  etc.  The  equation  (b)  p.  225,  of  Eisenstein's  memoir,  is  effectively  the  equation 


i  Crelle,  xxxv.  (1847),  p.  277. 

§  Mem.  sav.  etrang.  xi.  (1851),  p.  361.     The  paper  is  dated  1846. 

||  Crelle,  LIV.  (1857)  ;  Ges.  Werke,  p.  81. 

1f  Crelle,  XLVII.  (1854);  Crelle,  LIT.  (1856);   Ges.  Werke,  pp.  133,  297. 


174]  CONVERGENCE   OF   THE   THETA   SERIES.  247 

the  Riemann  theta  functions  are  not  the  most  general  form  possible.     The 
subsequent  development  of  the  general  theory  is  due  largely  to  Weierstrass. 

174.  In  the  case  p  =  l,  the  convergence  of  the  series  obtained  by  Jacobi 
depends  upon  the  use  of  two  periods  2<w,  2<o',  for  the  integral  of  the  first 
kind,  such  that  the  ratio  o>'/&>  has  its  imaginary  part  positive.  Then  the 


quantity  q  =  e    w  is,  in  absolute  value,  less  than  unity. 

Now  it  is  proved  by  Riemann  that  if  we  choose  normal  integrals  of  the 
first  kind  v1^'  a,  ...,  v^a,so  that  v*'a  has  the  periods  0...0,  1,  0,  ...,  rr>l,  ...,Tr>p, 
the  imaginary  part  of  the  quadratic  form 

<£  =  run^+  ......  +  Trtrnrz+  ......  +  2rlj2w1w2  +  ......  +  2rr>snrns+  ...... 

is  positive*  for  all  real  values  of  the  p  variables  nly  ...,np.  Hence  for  all 
rational  integer  values  of  nl}  ...,  np,  positive  or  negative,  the  quantity  ein<i) 
has  its  modulus  less  than  unity.  Thus,  if  we  write  rr>  s  =  pr>  s  +  iKr>  s,  pr,  s 
and  Kr>s  being  real,  and  a1}  =61  +  iclj  ...,  ap,  =  bp  +  icp,  be  any  p  constant 
quantities,  the  modulus  of  the  general  term  of  the  p-fold  series 


r»p=  —  o 


wherein  each  of  the  indices  Wj,  ...,  np  takes  every  real  integer  value 
independently  of  the  other  indices,  is  e~L,  where 

L  =  -  (b^  +  ......  +  bpnp)  +  TT  (Knn?  +  ......  +  2/c1>2  r^n,  +  ......  ), 

=  -(&1n1+  ......  +  bpnp)  +  -^,  say, 

where  i/r  is  a  real  quadratic  form  in  w1}  ...,  np,  which  is  essentially  positive 
for  all  the  values  of  Wj,  .  ..,  np  considered.  When  one  (or  more)  of  nlt  ...,  np 
is  large,  L  will  have  the  same  sign  as  ty,  and  will  be  positive  ;  and  if  p,  be  any 

(f\"f 
1  +  -)     ; 
P/ 

/         7"\  "^ 

now  the  series  whose  general  term  is  f  1  H  —  )      will  be  convergent  or  not 

\        ft/ 

according  as  the  series  whose  general  term  is  i/r~'x  is  convergent  or  not,  for 

the  ratio  1  +  -  :  ^  has  the  finite  limit  I///,  for  large  values  of  n^,  ...,np; 
P 

and  the  series  whose  general  term  is  i/r"'*  is  convergent  provided  JJL  be  taken 

*  The  proof  is  given  in  Forsyth,  Theory  of  Functions,  §  235.     If  W*  a,  ...  ,  ?**'  a  denote  a  set  of 
integrals  of  the  first  kind  such  that  wx'a  has  no  periods  at  the  b  period  loops  except  at  br,  and 

has  there  the  period  1,  and  <rr,  i  ,  .  .  .  ,  oy,  p  be  the  periods  of  «£•  a  at  the  a  period  loops,  the  quadratic 
function 

<rn«i2+ 
has  its  imaginary  part  negative. 


248  EXPLANATION  OF  NOTATION.  [174 

>  ^p.     (Jordan,  Cours  d  'Analyse,  Paris,  1893,  vol.  I.,  §  318.)     Hence   the 
series  whose  general  terra  is 

£«,«!  +  ......  +apnp+iir<}> 

is  absolutely  convergent. 

In  what  follows  we  shall  write  27riur  in  place  of  ar  and  speak  of  u1}  ...,up 
as  the  arguments;  we  shall  denote  by  un  the  quantity  uln1  4-  ......  +upnp, 

and  by  rn2  the  quadratic  r^n^  +  ......  +  2T12w17i2  +  .......     Then  the  Riemann 

theta  function  is  defined  by  the  equation 


where  the  sign  of  summation  indicates  that  each  of  the  indices  nlt  ...,np 
is  to  take  all  positive  and  negative  integral  values  (including  zero), 
independently  of  the  others.  By  what  has  been  proved  it  follows  that  ©  (u) 
is  a  single-valued,  integral,  analytical  function  of  the  arguments  v^,  ...,  up. 

The  notation  is  borrowed  from  the  theory  of  matrices  (cf.  Appendix  ii.)  ;  T  is  regarded 
as  representing  the  symmetrical  matrix  whose  (r,  s)th  element  is  rr>  g,  n  as  representing 
a  row,  or  column,  letter,  whose  elements  are  n^,  ...,  np,  and  u,  similarly,  as  representing 
such  a  letter  with  u^  ,  .  .  .  ,  up  as  its  elements. 

It  is  convenient,  with  ®  (u),  to  consider  a  slightly  generalized  function, 
given  by 

®  (u  ;  q,  q'},  or  ©  (u,  q)  =  Ze2iriu  (n+9'}+^r  (n+q')*+*riq  <n+3')  . 

herein  q  denotes  the  set  of  p  quantities  ql}  ...,qp,  and  q'  denotes  the  set 
of  p  quantities  #/,  .  .  .  ,  qp,  and,  for  instance,  u  (n  +  q)  denotes  the  quantity 
un  +  uq',  namely 

«iWi  +  ......  +  upnp  +  u^  +  ......  +  upqp, 

and  T  (n  +  <?')2  denotes  rn2  -f  Zrnq  +  rq"2,  namely 
(TllWl2  +  .  .  .  +  2r1>2  n,  w,  +...)  +  2  %   I  rr,s  nrqs'  +  (r11?1/2  +  .  .  .  +  2r1)2  q.'q,'  +...). 


=l  r= 


The  quantities  qlt  ...,  qp,  q^,  ...,  qp  constitute,  in  their  aggregate,  the 
characteristic  of  the  function  ©  (u  ;  q)  ;  they  may  have  any  constant  values 
whatever  ;  in  the  most  common  case  they  are  each  either  0  or  ^. 

The  quantities  r^j  are  the  periods  of  the  Riemann  normal  integrals  of  the  first  kind  at 
the  second  set  of  period  loops.  It  is  clear  however  that  any  symmetrical  matrix,  o-,  which 
is  such  that  for  real  values  of  £1}  ....  kp  the  quadratic  form  <rk*  has  its  imaginary  part 
positive,  may  be  equally  used  instead  of  T,  to  form  a  convergent  series  of  the  same  form  as 
the  6  series.  And  it  is  worth  while  to  make  this  remark  in  order  to  point  out  that  the 
Riemann  theta  functions  are  not  of  as  general  a  character  as  possible.  For  such  a 
symmetrical  matrix  o-  contains  \p  Q»  +  l)  different  quantities,  while  the  periods  rr,  g  are 
(Chap.  I.,  §  7),  functions  of  only  3p-3  independent  quantities.  The  difference  |^(p  +  l) 
-(3p-3)=£0°-2)(p-3),  vanishes  for  />=2  orp  =  3;  for  p  =  4  it  is  equal  to  1,  and  for 
greater  values  of  p  is  still  greater.  We  shall  afterwards  be  concerned  with  the  more 
general  theta-functiou  here  suggested. 


175]  FUNDAMENTAL    IDENTITIES.  249 

The  function  6  (w)  is  obviously  a  generalization  of  the  theta  functions  used  in  the 
theory  of  elliptic  functions.     One  of  these,  for  instance,  is  given  by 


and  the  four  elliptic  theta  functions  are  in  fact  obtained  by  putting  respectively  q,  q'  =  0,  £  ; 

=ii;  =i,o;  =0,0. 

175.  There  are  some  general  properties  of  the  theta  functions,  imme 
diately  deducible  from  the  definition  given  above,  which  it  is  desirable  to 
put  down  at  once  for  purposes  of  reference.  Unless  the  contrary  is  stated  it 
is  always  assumed  in  this  chapter  that  the  characteristic  consists  of  half 
integers;  we  may  denote  it  by  J&,  ...,  ^/3P,  ^a1}  ...,  ^ap,  or  shortly,  by 
^fi,  ^a,  where  fti,  ...,  j3p,  a1}  ...,  ap  are  integers,  in  the  most  common  case 
either  0  or  1.  Further  we  use  the  abbreviation  nTO)TO/,  or  sometimes  only  £lm, 
to  denote  the  set  of  p  quantities 


wherein  mlt  ...,  mp,  m/,  ...,  mp'  are  2p  constants.  When  these  constants 
are  integers,  the  p  quantities  denoted  by  Hm  are  the  periods  of  the  p  Riemanri 
normal  integrals  of  the  first  kind  when  the  upper  limit  of  the  integrals  is  taken 
round  a  closed  curve  which  is  reducible  to  mt  circuits  of  the  period  loop  6; 
(or  mi  crossings  of  the  period  loop  a{)  and  to  m{  circuits  of  the  period 
loop  at,  i  being  equal  to  1,  2,  ...,p.  (Cf.  the  diagram  Chap.  II.  p.  21.) 
The  general  element  of  the  set  of  p  quantities  denoted  by  flm,  will  also 
sometimes  be  denoted  by  mt  +  Tim',  T»  denoting  the  row  of  quantities  formed 
by  the  iih  row  of  the  matrix  r.  When  mlt  ...,mp  are  integers,  the  quantity 
mi  +  Tim  is  the  period  to  be  associated  with  the  argument  Ui  . 

Then  we  have  the  following  formulae,  (A),  (B),  (C),  (D),  (E)  : 

@  (-  u  ;  ift  }a)  =  e«**  @  (u  ;  ±0,  £a),  (A). 

Thus  @(w  ;  £/3,  £a)  is  an  odd  or  even  function  of  the  variables  M,,  ...,  up 
according   as   /3a,  ={3^  +  ......  +  /3pap>  is  an  odd  or  even  integer;  in  the 

former  case  we  say  that  the  characteristic  |/S,  £a  is  an  odd  characteristic,  in 
the  latter  case  that  it  is  an  even  characteristic. 

The  behaviour  of  the  function  ®  (it)  when  proper  simultaneous  periods 
are  added  to  the  arguments,  is  given  by  the  formulae  immediately  following, 
wherein  r  is  any  one  of  the  numbers  1,  2,  ...  ,  p, 

©  (?/!,  .  .  .  ,  ur  +  1,  .  .  .  ,  up  ;  i&  £o)  = 

®  (  1*1  +  Tlf  r  ,   U2  +  T2,  P  ,    .  .  .  ,   Up  +  Tp>  r  ]    %  0,  ±  Ct)  = 

Both  these  are  included  in  the  equation 

@  (u  +  nm;  i/S,  i«)  =  e-*ri"»'  («+*"»')  +«(»««-»n'p)  e  (M  ;  i  /8,  ^  a),         (B)  ; 


250  FUNDAMENTAL   IDENTITIES.  [175 

herein  the  quantities  m^  ...,  mp,  m/,  ...,  mp  are  integers,  u  +  £lm  stands  for 

the  p  quantities  such  as  ur  +  mr  +  m1'rr>  1  + +  mpTr>p,  and  the  notation 

in  the  exponent  on  the  right  hand  is  that  of  the  theory  of  matrices ;  thus 
for  instance  m'rm  denotes  the  expression 

•£ 

2,  mr'  (TV,  i  m/  + +  Tfj  p  mp'\ 

r=l 

and  is  the  same  as  the  expression  denoted  by  rm'2. 

Equation  (B)  shews  that  the  partial  differential  coefficients,  of  the  second 
order,  of  the  logarithm  of  @  (u  ;  £/3,  ^a),  in  regard  to  ult  ...,  up,  are  functions 
of  u1}  ...,up,  with  2p  sets  of  simultaneous  periods. 

Equation  (B)  is  included  in  another  equation ;  if  each  of  /3',  a!  denotes  a 
row  of  p  integers,  we  have 


®  (i*  +  ifV,  ..;  1/3,  £  a)  =  e-i-'CH-tf  +*'+*«•)  ®  (u  ;  1/3  +  1/3',  }a  +  &),    (C)  ; 

to  obtain  equation  (B)  we  have  only  to  put  /3/  =  2mr,  a/  =  2m/  in  equation 
(C).     If,  in  the  same  equation,  we  put  ft'  =  —  /3,  a.'  =  —  a,  we  obtain 

®  (w  -  |flp,  «  ;  i/3,  £a)  =  e™  <M-iTa)  6  (M  ;  0,  0)  =  e«ia  (M-^T">  0  (M)  ; 
from  this  we  infer 

©  (tt  +  1^,  .),  (D)  ; 


this  is  an  important  equation  because  it  reduces  a  theta  function  with  any 
half-integer  characteristic  to  the  theta  function  of  zero  characteristic. 

Finally,  when  each  of  m,  m  denotes  a  set  of  p  integers,  we  have  the 
equation 

®  (u  ;  i/3  +  m,  |a  +m')  =  e™  ®  (M  ;  i/3,  -|a),  (E)  ; 

thus  the  addition  of  integers  to  the  quantities  |«  does  not  alter  the  theta 
function  ©(?*;  -|/3,  ^a),  and  the  addition  of  integers  to  the  quantities  ^/3 
can  at  most  change  the  sign  of  the  function.  Hence  all  the  theta  functions 
with  half-integer  characteristics  are  reducible  to  the  2^  theta  functions  which 
arise  when  every  element  of  the  characteristic  is  either  0  or  £. 

176.  We  shall  verify  these  equations  in  order  in  the  most  direct  way.  The  method 
consists  in  transforming  the  exponent  of  the  general  term  of  the  series,  and  arranging  the 
terms  in  a  new  order.  This  process  is  legitimate,  because,  as  we  have  proved,  the  series  is 
absolutely  convergent. 

(A)    If  in  the  general  term 


we  change  the  signs  of  uly  ...,  up,  the  exponent  becomes 

-  n  -  a  +  ^a)  +  ITTT  (  -  n  -  a  +  |a)  +  nift  (  -  n  —  a 


176]  NUMBER  OF  ODD   AND   OF   EVEN   FUNCTIONS.  251 

Since  a  consists  of  integers  we  may  write  m  for  -n-a,  that  is  mr=  -(nr  +  ar),  for 
r=  1,  2,  ...,  p  ;  then,  since  #  consists  of  integers,  and  therefore  e2n^n=  1,  the  general  term 
becomes 

7n'/3a      Z-niu(m+^a)+WT(m+^a)+mft(m+^a), 

V         '  •  O  9 

save  for  the  factor  em^a,  this  is  of  the  same  form  as  the  general  term  in  the  original  series, 
the  summation  integers  mx,  ...,  mp  replacing  nt,  ...,  np.  Thus  the  result  is  obvious. 

(B)     The  exponent 

27rt  (u  +  m  +  rm')  (n  +  £  a)  +  iirr  (n  +  \  of  +  ni(3  (n  +  \  a\ 
wherein  m+rm'  stands  for  a  row,  or  column,  of  p  quantities  of  which  the  general  one  is 

™r+Tr,  i  %'  +  ......  +rr,pwip', 

is  equal  to 

2iriu  (n  +  ^a)  +  inr  (n  -f  ^  a)2  +  irifi  (n  +  ^  a)  -f  Znimn  +  nima 


+  iri  (ma  -  ra'/3)  +  2nimn. 

Replacing  /•nimn  by  1  and  writing  n  for  n+m',  the  equation  (Bj  is  obtained. 
(C)     By  the  work  in  (B),  replacing  m,  m'  by  ^/S7,  %a  respectively,  we  obtain 


and  this  is  immediately  seen  to  be  the  same  as 


This  proves  the  formula  (C). 

It  is  obvious  that  equations  (D)  are  only  particular  cases  of  equation  (C),  and  the 
equation  (E)  is  immediately  obvious. 

It  follows  from  the  equation  (A)  that  the  number  of  odd  theta  functions  contained  in 
the  formula  Q(u;  jfft  £•)  is  2»-1(2P-  1),  and  therefore  that  the  number  of  even  functions 
is22P-2P-1(2P-l),  or  2P-!(2P+1). 

For  the  number  of  odd  functions  is  the  same  as  the  number  of  sets  of  integers, 
•^i)  y\->  •'••>xj>->yv->  each  either  0  or  1,  for  which 

#13/1  +  ......  +  x],y))  =  an  odd  integer. 

These  sets  consist,  (i),  of  the  solutions  of  the  equation 

#12/1  +  ......  +  ^p  -  \yv  -  1  =  an  odd  integer, 

in  number,  say,  f(p-  1),  each  combined  with  each  of  the  three  sets 

(*P,  &>)  =  (<>,  1),  (1,0),  (0,0), 
together  with,  (ii),  the  solutions  of  the  equation 

^i2/i  +  ......  +#p_1yp_1  =  an  even  integer, 

in  number  ^p~2-f(p-l),  each  combined  with  the  set 


Thus 

^)  =  3/(p-l 

=  22"  ~2  +  2  {22»  -  *  +  2/  (p  -  2)}  =  etc. 


Hence  the  number  of  even  half  periods  is  2"  ~  l  (2"  +  1  ). 


252  THE   RIEMANN   FUNCTION   HAS  p  ZEROS.  [177 

177.  Suppose  now  that  61,  ...,  ep  are  definite  constants,  that  m  denotes  a 
fixed  place  of  the  Riemann  surface,  and  x  denotes  a  variable  place  of  the  surface. 

,  x,m  i  x,m  x,m 

We  consider  p  arguments  given  by  ur  —  vr  +er,  where  vv  ,  . . . ,  vp  are 
the  Riemann  normal  integrals  of  the  first  kind.  Then  the  function  ©  (it)  is 
a  function  of  x.  By  equation  (B)  it  satisfies  the  conditions 

©  (u  +  k)  =  ©  (u),    ©  (w,  +  rrk')  =  e-27rik'  <M+*T*'>  ©  (u), 

wherein  k  denotes  a  row,  or  column,  of  integers  k1}  ...,  kp  and  k'  denotes 
a  row  or  column  *  of  integers  &/,  ...,  kp'.  As  a  function  of  x,  the  function 

©  (vx>  m  +  e)  cannot,  clearly,  become  infinite,  for  the  arguments  vr'  +  er  are 
always  finite  ;  but  the  function  does  vanish  ;  we  proceed  in  fact  to  prove  the 
fundamental  theorem — the  function  ©  (vx' m  +  e)  has  always  p  zeros  of  the 
first  order  or  zeros  whose  aggregate  multiplicity  is  p. 

For  brevity  we  denote  vr'  +  er  by  ur.  When  the  arguments  u^,  ...,  up 
are  nearly  equal  to  any  finite  values  Ult  ...,  Up,  the  function  ©  (u)  can 
be  represented  by  a  series  of  positive  integral  powers  of  the  differences 
MI—  Ult  ...,up—  Up.  Hence  the  zeros  of  the  function  ©(M),  =  ©  (if-  m  +  e), 
are  all  of  positive  integral  order.  The  sum  of  these  orders  of  zero  is  there 
fore  equal  to  the  value  of  the  integral 

_— .  (d  log  0  (M)  =  ~ .  1 1  <K©/  0)/@  (u)  =  ^-.  I dx  I  (du,jdx)  (©/(»/©(w)), 

wherein  the  dash  denotes  a  partial  differentiation  in  regard  to  the  argument 
u,,  and  the  integral  is  to  be  taken  round  the  complete  boundary  of  the  p-ply 
connected  surface  on  which  the  function  is  single- valued,  namely  round  the  p 
closed  curves  formed  by  the  sides  of  the  period-pair-loops.  (Cf.  the  diagram, 
p.  21.) 

Now  the  values  of      * ,  .    -^  at  two  points  which  are  opposite  points  on 
0 (u)    dx 

a  period-loop  ar  are  equal,  and  in  the  contour  integration  the  corresponding 
values  of  dx  are  equal  and  opposite.  Hence  the  portions  of  the  integral 
arising  from  the  two  sides  of  a  period-loop  ar  destroy  one  another.  The 

values  of  •*}"  .  at  two  points  which  are  opposite  points  on  a  period-loop  br 
differ  by  —  2?™,  or  0,  according  as  s  =  r  or  not. 

Hence  the  part  of  the  integral  which  arises  from  the  period-loop-pair 
(ar,  br)  is  equal  to  —  I  dur,  taken  once  positively  round  the  left-hand  side  of 
the  loop  br,  namely  equal  to  —  (—  1)  =  1. 

The  whole  value  of  the  integral  is,  therefore,  p ;  this  is  then  the  sum 
of  the  orders  of  zero  of  the  function  ©  (vx> m  +  e), 

*  The  notation  ur  +  rrk'  denotes  the  p  arguments  UJ  +  TJ&',  ...,  up  +  rpk'. 


178] 


EQUATIONS    FOR   THE   POSITION    OF   THE   ZEROS. 


253 


178.  In  regard  to  the  position  of  the  zeros  of  this  function  we  are  able 
to  make  some  statement.  We  consider  first  the  case  when  there  are  p  dis 
tinct  zeros,  each  of  the  first  order.  It  is  convenient  to  dissect  the  Riemann 
surface  in  such  a  way  that  the  function  log  ©  (vx>  m  +  e)  may  be  regarded  as 
single-valued  on  the  dissected  surface.  Denoting  the  p  zeros  of  ©  (if-  m  +  e) 
by  zl}  ...,  zp,  we  may  suppose  the  dissection  made  by  p  closed  curves  such  as 
the  one  represented  in  Figure  [2],  so  that  a  zero  of  ©  (if-  m  +  e)  is  associated 
with  every  one  of  the  period-loop-pairs.  Then  the  surface  is  still  ^>-ply 
connected,  and  log  ©  (u)  is  single-valued  on  the  surface  bounded  by  the 

Fig.  2. 


p  closed  curves  such  as  the  one  in  the  figure.  For  we  proved  that  a  com 
plete  circuit  of  the  closed  curve  formed  by  the  sides  of  the  (ar,  br)  period- 
loop-pair,  gives  an  increment  of  2m  for  the  function  log  ©  (u) ;  when  the 
surface  is  dissected  as  in  the  figure  this  increment  of  2jri  is  again  destroyed 
in  the  circuit  of  the  loop  which  encloses  the  point  zr.  Any  closed  circuit 
on  the  surface  as  now  dissected  is  equivalent  to  an  aggregate  of  repetitions  of 
such  circuits  as  that  in  the  figure ;  thus  if  x  be  taken  round  any  closed 
circuit  the  value  of  log  ©  (u)  at  the  conclusion  of  that  circuit  will  be  the 
same  as  at  the  beginning.  From  the  formulae 


which  we  express  by  the  statement  that  ©  (u)  has  the  factors  unity  and 
e-^(ur+^r)  for  the  period  loops  ar  and  br  respectively,  it  follows  that  log@(w) 
can,  at  most,  have,  for  opposite  points  of  ar,  br,  respectively,  differences  of 
the  form  ^irigr,  -  2m  (ur  +  %rr,r}  -  2irihr,  wherein  gr  and  hr  are  integers. 
The  sides  of  the  loops  for  which  these  increments  occur  are  marked  in  the 
figure,  ur  denoting  the  value  of  v*' m  +  er  at  the  side  opposite  to  that  where 


254  INVESTIGATION   OF  THE   POSITION  [178 

the  increment  is  marked;  thus  ur  +  ^Tr>r  is  the  mean  of  the  values,  ur  and 
ur  +  Tr,r>  which  the  integral  ur  takes  at  the  two  sides  of  the  loop  br. 

Since   log  ®  (u)  is  now  single- valued,  the   integral  - — .  /  log  ®  (u) .  dus, 

£TTI  J 

taken  round  all  the  p  closed  curves  constituting  the  boundary  of  the  surface, 
will  have  the  value  zero.  Consider  the  value  of  this  integral  taken  round  the 
single  boundary  in  the  figure.  Let  Ar  denote  the  point  where  the  loops 
ar,  br,  and  that  round  zr,  meet  together.  The  contribution  to  the  integral 

arising  from  the  two  sides  of  ar  will  be  I  ffrdv,' m,  this  integral  being  taken 
once  positively  round  the  left  side  of  ar,  from  Ar  back  to  Ar.  This  contri 
bution  is  equal  to  grrr>  „.  The  contribution  to  the  integral  =— .  I  log  ©  (u)  dus 

ATTlJ 

which  arises  from  the  two  sides  of  the  loop  br  is  equal  to 


-  I 


dv] 


,  m 


taken  once  positively  round  the  left  side  of  the  curve  br,  from  Ar  back  to  Ar  ; 
this  is  equal  to 

I  /  x,  m        i  x    7  a;,  m       /        .    7    \  /• 

-  J  (vr     +  i  rr>  r)  dvs      +  (er  +  hr)fr>  ,  , 
where  fr>  s  is  equal  to  1  when  r  =  s,  and  is  otherwise  zero.     Finally  the  part 

i  f 

of  the  integral  =-  -.  I  log  @  (u)  dus,  which  arises  by  the  circuit  of  the  loop 
enclosing  the  point  zr,  from  Ar  back  to  Ar,  in  the  direction  indicated  by  the 
arrow  head  in  the  figure,  is  I  'dv*'  m  where  Ar  denotes  now  a  definite  point  on 

J  Ar 

the  boundary  of  the  loop  br.  If  we  are  careful  to  retain  this  signification  we 
may  denote  this  integral  by  vzsr'  r  .  When  we  add  the  results  thus  obtained, 
for  the  p  boundary  curves,  taking  r  in  turn  equal  to  1,  2,  ...,p,  we  obtain 


r=l 


wherein,  on  the  right  hand,  the  br  attached  to  the  integral  sign  indicates 
a  circuit  once  positively  round  the  left  side  of  br  from  Ar  back  to  Ar  ;  and  if 
kg  denote  the  quantity  defined  by  the  equation 


7  4?       I        /     X>m 

Ks=   21     (Vr 
r=l  J  br 


which,  beside  the  constants  of  the  surface,  depends  only  on  the  place  m, 
we  have  the  result 


179]  OF   THE  ZEROS   OF   RIEMANN'S  THETA   FUNCTION.  255 

179.     Suppose   now   that   places   m1,  ...,  mp   are   chosen   to   satisfy  the 
conruences 


this  is  always  possible  (Chap.  IX.  §§  1G8,  169)  ;  it  is  not  necessary  for  our 
purpose,  to  prove  that  only  one  set*  of  places  ml,  ...,mp,  satisfies  the  con 
ditions  ;  these  places,  beside  the  fixed  constants  of  the  surface,  depend  only 
on  the  place  m.  Then,  by  the  equations  just  obtained,  we  have 

/    Zi,1Tli  Zp,Wlp,  .  _       -.  . 

e,  =  -(v,       +  ......  +vs      p);        (s=l,2,...,p). 

Thus  if  we  express  the  zero  in  the  function  ©  (if>  m  +  e),  it  takes  the  form 

©/  x,  m         Zi.  Wi  Zn.  niv       7   /  , 

(vs     -vs1'    '-  ......  -vsp'    P-hs'-Tsg'), 

where  #/,  ...,  gp',  h{,  .  .  .  ,  hp'  are  certain  integers,  and  this,  by  the  fundamental 
equation  (B),  §  175,  is  equal  to 


z'mp 


-v/'p), 


save  for  the  factor  e-W  <«*"•-«*•"'-  ......  -„*.•*-  4^     This  factor  does  not 

vanish  or  become  infinite.  Hence  we  have  the  result  :  It  is  possible,  corre 
sponding  to  any  place  m,  to  choose  p  places,  ml}  ...,  mp,  whose  position  depends 
only  on  the  position  of  m,  such  that  the  zeros  of  the  function, 

(H)  (<yS,  TO  —  yz,  ,  nti  —  ......  _  vzp,  mp\ 

regarded  as  a  function  of  x,  are  the  places  z1}  .  ..,  zp.  This  is  a  very  funda 
mental  result  f. 

It  is  to  be  noticed  that  the  arguments  expressed  by  vx>  m  —  vZl>  mi—  ...  —  vZp>  m» 
do  not  in  fact  depend  on  the  place  m.  For  the  equations  for  m1}  ...,  mp, 
corresponding  to  any  arbitrary  position  of  m,  were 


mP,Ap  _  j  £     f    ,   x, 

+VS  =/Cs,    =   2,         (Vr 

r=lJ  br 


a  being  an  arbitrary  place.     If,  instead  of  m,  we  take  another  place  /*,  we 
shall,  similarly,  be  required  to  determine  places  fjL1}  ...,  ^p  by  the  equations 


^'Ap^ks,  =  f    !  (,r  +  K,r)^'a, 

r=l  J  br 


*  If  two  sets  satisfy  the  conditions,  these  sets  will  be  coresidual  (Chap.  VIII.,  §  158). 

t  Cf.  Riemann,  Ges.  Werke  (1876),  p.  125,  (§  22).  The  places  mlf  ...  ,  mp  are  used  by  Clebsch 
u.  Gordan  (Abel.  Functional,  1866),  p.  195.  In  Riemann's  arrangement  the  existence  of  the 
solution  of  the  inversion  problem  is  not  proved  before  the  theta  functions  are  introduced. 


256  CASE   WHEN  THE   ZEROS  [179 

thus 

Puttii  up,  mp         S.     i      m,  n  j  x,  a 

v,       +  ......  +<        =2       vr     dvs    ,  = 

r=lJ  br 


r=l 


wherein  fgj  r  =  1  when  r  =  s,  and  is  otherwise  zero,  as  we  see  by  recalling 
the  significance  of  the  br  attached  to  the  integral  sign.  Thus  (Chap.  VIII., 
§  158),  the  places  p,l,  ...,  pp,  m  are  coresidual  with  the  places  mlt  ...,  mp,  /*, 
and  the  arguments 


x,  m         z,,  m,  zp,  TOP 

«      —vs       — —fl 


congruent  to  arguments  of  the  form 


Zp,  ftp 

-vt      . 


The   fact  that  the  places   fi1,  ...,fj,p,m  are  coresidual  with   the  places 
m,i,  ...,  mp,  fji,  which  is  expressed  by  the  equations 

Ui  ,  nil  Mp,  Win  Wl.  M,  ~ 

•T       +  ......  +C       +fls      =0, 

will  also,  in  future,  be  often  represented  in  the  form 


If  the   places  wil5  ...,  mp  are  not  zeros  of  a  ^-polynomial,  this  relation 
determines  /AJ  ,  .  .  .  ,  JJ,P  uniquely  from  the  place  /A. 

Ex.     In  case  j0  =  l,  prove  that  the  relation  determining  m1}  ...,  mp  leads  to 


Hence  the  function  0  (v*-  2  +  ^  +  Jr)  vanishes  for  ^p=z,  as  is  otherwise  obvious. 

180.     The  deductions  so  far  made,  on  the  supposition  that  the  p  zeros  of 
the  function  @  (vz>  m  +  e)  are  distinct,  are  not  essentially  modified  when  this 
is  not  so.     Suppose  the  zeros  to  consist  of  a  jvtuple  zero  at  zlt  a  £>2-tuple  zero 
at  zz  ,  ...,  and  a  ^-tuple  zero  at  z^,  so  that  pl  -f  ......  +pk=P-     The  surface 

may  be  dissected  into  a  simply  connected  surface  as  in  Figure  3.  The 
function  log  ®(vx>m  +  e)  becomes  a  single-  valued  function  of  #  on  the 
dissected  surface  ;  and  its  differences,  for  the  two  sides  of  the  various  cuts, 
are  those  given  in  the  figure.  To  obtain  these  differences  we  remember 
that  log  @  (fl*'  m  +  e)  increases  by  2m  when  x  is  taken  completely  round 
the  four  sides  of  a  pair  of  loops  (ar,  br).  The  mode  of  dissection  of  Fig.  3, 
may  of  course  also  be  used  in  the  previous  case  when  the  zeros  of  ®  (vx>  m  +  e) 
are  all  of  the  first  order. 

The    integral  ^—  .  I  log  ©  (vx>  ™  +  e)  dv*'  m,  taken  along  the  single  closed 

ZiTTI  J 

boundary  constituted  by  the  sides  of  all  the  cuts,  has  the  value  zero.     Its 


180]  ARE   NOT    DISTINCT. 

value  is,  however,  in  the  case  of  Figure  3, 


257 


+pkv 


k'Al 


4-  ffl  f  dvT  m  -  h,  !  dvx;  *  -  1  (tf  m  +  *  +  KI)  dvx;  m  -  (P  -  i)  „ 

J  a\  J  b}  J  6, 


,At 


a. 


dv 


'm-[  (v*' 

J  6, 


r  r  r 

I     j  x'm      7  T  x,  Jtt       /     ,  a;, 

l    ctos     -hpl    dvs     -     (vp 

J  OP  J  bp  J  bp 


wherein  the  first  row  is  that  obtained  by  the  sides  of  the  cuts,  from  Al, 
excluding  the  zeros  zl}  ...,  zk,  and  the  second  row  is  that  obtained  from 
the  cuts  «!,  &j,  d,  and  so  on.  The  suffix  ^  to  the  first  integral  sign  in 


the  second  row  indicates  that  the  integral  is  to  be  taken  once  positively  round 
the  left  side*  of  the  cut  #1,  the  suffix  6j  indicates  a  similar  path  for  the 
cut  6j ,  and  so  on.  If,  as  before,  we  put  kx  for  the  sum 

/      v  r  /  x'm  ,  i     \  j  x>m 

Kg,    =    2,          (Vr       +$Trtr)dvs      , 
r=lJ  br 

we  obtain,  therefore,  as  the  result  of  the  integration,  that  the  quantity 

tl+ +  gprs>  p  +  eK 


*  By  the  left  side  of  a  cut  ax ,  or  fcj ,  is  meant  the  side  upon  which  the  increments  of  log  6  (M) 
are  marked  in  the  figure.     The  general  question  of  the  effect  of  variation  in  the  period  cuts  is 
most  conveniently  postponed  until  the  transformation  of  the  theta  functions  has  been  considered. 
B.  17 


258  THE   THETA    FUNCTION    VANISHES    IDENTICALLY  [180 

is  equal  to 

,  Zi,  A,  zk,  AI        ,  ,  x     A?,  A  ,        ,  £..     A3,  A.,  Ap,  Ap-i 

ks-pivs       -  ......  -JW      +  (p-l)v,        +  (p_2)v8        +  ......  +  V, 

and  this  is  immediately  seen  to  be  the  same  as 


We  thus  obtain,  of  course,  the  same  equations  as  before  (§  179),  save  that 
z1  is  here  repeated  pl  times,  ...,  and  z%  is  repeated  p^  times.  And 
we  can  draw  the  inference  that  ©  (vx>  m  +  e)  can  be  written  in  the  form 
©  (/••  «  _  ^.-  «,  _  ......  _  /,.  »«P  _  /is  _  Ts^  which,  save  for  a  finite  non-vanish 

ing  factor,  is    the    same    as  @(/>m-^"m'-  ......  _/»»w»);    the  argument 

v*'  m  -  /"  m'  -  .  .    .  .  -  vzp'  mp  does  not  depend  on  the  place  m. 

8  S  S  •*•  A 

181.     From  the  results  of  §§  179,  180,  we  can  draw  an  inference  which 
leads  to  most  important  developments  in  the  theory  of  the  theta  functions. 

For,  from  what  is  there  obtained  it  follows  that  if  zl,  ...,  zp  be  any  places 
whatever,   the   function   ®(vx'm  -  vZi'mi  -  ......  _^'m»)   has   zlt  ...,  zp   for 

zeros.     Hence,  putting  zp  for  x  we  infer  that  the  function 


vanishes  identically  for  all  positions  of  zl}  ...,  %_j.     Putting 

/2i,?«i    .  Zp-2,  Wu-2         m.n.m, 

>=VS          +  ......  +VS 


-V 


for  s=  1,  2,  ...,  p,  this  is  the  same  as  the  statement  that  the  function 
(S)  (vx>  in>>-1  +  f)  vanishes  identically  for  all  positions  of  a;  and  for  all  values 
of/j,  ...,fp  which  can  be  expressed  in  the  form  arising  here.  When/,  ...,/, 
are  arbitrary  quantities  it  is  not  in  general  possible  to  determine  places 
zl}  ...,Zp_2  to  express/,  ...,/,  in  the  form  in  question.  Nevertheless  the 
case  which  presents  itself  reminds  us  that  in  the  investigation  of  the  zeros 
of  <H)  (if'  m  +  e)  we  have  assumed  that  the  function  does  not  vanish  identically, 
and  it  is  essential  to  observe  that  this  is  so  for  general  values  of  els  ...,  ep. 
If,  for  a  given  position  of  x,  the  function  ®  (^  m  +  e)  vanished  identically  for 
all  values  of  ely  ...,  ep,  the  function  @  (r)  would  vanish  for  all  values  of  the 
arguments  rlt  ...,  rp.  We  assume*  from  the  original  definition  of  the  theta 
function,  by  means  of  a  series,  that  this  is  not  the  case. 

Further  the  function  @  (vx>  m  +  e)  is  by  definition  an  analytical  function  of 
each  of  the  quantities  e1}  ...,  ep  ;   and  if  an  analytical  function  do  not  vanish 

*  The  series  is  a  series  of  integral  powers  of  the  quantities  e2irir',  ____  e'mrp_ 


182]  FOR   CERTAIN    FORMS   OF   THE    ARGUMENT.  259 

for  all  values  of  its  argument,  there  must  exist  a  continuum  of  values  of 
the  argument,  of  finite  extent  in  two  dimensions,  within  which  the  function 
does  not  vanish*.  Hence,  for  each  of  the  quantities  ely  ...,ep  there  is  a 
continuum  of  values  of  two  dimensions,  within  which  the  function  @  («*>  m  +  e) 
does  not  vanish  identically.  And,  by  equation  (B),  §  175,  this  statement 
remains  true  when  the  quantities  e1}  ...,ep  are  increased  by  any  simultaneous 
periods.  Restricting  ourselves  then,  first  of  all,  to  values  of  e1}  ...,  ep  lying 
within  these  regions,  there  exist  (Chap.  IX.  §  168)  positions  of  zl}  ...,  zp  to 
satisfy  the  congruences 


and,  since  to  each  set  of  positions  of  zl}  ...,  zp,  there  corresponds  only  one  set 
of  values  for  elf  ...,  ep>  the  places  zlt  ...,  zp  are  also,  each  of  them,  variable 
within  a  certain  two-dimensionality.     Hence,  within  certain  two-dimensional 
limits,  there  certainly  exist  arbitrary  values  of  zlt  ...,  zp  such  that  the  function 
®(v*'m  -vz"m>  -  ......  _w*>«*)    does   not    vanish    identically.      For   such 

values,   and   the   corresponding   values   of  elt   ...,   ep,  the   investigation  so 
far    given    holds    good.      And    therefore,    for    such    values,    the    function 
®  (vm»<  '«_/..'«._  ......  _  ^P-I,  mp-i)  vanishes  identically.     Since  this  function 

is  an  analytical  function  of  the  placesf  ^,  ...,  zp_lt  and  vanishes  identically 
for  all  positions  of  each  of  these  places  within  a  certain  continuum  of  two 
dimensions,  it  must  vanish  identically  for  all  positions  of  these  places. 

Hence  the  theorem  (F)  holds  without  limitation,  notwithstanding  the 
fact  that  for  certain  special  forms  of  the  quantities  elt  ...,ep,  the  function 
<H)  (^  m  +  e)  vanishes  identically.  The  important  part  played  by  the  theorem 
(F)  will  be  seen  to  justify  this  enquiry. 

J82.  It  is  convenient  now  to  deduce  in  order  a  series  of  propositions  in 
regard  to  the  theta  functions  (§§  182—188);  and  for  purposes  of  reference 
it  is  desirable  to  number  them. 

(I.)    If  £1;  ...,%p  be  p  places  which  are  zeros  of  one  or  more  linearly 
independent  ^-polynomials,  that  is,  of  linearly  independent  linear  aggregates 
of  the  form  XIHI(«)+  ......  +  \p£lp(x)  (Chap.  II.  §  18,  Chap.  VI.  §  101),  then 

the  function 


vanishes  identically  for  all  positions  of  x. 

For  then,  if  r  +  1  be  the  number  of  linearly  independent  ^-polynomials 
which  vanish  in  the  places  £,,...,£,,  we  can,  taking  r  +  1  arbitrary  places 

*  E.g.  a  single-valued  analytical  function  of  an  argument  2,  =x  +  iy,  cannot  vanish  for  all 
rational  values  of  x  and  y  without  vanishing  identically. 

t  By  an  analytical  function  of  a  place  2  on  a  Riemann  surface,  is  meant  a  function  whose 
values  can  be  expressed  by  series  of  integral  powers  of  the  infinitesimal  at  the  place. 

17—2 


260                                                   SUMMARY   OF   RESULT.  [182 

zl}  ...,  zT+l,  determine  p—  r—  1  places  zT+2,  ...,  zp,  such  that  (zlt  ...,  zp) 
=  (&,  ...,£P)  (see  Chap.  VI.  §  93,  etc.,  and  for  the  notation,  §  179).  Then  the 
argument 

t?>  m  _  7,f"  m>  _                  _Jp>mP  (<i  —  ~(      2              V\ 

Us        —  Vg                 —  Vg           >  V6  ~~  L>  ^>  • '  • '  P/> 

can  be  put  in  the  form 


save  for  integral  multiples  of  the  periods  ;  thus  (§§  179,  180)  the  theta 
function  vanishes  when  a;  is  at  any  one  of  the  perfectly  arbitrary  places 
zlt  ...,  ZT+I.  Thus,  since  by  hypothesis  r+  1  is  at  least  equal  to  1,  the  theta 
function  vanishes  identically. 

It  follows  from  this  proposition  that  if  z2',  ...,  zp'  be  the  remaining  zeros 
of  a  (^-polynomial  determined  to  vanish  in  each  of  z2,  ...,zp,  and  neither 
x  nor  z-i  be  among  z2'>  •  •  •  >  Zp,  then  the  zeros  of  the  function 


regarded  as  a  function  of  zlt  are  the  places  x,  zj  ,  ...,  zp. 

From  this  Proposition  and  the  results  previously  obtained,  we  can  infer 
that  the  function  ®(v*'m  —  vZl'm>  —  ......  —vz>>'m")   vanishes   only  (i)   when   a; 

coincides  with  one  of  the  places  zl}  ...,  zp,  or  (ii)  when  zlt  ...,  zp  are  zeros  of 
a  ^-polynomial. 

(II.)  Suppose  a  rational  function  exists,  of  order,  Q,  not  greater  than  p, 
and  let  T  +  1  be  the  number  of  (^-polynomials  vanishing  in  the  poles  of  this 
function.  Take  r  +  1  arbitrary  places 

Sl)   •••>  b<?>  «^i>   •••»  ^T+l—qy 

wherein  q=  Q  —  p  +r+l,  and  suppose  zlt  ...,  z(t  to  be  a  set  of  places  core- 
sidual  with  the  poles  of  the  rational  function,  of  which,  therefore,  q  are 
arbitrary.  Then  the  function 


_  _  yZq+l  ,  »«T+2-q  _   ^       _  _  _  ^Z«>  mt>-Q\ 

vanishes  identically. 

For  if  we  choose  £q+l,  ...,  %Q  such  that  (%lt  ...,  £e)  =  (zlt  ...,  ZQ),  the 
general  argument  of  the  theta  function  under  consideration  is  congruent 
to  the  argument 

nip,  m        xl,m1  av-t-i-g.  mT+i-q         q+i,  mr+z-q  Q,  mp-q 


This  value  of  the  argument  is  a  particular  case  of  that  occurring  in 
(F),  §  181,  the  last  q—  1  of  the  upper  limits  in  (F)  being  put  equal  to  the 
lower  limits.  Hence  the  proposition  follows  from  (F). 


182]  A    PARTICULAR   FORM    OF   THE    INVERSION    PROBLEM.  261 

(III.)  If  r  denote  such  a  set  of  arguments  r,,  ...,  rp  that  0  (r)  =  0,  and, 
for  the  positions  of  z  under  consideration,  the  function  ®  (vx>  z  +  r)  does  not 
vanish  for  all  positions  of  as,  then  there  are  unique  places  zlt  ...,  ^_1( 
such  that 

r  -  ymp,  m  _  vzt  ,  mt  _  ^      ^  _  rfp-i,  mp-i 

In  this  statement  of  the  proposition  a  further  abbreviation  is  introduced 
which  will  be  constantly  employed.  The  suffix  indicating  that  the  equation 
stands  as  the  representative  of  p  equations  is  omitted. 

Before  proceeding  to  the  proof  it  may  be  remarked  that  if  m',  m/,  ...,mp' 
be  places  such  that  (cf.  §  179) 

(m',  m1}  ...,  mp)  =  (m,  w/,  ...,  mp'} 
and  therefore,  also, 


then  the  equation 


ym',  7/1  _  vm,',  »«i  _  ^      ^  _  vm,,',  m,, 


r  =  vm>"  m 


is  the  same  as  the  equation 


r  =  v 


This  proposition  (III.)  is  in  the  nature  of  a  converse  to  equation  (F). 
Since  the  function  @  (vx'  z  -f  r)  does  not  vanish  identically,  its  zeros,  z1}  ...,  zp, 
are  such  that 

vx'z+r=vx'm-vZt'Wl-  ......  _/"•'«"; 

now  we  have 

vz»  m'  +  vz»>  mp  =  vz»-  '"'  +  vz»  m" 

so  that  the  zeros  zlt  ...,  zp  may  be  taken  in  any  order  ;  since  ®  (r)  vanishes, 
z  is  one  of  the  zeros  of  %  (vx>  z  +  r);    hence,  we  may  put  zp  =  z,  and  obtain 


r  =     .       _    '•    . 

_     m,,,  m         zlt  m, 


which  is  the  form  in  question. 

If  the  places  zlt  ...,zp_l  in  this  equation  are  not    unique,  but,  on   the 
contrary,  there  exists  also  an  equation  of  the  form 


r  =  v™1"  m  —  v*1 
then,  from  the  resulting  equation 


262  A    PARTICULAR   FORM  [182 

we  can  (Chap.  VIII.  §  158)  infer  that  there  is  an  infinite  number  of  sets  of 
places  Zi,  ...,  z'p-!,  all  coresidual  with  the  set  zl}  ...,  zp_-^  ;  hence  we  can  put 


wherein  at  least  one  of  the  places  z^,  .  .  .  ,  zfp^l  is  entirely  arbitrary.  Then  the 
function  ©  (vx>  z  +  r)  vanishes  for  an  arbitrary  position  of  x,  that  is,  it 
vanishes  identically  ;  this  is  contrary  to  the  hypothesis  made. 

It  follows  also  that  whenever  it  is  possible  to  find  places  ^  ,  .  .  .  ,  zp^l  to 
satisfy  the  inversion  problem  expressed  by  the  p  equations 


the  function  ©  (vm>"  m  —  u)  vanishes  ;  conversely,  when  u  is  such  that  this 
function  vanishes  we  can  solve  the  inversion  problem  referred  to. 

(IV.)  When  r  is  such  that  ©  (r)  vanishes,  and  ©  (vx>  z  +  r)  does  not, 
for  the  values  of  z  considered,  vanish  identically  for  all  positions  of  a,  the 
zeros  of  ©  (vx>  z  +  r),  other  than  z,  are  independent  of  z  and  depend  only  on 
the  argument  r. 

This  is  an  immediate  corollary  from  Proposition  (III.)  ;  but  it  is  of 
sufficient  importance  to  be  stated  separately. 

(V.)  If  ©  (r)  =  0,  and  ©  (vx>  z  +  r)  vanish  identically  for  all  positions 
of  x  and  z,  but  ©  (vx<  z  4-  tf'  ^  +  r)  do  not  vanish  identically,  in  regard  to  x, 
for  the  positions  of  z,  £,  %  considered,  then  it  is  possible  to  find  places 


z1}  ...,  Zp-2  such  that 


m"'  m  —   Zl'  m' 


and  these  places  z1)  ...,  Zp_,,  are  definite. 
Under  the  hypotheses  made,  we  can  put 


r  = 


wherein  zlt  .  .  .  ,  zp  are  the  zeros  of  ©  (if-  z  +  v*'  *  +  r)  ;  now  z  is  clearly  a  zero  ; 
for  the  function  ©  (v*'*+  r)  is  of  the  same  form  as  ©  (v*>z  +  r),  and  vanishes 
identically;  and  fis  also  a  zero;  for,  putting  ffor#,  the  function  ®(vx'z+vt>t+r) 
becomes  ©  (v*  >  z  +  r),  which  also  vanishes  identically.  Putting,  therefore,  f,  z 
for  ,Zp_i  and  zp  respectively,  the  result  enunciated  is  obtained,  the  uniqueness 
of  the  places  zl}  ...,  Zp_2  being  inferred  as  in  Proposition  (III.). 

We  may  state  the  theorem  differently  thus  :  If  ©  (vx>  z  +  r)  vanish  for 
all  positions  of  x  and  z,  and  @  (vx>  z  +  v*>  *  +  r)  do  not  in  general  vanish 
identically,  the  equations 


r  =  v 


182]  OF   JACOBI'S    INVERSION    PROBLEM.  263 

can  be  solved,  and  in  the  solution  one  of  z1}  .  ..,  Zp__^  may  be  taken  arbitrarily, 
and  the  others  are  thereby  determined.  Hence  also  we  can  find  places 
Zi,  ...,  z'p-i,  other  than  z1}  ...,  zp_l,  such  that 


one  of  the  places  £/,  ...,  z'p_l  being  arbitrary.  Hence  by  the  formula 
Q-q  =  p  —  T  —  1,  putting  Q=p—lt  q=l,  we  infer  r+l=2,  so  that  a 
0-polynomial  vanishing  in  zlt  ...,  zp^  can  be  made  to  vanish  in  the  further 
arbitrary  place  z.  Thus,  when  ©  («*>  z  +  r)  vanishes  identically,  we  can  write 

/•  *  +  r  =  v*>  "<  _  /..  «».  _  ......  _  ^'->.  «P-«  _  /•  »* 

wherein  the  places  ^,  ...,  ^_1}  z  are  zeros  of  a  ^-polynomial  (cf.  Prop.  I.). 

(VI.)     The    propositions   (III.)   and   (V.)   can   be   generalized   thus  :    If 
©  (vx>'Zt  +  ......  +  vx"'Zq  +  r)  be  identically  zero  for  all  positions  of  the  places 

xl,zl,  ...,xq,  zq,  and  the  function  ©  (vx'z  +  vx"z'  +  ......  +vx<i'z''  +  r)  do   not 

vanish  identically  in  regard  to  x,  then  places  £i,  ...,  ^p_l  can  be  found  to 
satisfy  the  equations 


r  =  v 


and,  of  these  places,  q  are  arbitrary,  the  others  being  thereby  determined. 

These  arbitrary  places,  £,,  ...,  %q,  say,  must  be  such  that  the  function 
©  (/'  s  +  /"  Zl  +  ......  +  v*"'  Zq  +  r)  does  not  vanish  identically. 

For  as  before  we  can  put 


,  z 


wherein  ^  ,  .  .  .  ,  fp  are  the  zeros  of  the  function  ©  (vx>  z  +  v*1'  Zl  +  .  .  .  +  v*"  Zq  +  r). 
It  is  clear  that  z  is  one  zero  of  this  function  ;  also  putting  z1  for  x  the  function 
becomes  @  (vx"z  +  tf"  2s  +  ......  +  wx"  Zq  +  r),  which  vanishes,  by  the  hypothesis. 

Thus  the  places  z,  z1}  ...,  zq  are  all  zeros  of  the  function 


Putting  then  z,,  ...,  gq,  z  respectively  for  f,,  ...,  £q,  £p  in  the  congruence 
just  written,  it  becomes 


and  this  is  the  same  as 


replacing  #1,  ....  a;7  by  £,,...,  f,  we  have  the  result  stated. 


264  PROPERTIES   OF   THE    PLACES  [182 

Hence  also,  we  can  tiud  places  £/,  .  ..,  £p-l}  other  than  £1;  ...,  ^p_l,  such 
that 


q  of  the  places  £/,  ...,  £'p-i  being  arbitrary.  Therefore  a  (^-polynomial  can 
be  chosen  to  vanish  in  ^  ,  .  .  .  ,  ^p_1  and  in  q  (=  p  —  1  —  (Q  —  q),  when  Q=p—  1) 
other  arbitrary  places.  Thus  the  argument 


for  which  the  theta  function  vanishes  identically,  can  be  written  in  the  form 


>  m» 


wherein  .Zj,  ...,zq_l}  ^IJt  .  ..,  %P-I>  z  are  zeros  of  q+l  linearly  independent 
(^-polynomials. 

(VII.)     If  the  function  ©  (/"  Zl  +  ......  +  vx"'  Zl'  +  r)  be  identically  zero  for 

all  positions  of  the  places  x1,  zly  x2,  z2,  ...,  xq,  zq,  and,  for  general  positions  of 
aslt  z,,   ...,  seq,   zq,   the   function    @  (/'  z  +  v*1'  z>  +  ......  +vx"'Zq+r)   be    not 

identically  zero,  as  a  function  of  x,  for  proper  positions  of  z,  and  be  not 
identically  zero,  as  a  function  of  z,  for  proper  positions  of  x,  then  we  can  find 
places  £i,  ...,  £p-lt  of  which  q  places  are  arbitrary,  such  that 


and  can  also  find  places  £1}  ...,  £p_i,  of  which  q  places  are  arbitrary,  such 
that 

—  r  =  vmp>  m  —  v*1  '  m'  —       .  .  —  v*1"  lf  m"'\ 

This  is  obvious  from  the  last  proposition,  if  we  notice  that 


We  can  hence  infer  that 

2vmp'  m  +  vmi'^  +  vmi'*l  +  ......  -f  v"1"-1'  &~1  +  vmp~1'  fp~1  =  0, 

and  this  is  the  same  (Chap.  VIII.  §  158)  as  the  statement  that  the  set  of 
2p  places  constituted  by  &,...,  %p-i,  &,  ...,  ^,_i  and  the  place  m,  repeated,  is 
coresidual  with  the  set  of  2p  places  constituted  by  the  places  m^,  ...,  mp,  each 
repeated.  This  result  we  write  (cf.  §  179)  in  the  form 

(m2,  £,  ...  ,  ^_1}  f,,  ...,  ^j)  =  (m^,  mj,  ...,  m/}. 

(VIII.)     We  can  now  prove  that  if  £,  ...,  ^_j  be  arbitrary  places,  places 
£1}  ...,  £p_j  can  be  found  such  that 

(m2,  f  !,...,  fp_i,  ?!,...,  fp-O  =  (wh3,  w22,  ...,  wip3). 
Let  r  denote  the  set  of  j9  arguments  given  by 


182]  mlt  nit,  ...,  mp.  265 

£i>  •••>  £p-i  being  quite  arbitrary.     Then,  by  theorem  (F),  (§  181),  the  function 
®  (r)  certainly  vanishes.     It  may  happen  that  also  the  function  ®  (vx-  z  +  r) 
vanishes  identically  for  all  positions  of  #  and  z.     It  may  further  happen  that 
also  the  function  S  («*•  z  +  if1'  Zi  +  r)  vanishes  identically  for  all  positions  of 
x,  z,  #!,  z1.     We  assume*  however  that  there  is  a  finite  value  of  q  such  that 
the  function  ©  (vx'  z  +  vx>'Zl  +  ......  +  /'"  *  +  r)  does  not  vanish  identically  for 

all  positions  of  x,  z,  aslt  zl}  .  ..,  xq,  zq.     Then  by  Proposition  VII.  it  follows 
that  we  can  find  places  £lf  ...,  gp_lt  such  that 


—  r  =  v 


=   ™1" 


comparing  this  with  the  equations  defining  the  argument  r,  we  can,  as 
in  Proposition  (VII.)  infer  that  the  congruence  stated  at  the  beginning  of 
this  Proposition  also  holds. 

(IX.)  Hence  follows  a  very  important  corollary.  Taking  any  other 
arbitrary  places  £/,  ...,  ^'p-lt  we  can  find  places  £/,  ...,  ^'^  such  that 

(m2,  £',  ...,  f'^,  £/,  ...,  £'^)  =  (m*,  m22,  ...,  m/); 

therefore  the  set  £,  ...,  ^p_lt  £,  ....f^  is  coresidual  with  the  set  £',  ...,^_1, 
£/>  •••»  ^"p-i-  Now,  of  a  set  of  2p  —  2  places  coresidual  with  a  given  set 
we  can  in  general  take  only  p  —  2  arbitrarily  ;  when,  as  here,  we  can  take 
p  —  1  arbitrarily,  each  of  the  sets  must  be  the  zeros  of  a  ^-polynomial 
(Chap.  VI.  §  93).  Thus  the  places  £,  ...,  £,_,,  £,  ...,  ^  are  zeros  of  a 
</>-polynomial. 

Therefore,  if  a1}  ...,  O2p_2  be  the  zeros  of  any  ^-polynomial  whatever, 
that  is,  the  zeros  of  the  differential  of  any  integral  of  the  first  kind,  the 
places  m^,  ...  ,  mp  are  so  derived  from  the  place  m  that  we  have 


(w2,  a1}  .  .  .  ,  a2i,_2)  =  (m,-,  w22,  .  .  .  ,  m/),  (G)  ; 

in  other  words,  if  c1}  .  .  .  ,  cp  denote  any  independent  places,  the  places  ma,        mp 
satisfy  the  equations 

2  /''  '  Cl  +  ......  +  v™>"  e"  =  2l)  c"      "1'  c>1         '  Cl  *2p-3'  Cp       "2"-2'  c" 


for  s  =  1,  2,  .  .  .  ,  p.  Denoting  the  right  hand,  whose  value  is  perfectly  definite, 
by  Ag,  and  supposing  ffl,  ...,  ffpt  h,,  ...,  hp  to  denote  proper  integers,  these 
equations  are  the  same  as 

C'C'  +  ......  +  C>Cj>=^.  +  H*.  +  flriT.|1  +  ......  +ffPT.,p),        (G'), 

where  8=1,  2,  ...,p. 

*  It  will  be   seen   in   Proposition   XIV.   that  if  0  (v*>  z+vx»  z'  +  ......  +vx*<z'  +  r)   vanishes 

identically,  then  all  the  partial  differential  coefficients  of  9  (M),  in  regard  to  i^,  ...  ,  up,  up  to  and 
including  those  of  the  (q  +  l)th  order,  also  vanish  for  u  =  r. 


266  GEOMETRICAL    INTERPRETATION  [182 

There  are  however  2'-*  sets  of  places  -m^,  ...,mp,  corresponding  to  any 
position  of  the  place  m,  which  satisfy  the  equation*  (G).  For  in  equations 
(G')  there  are  22^  values  possible  for  the  right-hand  side  in  which  each 
of  (ft,  . .. ,  gp,  hlt  . ..,  hp  is  either  0  or  1,  and  any  two  sets  of  values  glt  ...,  gp, 
h1}  ...,  hp  and  #/,  ...,  gp',  A/,  ...,  hp',  such  that  g^g{ differ  by  an  even  integer, 
and  hi,  A/  differ  by  an  even  integer,  for  i  =  l,  2,  ...,p,  lead  to  the  same 
positions  for  the  places  mlt  ...,  mp.  (Chap.  VIII.  §  158.) 

We  have  seen  (§  179)  that  the  places  m1}  ...,mp  depend  only  on  the  place 
m  and  on  the  mode  of  dissection  of  the  Riemann  surface.  We  are  to  see, 
in  what  follows,  that  the  22p  solutions  of  the  equation  (G)  are  to  be  associated, 
in  an  unique  way,  each  with  one  of  the  2-p  essentially  distinct  theta  functions 
with  half  integer  characteristics. 

183.  The  equation  (G)  can  be  interpreted  geometrically.  Take  a  rion- 
adjoint  polynomial,  A,  of  any  grade  /JL,  which  has  a  zero  of  the  second  order 
at  the  place  m  ;  it  will  have  tip  —  2  other  zeros.  Take  an  adjoint  polynomial 
>|r,  of  grade  (n  —  1)  0  +  n—  3  +  p,  which  vanishes  in  these  other  n/j,—  2  zeros 
of  A.  Then  (Chap.  VI.  §  92,  Ex.  ix.)  ^  will  be  of  the  form  X^0  +  A<£, 
where  i/r0  is  a  special  form  of  ty,  A,  is  an  arbitrary  constant,  and  <f>  is  a 
general  (^-polynomial.  The  polynomial  i/r  will  have  Zp  zeros  other  than 
those  prescribed  ;  denote  them  by  klt  . . . ,  k.^.  If  </>'  be  any  ^-polynomial,  with 
a1} ...,  a2p-2  as  zeros,  we  can  form  a  rational  function,  given  by  (Xi/r0+A</>)/A<£', 
whose  poles  are  the  places  al,  ...,  a^-z,  together  with  the  place  m  repeated, 
its  zeros  being  the  places  kl}  ...,  kzp.  Hence  (Chap.  VI.  §  96)  we  have 

\ni~,  a>i,  ...,  a.2p—2)^(K1,  **  '••>  "'zp— 1>  kzp), 
and  therefore,  by  equation  (G), 

(nij1,  ... ,  mp-}  =  (&j ,  ki, ...,  £sp_i ,  k2p)  (G") ; 

hence  (Chap.  VI.  §  90)  it  is  possible  to  take  the  polynomial  -fy  so  that 
its  zeros  kly  ...,  k2p  consist  of  p  zeros  each  of  the  second  order,  and  the 
places  nil,  ...,  mp  are  one  of  the  sets  of  p  places  thus  obtained. 

There  are  22p  possible  polynomials  ty  which  have  the  necessary  character, 
as  we  have  already  seen  by  considering  the  equation  (G');  but,  in  fact, 
a  certain  number  of  these  are  composite  polynomials  formed  by  the  product 
of  the  polynomial  A  and  a  ^-polynomial  of  which  the  2p  —  2  zeros  consist  of 
p  -  1  zeros  each  repeated.  To  prove  this  it  is  sufficient  to  prove  that  there 
exist  such  ^-polynomials  having  only  p  —  1  zeros,  each  of  the  second  order ; 
for  it  is  clear  that  if  <£  denote  such  a  polynomial,  the  product  A<I>  is  of  grade 

*  If  for  any  set  of  values  for  gl ,  . . . ,  gp ,  /ij ,  . . . ,  hp  the  equations  (G')  are  capable  of  an  infinity 
of  (coresidual)  sets  of  solutions,  the  correct  statement  will  be  that  there  are  22P  lots  of  coresidual 
sets,  belonging  to  the  place  m,  which  satisfy  the  equation  (G).  The  corresponding  modification 
may  be  made  in  what  follows. 


184]  OF   THESE   PLACES.  267 

(ft  —  l)a  +  n  —  3  +  /u,  and  satisfies  the  conditions  imposed  on  the  polynomial  -ty. 
That  there  are  such  (^-polynomials  <I>  is  immediately  obvious  algebraically. 
If  we  form  the  equation  giving  the  values  of  x  at  the  zeros  of  the  general 
(^-polynomial, 


the  p  —  1  conditions  that  the  left-hand  side  should  be  a  perfect  square,  will 
determine  the  necessary  ratios  Xj  :  X2  :  ...  :  \p,  and,  in  general,  in  only  a 
finite  number  of  ways.  (Cf.  also  Prop.  XL  below.) 

It  is  immediately  seen,  from  equation  (G"),  that  if  m^  ,  ...,  mp  be  the 
double  zeros  of  one  such  polynomial  -fy-  as  described,  and  w/,  .  .  .  ,  mp'  of 
another,  both  sets  being  derived  from  the  same  place  ra,  then 

vmt''mt  +  ......  +  /'"''  ""'  =  |  flPi  .  ,  (H) 

where  £Lpt  tt  stands  for  p  quantities  such  as 


«n  •••»  «?>  A.  •••!  $p  being  integers. 

We  may  give  an  example  of  the  geometrical  relation  thus  introduced,  which  is  of  great 
importance.     It  will  be  sufficient  to  use  only  the  usual  geometrical  phraseology. 

Suppose  the  fundamental  equation  is  of  the  form 

;/)i  +  (x,  y)jj  +  (x,  y)3  +  (#,  y\  =  0, 


representing  a  plane  quartic  curve  (p  =  3).  Then  if  a  straight  line  be  drawn  touching  the 
curve  at  a  point  m,  it  will  intersect  it  again  in  2  points  A,  B.  Through  these  2  points 
A,  J3,  oo  3  conies  can  be  drawn  ;  of  these  conies  there  are  a  certain  number  which  touch 
the  fundamental  quartic  in  three  points  P,  Q,  R  other  than  A  and  B.  There  are  22*  =  64 
sets  of  three  such  points  I1,  Q,  R  ;  but  of  these  some  consist  of  the  two  points  of  contact 
of  double  tangents  of  the  quartic  taken  with  the  point  m  itself. 

In  fact  there  are  (Salmon,  Higher  Plane  Curves,  Dublin,  1879,  p.  213)  28,  =  2»-1(2p-l), 
double  tangents  ;  these  do  not  depend  at  all  on  the  point  m  ;  there  are  therefore 
36,  =2"-1(2''4-l),  proper  sets  of  three  points  P,  Q,  R  in  which  conies  passing  through 
A  and  B  touch  the  curve.  One  of  these  sets  of  three  points  is  formed  by  the  points 
wij,  m2,  m3.  It  has  been  proved  that  the  numbers  2"  -1  (2"-  1),  2^~J  (2^+1)  are  respectively 
the  numbers  of  odd  and  even  theta  functions  of  half  integer  characteristics  (§  176). 

184.  (X.)  We  have  seen  in  Proposition  (VIII.)  (§  182)  that  the  places 
Wj  ,  .  .  .  ,  mp  are  one  set  from  2s*  sets  of  p  places  all  satisfying  the  same 
equivalence  (G).  We  are  now  to  see  the  interpretation  of  the  other  22^  —  1 
solutions  of  this  equation. 

Let  w/,  ...,mp'  be  any  set,  other  than  ml}  ...,mp,  which  satisfies  the 
congruence  (G).  Then,  by  equations  (G'),  we  have 

2  «"''""  +  ......  +<"'-'"")^0.  (*=1,2,  ...,p), 


268  THE    2^   POSSIBLE    POSITIONS.  [184 

and  therefore,  if  H^>0  denote  the  set  of  p  quantities  of  which  a  general  one  is 
given  by 

&  +  aiT*,i  4-  ......  +<*PTgjp>  (s  =  l,  2,  ...,p), 

where  a1}  ...,  ap,  @i,  ...,  &p  are  certain  integers,  we  have 

Mil',  »»,  mp,  ma        !    .-. 

vs         +  ......  +v,p     P=^n^a; 

hence  the  function 


=  e®*  ©  (vz< ' mi' 
where 
the  function  is  therefore  equal  to 


,m,p         x,  m  /         -i     c\  \ 

P-w      ,         (s  =  l,  2,  ...,_p); 


by  equation  (C),  §  175  ;  thus  the  function  ®(vx'  m-vz»m>  -  ......  -  vz">  '""'  , 

vanishes  when  x  is  at  either  of  the  places  z1,  ...,  zp. 

We  can  similarly  prove  that 


It  has  been  remarked  (§  175)  that  there  are  effectively  22^  theta  functions, 
corresponding  to  the  2^  sets  of  values  of  the  integers  a,  /3  in  which  each 
is  either  0  or  1.  The  present  proposition  enables  us  to  associate  each  of 
the  functions  with  one  of  the  solutions  of  the  equivalence  (G).  When  the 
function  ®  (vx>  m  ;  ^(3,  ^a)  does  not  vanish  identically  in  respect  to  x,  its 
zeros  are  the  places  m/,  ...,  mp'  '.  Therefore,  instead  of  the  function  ©  (u), 
we  may  regard  the  function  ®(u;  £/3,  ^a)  as  fundamental,  and  shall  only  be 
led  to  the  places  m^,  ...,  mp',  instead  of  m1}  ...,mp. 

(XL)  The  sets  of  places  m/,  .  .  .  ,  mp  which  are  connected  with  the  places 
m1}  ...,  nip  by  means  of  the  equations 


wherein  a1}  ...,  ap,  {3lt  ...,  /3P  denote  in  turn  all  the  22p  sets  of  values  in  which 
each  element  is  either  0  or  1,  may  be  divided  into  two  categories,  according 
as  the  integer  /3a,  =  fti^  +  ......  +  @pap  ,  is  even  or  odd.     We  have  remarked, 

in  Proposition  (IX.),  that  they  may  be  divided  into  two  categories  according 
as  they  are  the  zeros,  of  the  second  order,  of  a  proper  polynomial  X-^0  +  A</>, 
or  consist  of  the  p  —  1  zeros,  each  of  the  second  order,  of  a  ^-polynomial 
together  with  the  place  m.  When  the  fundamental  Riemann  surface  is 
perfectly  general  these  two  methods  of  division  of  the  22^  sets  entirely  agree. 
When  /3a  is  odd,  m^,  .  .  .  ,  mp'  consist  of  the  place  m  and  the  p  -  1  zeros, 
each  of  the  second  order,  of  a  ^-polynomial.  When  /3a  is  even,  m/,  .  .  .  ,  mp' 


184]  ODD   AND   EVEN   CHARACTERISTICS.  269 

consist  of  the  zeros,  each  of  the  second  order,  of  a  proper  polynomial  >/r.  In 
the  latter  case  we  may  speak  of  the  places  ?»/,  .  .  .  ,  mp'  as  a  set  of  tangential 
derivatives  of  the  place  m. 

For  by  the  equations  (D),  (A),  (§  175),  we  have 

e,iau  (B)  Qft^  B  +  M)/g-«-u  (H)  Qft^  a  _  w)  =  e-nifia  . 

hence,  when  /3<z  is  odd,  eniau  ®  (^flftt  a  +  u)  is  an  odd  function  of  u,  and 
must  vanish  when  u  is  zero;  since  then  ®  (|n^a)  vanishes,  there  exist,  by 
Proposition  (VII.),  places  nl}  ...,  np_l}  such  that 


or 


Hence  (Chap.  VIII.  §  158)  we  have 

(m2,  w,2,  ...,  ny,)  =  (m,2,  ...,  m/), 

so  that,  by  equation  (G),  the  places  nlt  ...,  wp_,  are  the  zeros  of  a  ^-polynomial, 
each  being  of  the  second  order. 

When  pa.  is  even,  the  function  e™u  ®  (£O0,  a  +  u}  is  an  even  function,  and 
it  is  to  be  expected  that  it  will  not  vanish  for  u  =  0.  This  is  generally  the 
case,  but  exception  may  arise  when  the  fundamental  Riemann  surface  is  of 
special  character.  We  are  thus  led  to  make  a  distinction  between  the  general 
case,  which,  noticing  that  ®  (%&?,*  +  u)  is  equal  to  e~iria(u+^~^Ta}  ®  (u  ;  £/3,  £a), 
may  be  described  as  that  in  which  no  even  theta  function  vanishes  for  zero 
values  of  the  argument,  and  special  cases  in  which  one  or  more  even  theta 
functions  do  vanish  for  zero  values  of  the  argument. 

Suppose  then,  firstly,  that  no  even  theta  function  vanishes  for  zero  values 
of  the  argument.  Then  if  w/,  ...,  np_^  be  places  which,  repeated,  are  the 
zeros  of  a  ^-polynomial,  we  have 

(m2,  w/2,  .  .  .  ,  M/ap_i)  =  0»,s,  ™22,  •  •  •  ,  ?V)  5 
hence  the  argument 


is  a  half-period,  =  -  £ft/r,  a',  say.  Thus,  by  the  result  (F),  @  (^^Vy)  is  zero  ; 
therefore,  by  the  hypothesis  pet  is  an  odd  integer.  So  that,  in  this  case, 
every  odd  half-period  corresponds  to  a  </>-polynomial  of  which  all  the  zeros 
are  of  the  second  order,  and  conversely. 

Further,  in  this  case  it  is  immediately  obvious  that  the  places  TW,,  ...,  mp 
do  not  consist  of  the  place  m  and  the  zeros  of  a  ^-polynomial  whose  zeros  are 
of  the  second  order  ;  for  if  mlt  ...,mp  were  the  places  n,,  ...,  np_lt  m,  then,  by 

the  result  (F),  the  function  ©  (vz"n'  + +  /"-'• ""-')  would  vanish  for  all 

positions  of  z} zp_^  and  therefore  <")  (0)  would  vanish. 


270  EVEN    THETA    FUNCTIONS    MAY    VANISH  [185 

185.  If,  however,  nextly,  there  be  even  theta  functions  which  vanish 
for  zero  values  of  the  argument,  it  does  not  follow  as  above  that  every 
^-polynomial  with  double  zeros  corresponds  to  an  odd  half-period  ;  there 
will  still  be  such  ^-polynomials  corresponding  to  the  W~l  (2^  —  1)  odd  half- 
periods,  but  there  will  also  be  such  ^-polynomials  corresponding  to  even 
half-periods. 

For  if  fli,  ...,  ap,  fti,  ...,  ftp  be  integers  such  that  fta.  is  even,  and 
®  (w  -f-  1  H^  „)  vanishes  for  u  =  0,  the  first  differential  coefficients,  in  regard 
to  ulf  ...,up,  of  the  even  function  e7"""  S(u  +  ^ft^  „),  being  odd  functions, 
will  vanish  for  u  =  0.  By  an  argument  which,  for  convenience,  is  postponed 
to  Prop.  XIV.,  it  follows  that  then  the  function  0  (v*'  z  +  \  fl^  „)  vanishes 
identically  for  all  positions  of  x  and  z.  Therefore,  by  Prop.  V.,  there  is  at 
least  a  single  infinity  of  places  zl  ,  ...,  zp_^  satisfying  the  equations 

-  100,  0^W"'W  -/"""-  ......  -a*-'.""-'  ; 

these  equations  are  equivalent  to 


hence  there  is  a  single  infinity  of  ^-polynomials  with  double  zeros  corre 
sponding  to  the  even  half-period  ^Ii^)  „  ,  and  their  p  —  1  zeros  form  coresidual 
sets  with  multiplicity  at  least  equal  to  1. 

By  similar  reasoning  we  can  prove  another  result*;  the  argument  is 
repeated  in  the  example  which  follows  ;  if,  for  any  set  of  values  of  the 
integers  ftlt  ...,  ftp,  a1}  ...,  <xp,  it  is  possible  to  obtain  more  than  one  set  of 
places  nl}  ...  ,  np^l  to  satisfy  the  equations 


then  it  is,  of  course,  possible  to  obtain  an  infinite  number  of  such  sets.  Let 
oo  i  be  the  number  of  sets  obtainable.  Then  fta.  =  q  +  1  (mod.  2).  And  this 
may  be  understood  to  include  the  general  cases  when  (i)  for  an  even  value 
of  ft  a,  no  solution  of  the  congruence  is  possible  (q  =  —  1),  (ii),  for  an  odd  value 
of  fta,  only  a  single  solution  is  possible  (q  —  0). 

As  an  example  of  the  exceptional  case  here  referred  to,  consider  the  hyperelliptic 
surface  ;  and  first  suppose  p  =  3,  the  equation  associated  with  the  surface  being 


then  we  clearly  have  ()  =  28  =  2':'~1(2P—  1)  ^-polynomials,  each  of  the  form  (x  -  at)  (x  -  ay), 

\*/ 

of  which  the  zeros  are  both  of  the  second  order.  We  have,  however,  also,  a  ^-polynomial, 
of  the  form  (.r-c)2,  in  which  c  is  arbitrary,  of  which  the  zeros  are  both  of  the  second 
order  ;  denote  these  zeros  by  c  and  c  ;  then  if  |Qo  o  be  a  proper  half-period 


*  Weber,  Math.  Ann.  xin.  p.  42. 


185]  FOR  ZERO  VALUES  OF  THE  ARGUMENTS.  271 

but,  since,  if  e  be  any  other  place,  the  function  (x-c)j(x-e)  is  a  rational  function,  it 
follows  that  (c,  c)  =  (e,  e)y  and  therefore  that  in  the  value  just  written  for  ^G^  a,  c  may 
be  replaced  by  e,  and  therefore,  regarded  as  quite  arbitrary.  By  the  result  (F),  the 
function  Q(u)  vanishes  when  u  is  replaced  by  %Qp  a,  and  therefore  e  (^''-^fl^  J,  which 

is  equal  to  Q(vx>  m  —  vc>  mi  —  vc>m'1  —  'if'  ™3),  vanishes  when  x  is  at  c;  since  c  is  arbitrary  the 
function  e  (vx>  z  -  |li^  J  vanishes  identically  in  regard  to  x,  for  all  positions  of  z.  If  the 

function  Q(vx'z  +  vXl'  Zl-Afl^  0)  vanished  identically,  it  would,  by  Prop.  VI.,  be  possible, 
in  the  equation 


to  choose  both  zl  and  z2  arbitrarily.  As  this  is  not  the  case,  it  follows,  by  Prop.  XIV. 
below,  that  the  function  G(?t  +  £Qo  a),  and  its  first,  but  not  its  second  differential 
coefficients,  vanish  for  u  =  0.  Hence  \Q^  a  is  an  even  half-period.  (See  the  tables  for 
the  hyperelliptic  case,  given  in  the  next  chapter,  §§  204,  205.) 

There  is  therefore,  in  the  hyperelliptic  case  in  which  p  =  3,  one  even  theta  function 
which  vanishes  for  zero  values  of  the  argument. 

In  any  hyperelliptic  case  in  which  p  is  odd,  the  equation  associated  with  the  surface 
being 

y1  =  (x-av}  ......  0»-«2P  +  2) 

(^-polynomials  with  double  zeros  are  given  by 

(i)     the  (  ]  polynomials  such  as  (x  -04)  ......  (x-ap_l).     As  there  is  no  arbitrary 

place  involved,  the  q  of  the  theorem  enunciated  (§  185)  is  zero,  and  the  half-  period  given  by 
the  equation 


where  nfi  ...,  n\-i  are  the  zeros  of  the  (^-polynomial  under  consideration,  is  consequently 
odd. 


/2»  +  2\ 
(ii)     the  (   2         j    polynomials   such   as   (x  —  at)  ......  (x-ap_3}  (x-c)2,  wherein   c   is 

arbitrary.     Here  <?  =  !  and  /3a  =  0  (mod.  2). 


(2v)_|_2\ 
r  j  polynomials  such  as  (x-a^)  ......  (x  —  a,,  _  6)  (x  —  cf  (x  —  e)2,  for  which 

5  =  2,  |3a=  1  (mod.  2)  ;  and  so  on.     And,  finally, 

the  single  polynomial  of  the  form  (x-c^  ......  (.r-Cjj_j)2,  in  which  all  of  clt  ...,  Cp_i 

~iT  ~2 

are  arbitrary  ;  in  this  case  q=--~-  ,  /3a=*-^-    (mod.  2). 

2i  Jt 

On  the  whole  there  arise 


^-polynomials  corresponding  to  odd  half-  periods,  according  as  p=l  or  3  (mod.  4). 
Now  in  fact,  when  p=  1  (mod.  4) 

4*)+  ...... 


272  EXAMPLE   OF  THE   HYPERELLIPTIC   CASE.  [185 

is  equal  to 


while,  when^>  =  3  (mod.  4) 


is  equal  to  £  (^  +  2  -  2*  +  2  cos  ^^  TT}  ,  and  therefore,  also  to  2"  ~  J  (2"  -  1  ). 
Thus  all  the  odd  half-periods  are  accounted  for.     And  there  are 


even  half-periods  which  reduce  the  theta  function  to  zero.     This  number  is  equal  to 


namely  to  2P~1(2P  +  l)-(  P+    J.     This  is  the  number  of  even  theta  functions  which 

vanish  for  zero  values  of  the  argument.  It  is  easy  to  see  that  the  same  number  is 
obtained  when  p  is  even.  For  instance  when  jo  =  4,  there  are  10  even  theta  functions 
which  vanish  for  zero  values  of  the  argument.  They  correspond  to  the  10  ^-polynomials 
of  the  form  (x  -  c)2  (x  -  at),  wherein  c  is  arbitrary,  and  a^  is  one  of  the  10  branch  places. 

There  are  therefore  (  ^  +     )  even  theta  functions  which  do  not  vanish  for  zero  values  of 

\    P    J 
the  argument. 

In  regard  to  the  places  m1,  ...,  mp  in  the  hyperelliptic  case  the  following  remark  may 
conveniently  be  made  here.  Suppose  the  place  TO  taken  at  the  branch  place  a2p  +  2  >  using 
the  geometrical  rule  given  in  §  183,  we  may  take  for  the  polynomial  A,  of  grade  /*,  the 
polynomial  #-a2p  +  2,  of  grade  1;  its  remaining  ?i/i-2,  =0,  zeros,  give  no  conditions  for 
the  polynomial  ^  of  grade  (n-  l)<r+»i-3  +  /n,  =  (2-  1)  p  +  2-3  +  1,  =p.  Since  o-  +  1,  the 
dimension  of  y,  is  p+l,  the  only  possible  form  for  ^  is  that  of  an  integral  polynomial 
in  x  of  order  p.  This  is  to  be  chosen  so  that  its  2jo  zeros  consist  of  p  repeated  zeros. 
When  p  =  3,  for  example,  it  must,  therefore,  be  of  one  of  the  forms  (x  -  a^  (x  -  a;}  (x  -  a*}, 
(x-<ti}  (x-cf,  where  c  is  arbitrary.  It  will  be  seen  in  the  next  chapter  that  the  former 
is  the  proper  form. 

186.  Another  matter*  which  connects  the  present  theory  with  a  subject  afterwards 
(Chap.  XIII.)  dealt  with  may  be  referred  to  here.  Let  £G  be  a  half-period  such  that 
the  congruence 

\Q.  =  vm>"  m-tf"  '"'  -  ......  -ir2"-1-  m"-1 

can  be  satisfied  by  oc«  coresidual  sets  of  places  zlt  ...,  zp-l  (as  in  Proposition  VI.).     Then 

we  have 

(m2,  z^,  ...,22p_1)  =  (m18,  ...,mp2), 

so  that  (Prop.  IX.)  zlt  ...,  zp_lt  each  repeated,  are  the  zeros  of  a  ^-polynomial  ;  denote 
this  polynomial  by  0.  If  zj,  ...,  zfr>_l  be  another  set,  which,  repeated,  are  the  zeros  of  a 
0-polynomial  <£',  and  are  such  that 


Cf.  Weber,  Math.  Annul,  xni.  p.  35;  Noether,  Math.  Anna!,  xvn.  263. 


186]  RESULTING   RELATIONS   CONNECTING   <£-  POLYNOMIALS. 

then  we  have 


273 


0  =  2vmp'  m-vz"  m>  -  v*1''  m'  -  ......  - 


so  that  SI,...,ZP-I,  Zi,  ...,  «'p_,  are  the  zeros  of  a  ^-polynomial  ;  denote  this  polynomial 
by  iff. 


The  rational  functions  >//•/<£,  </>'/^  have  the  same  poles,  the  places  zn  ...,  zp_lt  and 
the  same  zeros,  the  places  zt',  ...,2v_r  Therefore,  absorbing  a  constant  multiplier  in  ^, 
we  have 

^  =  W,  and  074>  = 


and  thus  the  function  V0'/<£  may  be  regarded  as  a  rational  function  if  a  proper  sign 
be  always  attached.  The  function  has  zlt  ...,  zp_l  for  poles  and  z^,  ...,  z'p_1  for  zeros. 
Conversely  any  rational  function  having  zlt  ...,  zp_l  for  poles  can  be  written  in  this  form. 
For  if  Zj",  ...,  z"p-i  be  the  zeros  of  such  a  function,  we  have 


vz>"'z>  +  ...... 

and  therefore,  by  the  first  equation  of  this  §,  also 


thus  q  of  the  zeros  can  be  taken  arbitrarily  ;  and  if  $  be  any  ^-polynomial  whose  zeros 
Cu  •••  >  fp-i  are  all  of  the  second  order,  and  such  that 


we  can  put 


where  fa,  ...,  0,  are  particular  polynomials  such  as  </>'  or  *,  andX,  X1;  ...,  X,  are  constants. 
In  other  words,  corresponding  to  the  GO  «  sets  of  solutions  of  the  original  equation  of  this 
§,  we  have  an  equation  of  the  form 


wherein  proper  signs  are  to  be  attached  to  the  ratios  of  any  two  of  the  square  roots,  and 
any  two  of  the  q  +  l  polynomials  $,  ^lt  ...,$„  are  such  that  their  product  is  the  square  of 
a  0-polynomial.  There  are  therefore  fa  (q  +  l)  linearly  independent  quadratic  relations 
connecting  the  ^-polynomials.  (Cf.  Chap.  VI.  §§  110—112.) 

For  example  in  the  hyperelliptic  case  in  which  p  =  3,  the  vanishing  of  an  even  theta 
function  corresponds  to  the  existence  of  a  ^-polynomial  *  =  (#-c)2,  such  that 


where  0^3,  =(*)*,  =$*. 

Ex.  i.  Prove,  for  j»  =  3,  that  if  an  even  theta  function  vanishes  for  zero  values  of  the 
arguments  the  surface  is  necessarily  hyperelliptic. 

Ex.  ii.  Prove,  for  jo  =  4,  that  if  two  even  theta  functions  vanish  for  zero  values  of  the 
arguments  the  surface  is  necessarily  hyperelliptic  ;  so  that,  then,  eight  other  even  theta 
functions  also  vanish  for  zero  values  of  the  arguments.  The  number,  2,  of  conditions  thus 
necessary  for  the  fundamental  constants  of  the  surface,  in  order  that  it  be  hyperelliptic,  is 
the  same  as  the  difference,  9-7,  between  the  number,  3p-3,  of  constants  in  the  general 
surface  of  deficiency  4,  and  the  number,  2/>-l,  of  constants  in  the  general  hyperelliptic 
surface  of  deficiency  4. 

B-  18 


274  INTEGRALS   OF   THE  THIRD   KIND  [187 

187.  (XII.)  If  r  denote  any  arguments  such  that  @  (r)  =  0,  and  such 
that  ®(vx'z  +  r)  does  not  vanish  identically  for  all  positions  of  x  and  z, 
the  Riemann  normal  integral  of  the  third  kind  can  be  expressed  in  the  form 


©(^>0+r)_|' 
For  consider  the  function  of  x  given  by 

+  r)  ©  (if'  P  +  r) 


"      ~ 


(a)  it  is  single-valued  on  the  Riemann  surface  dissected  by  the  a  and  b 
period  loops  ; 

(/3)  it  does  not  vanish  or  become  infinite,  for  the  zeros  of  ®  (vx'  z  +  r), 
other  than  z,  do  not  depend  upon  z  (by  Proposition  IV.); 

(7)  it  is  unaffected  by  a  circuit  of  any  one  of  the  period  loops.  At 
a  loop  at  it  has  clearly  (Equation  B,  §  175)  the  factor  unity  ;  at  a  loop 
bi  it  has  the  factor 


e          l     .  e 

which  is  also  unity.     Thus  the  function  is  single-valued  on  the  undissected 
surface  ; 

(8)     thus  the  function  is  independent  of  x  ;  and  hence  equal  to  the  value 
it  has  when  the  place  x  is  at  zy  namely  1. 

A  particular  case  is  obtained  by  taking 


where  z1}  ...,  zp-i  are   any  places   such   that   ®(vx>z  +  r)  does  not  vanish 
identically.     Then  by  the  result  (F)  the  function  ®  (r)  vanishes. 

Hence  we  have 


Another  particular  case,  of  great  importance,  is  obtained  by  taking 
r  =  ^ftjt, tf,  k,  k'  denoting  respectively  p  integers  k1}  ...,kp,  h',  ...,  kp',  such 
that  kk'  is  odd,  the  assumption  being  made  that  the  equations 


188]  EXPRESSED   BY  THETA   FUNCTIONS.  275 

are  not  satisfied  by  more  than  one  set  of  places  £,,  ...,  £p_j  (cf.  Props.  III.,  V.). 
Then  the  function  ©  (ifK>z  +  ^Qk,k)  does  not  vanish  identically,  and  we  have 


(XIII.)     Suppose  k  equal  to  or  less  than  p  ;    consider  the  function  given 
by  the  product  of 

g-n^-n^- -n*;^ 

and 

(H)  (i&i  m 9)°"  wi  -^  —  V^k'  mk  -t-  ^^   /  @  ^D2'  "* li"1 '  wl' —  Wa*'  *"*  -4-  T} 

wherein  r  denotes  arguments  given  by 


and  each  of  the  sets  a1}  ...,  a^,  7^+1,  •••,%,&,  •••,  0k,  7*+i>  •••»  7p  ^s  sucn 
that  the  functions  involved  do  not  vanish  identically  in  regard  to  x. 

This  function  is  single-valued  on  the  dissected  Riemann  surface,  does  not 
become  infinite  or  zero,  and,  for  example,  at  the  period  loop  6;  it  has  the  factor 
eL,  where 


L,  =  -  2m  (v°>  '  P'  +  ......  +  v°>;>  h)  -  2-rn  (v*>  m  -  -va"  ™-  - 

+  2-Trt  (va>  »»  -  1^1 


is  zero.     Thus  the  function  has  the  constant  value,  unity,  which  it  has  when 
x  is  at  z.    Therefore 

na;(3  x,z      _, 

+  '  '  '  +  ~    ° 


the  places  7i+1,  ...,<yp  being  arbitrarily  chosen  so  that  a1}  ...,«£, 

are  not  zeros  of  a  ^-polynomial,  and  /3lt  ...,  ^8^,  7^+1,  .  ..,  yp  are  not  zeros  of  a 

^-polynomial. 

Thus,  when  k  =  p,  we  have  the  expression  of  the  function  considered  in 
§171,  Chap.  IX.  in  terms  of  theta  functions.  For  the  case  where  oti,  ...,  a* 
are  the  zeros  of  a  ^-polynomial,  cf.  Prop.  XV.  Cor.  iii 

188.   (XIV.)   We  return  now  to  the  consideration  of  the  identical  vanishing 
of  the  ®  function.     We  have   proved  (Prop.  VII.),  that  if  ®(vx"z>+  ...... 

+  tfB«'z<«  +  r)  be  identically  zero  for  all  positions  of  xl>  ,..,xq,z-i,  ...,zq,  but 
(5)  (rx,  z  +  vx,  ,  z,  +  ......  +  7,a-,,  z,,  +  r}  ^e  not  i(jentically  zero  for  all  positions  of 

18—2 


276  INVESTIGATION  [188 

x  and  z,  then  there  exist  oo  «  sets  of  places  £,...,  £p_i,  and  oo  9  sets  of  places 
£,  ...,&>_!,  such  that 


and 

_  j-  =  <)finp,  in  _  yfi  ,  m,  _  ^      _  ^  _  •yfp-i.  *»j»-it 


Now,  if  in   the   equation   ®  (^  >  *>  +  ......  +  t^  *«  +  r)  =  0,   we   make   xq 

approach  to  and  coincide  with  zq,  we  obtain 

t  6/  (tf*'>  *>  +  ......  +  v*'-1'  z<-'  +  r)  ^  (s9)  =  0, 

i=l 

• 

wherein  ©/  (it)  is  put  for  r—  ®  (u),  H;  (a;)  for  2-Trt  Dxvf  ",  a  being  arbitrary  ; 

(7Mj 

and  this  equation  holds  for  all  positions  of  ac1,  z1}  ...,  #9_a,  ^9_i.     Since,  how 
ever,  the  quantities  fl]  (zq),  ...  ,  flg  (^q)  cannot  be  connected  by  any  linear 
equation  whose  coefficients  are  independent  of  zq,  we  can  thence  infer  that 
the  first  differential  coefficients  of  ®  (u)  vanish  identically  when  u  is  of  the 
form^"  z>  +  ......  +0*9-1.29-1  +  T».     It  follows  then  in  the  same  way  that  the 

second  differential  coefficients   of  @  (u)  vanish  identically  when  u  has  the 
form  vXi>  2>+  ......  +  vxi-°->  z<>-2  +  r  ;  in  particular  all  the  first  and  second  differ 

ential  coefficients  vanish  when  u  =  r.  Proceeding  thus  we  finally  infer  that 
®  (w)  and  all  its  differential  coefficients  up  to  and  including  those  of  the  <jth 
order  vanish  when  u  =  r. 

We  proceed  now  to  shew  conversely  that  when  ©  (u)  and  all  its  differential 
coefficients  up  to  and  including  those  of  the  <?th  order,  vanish  for  u  =  r, 
then    ©  (vXl  '  z>  4-  ......  +^9.29+r)   vanishes   identically   for   all   positions   of 

#1,  ^i,  ^2,^2,  ...,xq,Zq.     By  what  has  just  been  shewn  ©  (v**  z  +  v*"*!  +  ...... 

+  -y*,,  zq  +  rj  wiH  not  vanish  identically  unless  the  differential  coefficients  of 
the  (q  +  l)th  order  also  vanish. 

We  begin  with  the  case  q=l.  Suppose  that  ®  (M),  ©/  (u),  ...  ,  Sp'  (u),  all 
vanish  for  u  =  r  ;  we  are  to  prove  that  ®  (#*•  z  +  r)  vanishes  identically  for  all 
positions  of  x  and  z. 

Let   e,  f  be   such   arguments  that  @(e)=0,  ®  (/)=(),  but  such  that 
©/  (e)  are  not  all  zero  and  ©/(/)  are  not  all  zero,  and  therefore  ®  (vx> 
(J0  not  vanish  identically;  consider  the  function 

@  (e  +  if6'  z)  @  (e  -  tf>  z) 


firstly,  it  is  rational  in  x  and  z  ;  for,  considered  as  a  function  of  x,  it  has, 
at  the  period  loop  br,  (Equation  B,  §  175)  the  factor 


188]  OF  THE  GENERAL  PROBLEM  277 

whose  value  is  unity  ;  and  a  similar  statement  holds  when  the  expression  is 
considered  as  a  function  of  z,  for  the  expression  is  immediately  seen  to  be 
symmetrical  in  x  and  z ;  secondly,  regarded  as  a  function  of  x,  the  expression 
has  2  (p  —  1)  zeros,  and  the  same  number  of  poles,  and  these  (Prop.  IV.) 
are  independent  of  z.  Similarly  as  a  function  of  z  it  has  2  (p  —  1)  zeros  and 
poles,  independent  of  a; ;  therefore  the  expression  can  be  written  in  the  form 
F(x}F(z},  where  F(x)  denotes  the  definite  rational  function  having  the 
proper  zeros  and  poles,  multiplied  by  a  suitable  constant  factor,  and  F  (z)  is 
the  same  rational  function  of  z. 

Putting,  then,  x  to  coincide  with  z,  and  extracting  a  square  root,  we  infer 

p 


where  flt  (a?)  =  2m  Dxv*'a,  for  a  arbitrary,  is  the  differential  coefficient  of  an 
integral  of  the  first  kind  ;  thence  we  have 


In  this  equation  suppose  that  e  approaches  indefinitely  near  to  r,  for  which 
®(r)  =  0,  ®/(r)  =  0.  Then  the  right  hand  becomes  infinitesimal,  inde 
pendently  of  x  and  z.  Therefore  also  the  left  hand  becomes  infinitesimal 
independently  of  x  and  z  ;  and  hence  0  (vx'  z  +  r)  vanishes  identically,  for 
all  positions  of  as  and  z. 

We  have  thus  proved  the  case  of  our  general  theorem  in  which  q  =  l. 
The  theorem  is  to  be  inferred  for  higher  values  of  q  by  proving  that  if  the 
function  ®  (vx><  '•  +  ......  +  t^»->'  *->  +  r)  vanish  identically  for  all  positions  of 

#!,  2j,  ...  ,  #,„_!,  2m_i,  and  also  the  differential  coefficients  of  ®(w),  of  order 
m,  vanish  for  it  =  r,  then  the  function  ®(^i.«i  +  ......  +^»,  ««  +  r)  vanishes 

identically.  For  instance  if  this  were  proved,  it  would  follow,  putting  m  =  2, 
from  what  we  have  just  proved,  that  also  ®(vx><  ^  +  if*'**  +  r)  vanished 
identically,  and  so  on. 

As  before  let/  be  such  that  ®  (/)  =  0,  but  all  of  ©/  (/)  are  not  zero  ;  so 
that   ®  («*.  z  +/)   does  not  vanish  identically  in  regard   to  x  and   z.     Let 
e   be  such  that  ®(v«..^  +  ......  +  w*»-i,«w-i+e)   vanishes  identically  for  all 

positions  of  #,,  *„  iV.ViUi  Zm-i  ,  but  such  that  the  differential  coefficients  of 
®(M)  of  the  first  order  do  not  vanish  identically  for  u  =  vxi>zi+...  +  •y*»«-i,«'«-i  -j.  e- 
so  that  the  function  @  (t^i.  ^  +  ......  +  &m,  ^  +  e)  does  not  vanish  identically.' 

Consider  the  product  of  the  expressions 


e) 


_ 
nn®  (w«x.  v  +/)  0  (t^x.  v  -/) 


278  OF   THE   IDENTICAL   VANISHING  [188 

wherein  h,  k  in  the  numerator  denote  in  turn  every  pair  of  the  numbers 
1,2,  ...  ,  m,  so  that  the  numerator  contains  4  .  \m  (m  —  1)  +  2  =  2  (m2  —  m  +  1) 
theta  functions,  and  X,  /-t  in  the  denominator  are  each  to  take  all  the  values 
1,  2,  ...,  m,  so  that  there  are  2m2  theta  functions  in  the  denominator. 

Firstly,  this  product  is  a  rational  function  of  each  of  the  2m  places 
a?!,  Zi,  ...,  xm,  zm.  Consider  for  instance  ccl;  it  is  clear  that  if  the  product 
be  rational  in  xlt  it  will  be  entirely  rational.  As  a  function  of  xl}  the 
product  has  at  the  period  loop  br  a  factor  e~2iriK  where 


and  this  expression  is  identically  zero. 

Secondly,  considering  the  product  as  a  rational  function  of  x1}  the 
denominator  is  zero  to  the  second  order  when  x±  coincides  with  any  one  of 
the  m  places  zlt  ...,  zm,  and  is  otherwise  zero  at  2m  (p  —  1)  places  depending 
on  /  only  ;  of  these  latter  places  2  (m  —  1)  (p—  1)  are  also  zeros  of  the 
factors  H'0  («**'**+/)©(«**•**--/);  there  are  then  2(jp-l)  poles  of  the 
function  which  depend  on  /  only.  The  factors  II'®  (tf"*«  **  +/)  ©(«"*«  **  -/) 
have  also  the  zeros  #2>  •••>  #»»>  each  of  the  second  order.  The  factors 
®  (tfii  ,«i  +  ...+  tf*.  ,  zm  +  e)@  (t^i  ,  zi  +  .  .  .  +  if*  ,  z».  _  e)  have,  by  the  hypothesis 
as  to  e,  the  zeros  zlt  z2}  ...,  zm,  each  of  the  second  order,  as  well  as  2  (p  —  m) 
other  zeros  depending  on  e  only.  On  the  whole  then,  regarded  as  a  function 
of  ac1  ,  the  product  has 

for  zeros,  2(p  —  m)  zeros  depending  on  e,  as  well  as  the  zeros  #2,  ...,  xmy 
each  of  the  second  order, 

for  poles,  2  (p  —  1)  poles  depending  on/; 

the  function  is  thus  of  order  2(p  —  1);  and  it  is  determined,  save  for  a 
factor  independent  of  xly  by  the  assignation  of  its  zeros  and  poles.  It  is 
to  be  noticed  that  these  do  not  depend  on  z1}  z2,  ...,  zm. 

It  is  easy  now  to  see  that  the  product,  regarded  as  a  function  of  zl} 
depends  on  z2,  ...,  zm,  e,f  in  just  the  same  way  as,  regarded  as  a  function 
of  x1}  it  depends  on  cc2,  ...,  xm,  e,f. 

The  expression  is  therefore  of  the  form  F(xlt  #2>  •••>  ®m)  F  (z\>  2-2,  •••>  zm\ 
wherein  F  denotes  a  rational  function  of  all  the  variables  involved. 

The  form  of  F  can  be  determined  by  supposing  xlt  ...,xm  to  approach 
indefinitely  near  to  z1}  ...,  zm  respectively;  then  we  obtain 


where  tm  is  the  infinitesimal  for  the  neighbourhood  of  the  place  zm, 

0.'    ^,  ,Zl+  ......  +  vX,n-l,  Z« 


188]  OF  THE  THETA   FUNCTION.  279 

where  tm-i  is  the  infinitesimal  for  the  neighbourhood  of  the  place  2m_i,  and 
so  on,  and  eventually, 


\47rl)       fm  =  i        t'i=l 

Similarly 


where  /i,  A;  refers  to  all  pairs  of  different  numbers  from  among  1,  2,  ...,  m. 
Therefore,  dividing  by  a  factor 


which  is  common  to  numerator  and  denominator,  and  taking  the  square  root, 
we  have 


i.  i  e'^,  j,,.  ...  iw  (<o  HI  (^on,^.  ..««(*») 


,  t>» 

i  ' ' '  '  zm)  ~ 


On  the  whole  therefore  we  have  the  equation 

!• z'  + +  w*m'ZBl  -  e) 

*  -    IT®  * .  zt  +    @ 


nn@(/A> 

•vEr/'/v.  r      f>\ty(?  ?      o\ 

•K    ^!  ,    .  .  .  ,    J/m  ,  K)    X    \^i,    .  •  •  ,    4m  >   K) 


where 


^(^,...,^,6)=  2  ...       @'il)r-2  .....  ^(ejfl^fo)...  flfM(ff,w). 

l-m  =  l         H  =  l 

Suppose  now  that  ef  is  made  to  approach  to  r;  ;  then  the  conditions  we 
have  imposed  for  e  are  satisfied,  and  there  is  added  the  further  condition 
that  the  differential  coefficients  of  order  m,  O',-^  ,-2)  ...,,•„>,  also  vanish.  Hence 
it  follows  that  ®  (^  <z>  +  ......  +  1^«.  z-»  +  ?•)  vanishes  identically. 

The  whole  theorem  enunciated  is  thus  demonstrated. 


280  RESULTING   EXPRESSION  [188 

(XV.)  The  remarkable  investigation  of  Prop.  XIV.  is  due  to  Riemann  ; 
it  is  worth  while  to  give  a  separate  statement  of  one  of  the  results  obtained. 
Using  q  instead  of  m  —  1,  we  have  proved  that  if  the  equations 


Q  =  vmp>  m  —  i1'  m'  —  .  .     .  .  —  I;P 

are  satisfied  by  oc  1  sets  of  places  fi,  ...,  ^_1(  so  that  also  the  equations 
—  e  =  v™*1  '  m  —  v^  >  '  rrti  —  ......  —  ?;£  p 


are  satisfied  by  x«  sets  of  places  £,  ...,  f^,  then  their  exists  a  rational 
function,  which  has  (i)  for  poles,  the  2(p  —  1)  places  tl}  ...,  tp,l}  zlt  ...,  zp^, 
which  satisfy  the  equations 


f= 


f  being  supposed  such  that  these  equations  have  one  and  only  one  set  of 
solutions,  and  has  (ii)  for  zeros,  the  arbitrary  places  xlt  ...,acq,  each  of  the 
second  order,  together  with  2(p-  1  -q)  places  £9+1,  ...,  Zp_l}  j-q+1,  ...,  g^, 
satisfying  the  equations 

Q  =  Vmp'  m  —  iF1'  m'  —  ......  —  •y2'9'  1Hq  —  l)£<i+l>  m4+i  _  ..     ..  _  yfp-i»  mp-i 

—  e  =  vm*'  m  —  V^1'  TOI  —  .  .     .  .  —  VXq>  inq  —  ifig+1>  niq+l  _  .  .     .  .  _  •yfp-1'  *»?-! 

and  the  function  can  be  given  in  the  form 

¥(#!,  xz,  ...,  acq,  x,e)  +  ®  (a;,/), 

the  notation  being  that  employed  at  the  conclusion  of  Proposition  (XIV.). 
The  expressions  M',  $  occurring  here  have  the  zeros  of  certain  (^-polynomials, 
to  which  they  are  proportional. 

Corollary  i.     If  we  take  p  —  1  places  £,  ...,  ^p_1)  so  situated  that  only 
one  ^-polynomial  vanishes  in  all  of  them,  and  define  e  by  the  equations 


e  = 


there  will  be  no  other  set  £i,  ...,  ^,_1(  satisfying  these  equations,  or  5=0. 
If  fi>  •••>  Zp-i  be  the  remaining  zeros  of  the  ^-polynomial  which  vanishes  in 
£i,  ...  ,  %p-i,  we  have  (Prop.  IX.) 

(m\  5i,  ...,  ^_!,  £,  ...,  1^0  =  (wh8,  ....  7?i/), 
and  therefore 


Similarly  if  tlf  .  .  .  ,  <p_!  be  arbitrary  places  which  are  the  zeros  of  only  one 
^-polynomial,  we  can  put 

f  '  —  <yWiy),  m  _  n,tt  ,  m,  _  _  OI^P-II  Wp-i 

—  f=  vm'"  '"  —  vz>  >  m<  —  ......  —  v*"-1-  '"p-1. 


188]  OF    RATIONAL   FUNCTIONS  281 

Then  the  rational  function  having  tit  .  ..,  £p_i,  z^,  ...,  Zp-i  for  poles,  and 

(Ti.  •••.  KP-I,  &>  ••-.  &-i  for  zeroy  is  given  by  ^(^  «)  -5-  <&  (#>  /)•     Thus  tne 
^-polynomial  which  vanishes  in  %\>  •  ••>  £p-i>  £i>  •••>  £p-i  is  given  by 

P 

2  ®/  (vm»'  m  —  v^'m>  —  ......  —  Vs"-1'  mp~l)  fa  (x), 

1=1 

where  fa  (a),  ...,<}>p(x)  are  the  ^-polynomials  occurring  in  the  differential 
coefficients  of  Riemann's  normal  integrals  of  the  first  kind. 

Hence  if  n^  ...,  np_!  be  places  which,  repeated,  are  all  the  zeros  of  a 
^-polynomial,  the  form  of  this  polynomial  is  known.  Since,  then,  we  have 
(Prop.  XI.  p.  269) 


we  can  write  this  polynomial 


|fl  being  an  odd  half-period. 

If  another   ^-polynomial   than  this  one  vanished  in  nlt  ...,  np_lt  there 
would  be  other  places  n^,  ...,  rip_1}  such  that 


and  therefore  (Prop.   VI.)  the  function  B(^»*.+  ^(l)  would  vanish  identi 
cally;  in  that  case  (Prop.  XIV.  p.  276)  the  coefficients  ®/(£H)  would  vanish. 


We  can  express  the  0-polynomial  in  terms  of  any  integrals  of  the 
first  kind;  if  Vi  '",...,  Vp'  "  be  any  linearly  independent  integrals  of 
the  first  kind,  expressible  in  terms  of  the  Riemann  normal  integrals 
v*'  ,  ...,  Vp  m  by  linear  equations  of  the  form 

*•  m       -\        -irx>  m  .  ,    -v        irx<  m  /-to 

Vi       =X;)1F1       +  ......  +\,pVp      ,  (l  =  l,  2,  ...,/>), 

and  the  function  ®  (u)  be  regarded  as  a  function  of  Ul}  .  .  .  ,  Up  given  by 

w»  =  Xi>1  t/i4  ......  +  \iif  Up,  (i=l,  2,  ...,p), 

and,  so  regarded,  be  written  ^  (  U),  the  ^-polynomial  which  has  zeros  of  the 
second  order  at  nlt  ...,  wp_i  can  be  written 


'm 


where  ^  (a;),  .  .  .  ,  -^  («)  are  the  ^-polynomials  corresponding  to   V? 

V*'m,  and  ^H  denotes  a  set  of  simultaneous  half-periods  of  the  integrals 

FI  '  '",  ...,  Vfl'm.     If  ^n  stand  for  p  quantities  of  which  a  general  one  is 


282  OF   SPECIAL   KIND.  [188 

and  (»,.,  s,  w'r,  g  be  2p-  quantities  given  by 

J-  =  2\  j  «i,  8  +  2X;,  2  ft)2i  g     +  ......  +  2X/(  p  Op,  ,,     (t,  5  =  1,  2,   .  .  .  ,  p), 

Tt-,  g  =  2\i,  ]  o)'^  g  -I-  2X,-,  2  a/-,  g  +  ......  +  2\it  p  a>'p>  8, 

where,  in  the  first  equation,  we  are  to  take  1  or  0  according  as  i  =  s  or  i^s, 
then  £fl  will  stand  for  p  quantities  of  which  one  is 

Aa®*,  i  +  ......  +  kpcot,  p  +  ki(o'it  i  +  ......  +  kp'o)'it  p,     (i  =  I,  2,  .  .  .  ,  p). 

For  example  when  the  fundamental  Riemann  surface  is  that  whose 
equation  may  be  interpreted  as  the  equation  of  a  plane  quartic  curve,  every 
double  tangent  is  associated  with  an  odd  half-period  and  its  equation  may 
be  put  into  the  form 

*&/  (in)  +  jfo'  (f  ii)  4-  *;  (in)  =  o. 

Corollary  ii.     If  the  equations 

e  =  vm>"  m  —  if1'  Wi  —  v^2  '  m*  _  .  .       —  v^p~l>  mi>-1 

can  be  satisfied  with  an  arbitrary  position  of  x^  and  suitable  positions  of 
£,,  ...,  %p-i,  and  therefore,  also,  the  equations 


—  e  = 


can  be  satisfied,  then  a  ^-polynomial  vanishing  at  x1  to  the  second  order,  and 
otherwise  vanishing  in  £,,  ...,  £p_!,  ^2,  •••,  fp-i,  is  given  by 


Ex.  In  the  case  of  a  plane  quintic  curve  having  two  double  points,  this  gives  us  the 
equation  of  the  straight  lines  joining  these  double  points  to  an  arbitrary  point  x1,  of  the 
curve. 

Corollary  iii.  We  have  seen  (Chap.  VI.  §  98)  that  any  rational  function 
of  which  the  multiplicity  (q)  is  greater  than  the  excess  of  the  order  of  the 
function  over  the  deficiency  of  the  surface,  say,  q  =  Q—p  +  r  +  I,  can  be 
expressed  as  the  quotient  of  two  ^-polynomials.  If  the  function  have 
£i,  •••>  &  f°r  zeros,  and  £,  ...,  J?Q  for  poles,  and  the  common  zeros  of  the 
^-polynomials  expressing  the  function  be  zlt  ...,  ZR,  where  R=2p-2-Q, 
the  function  is  in  fact  expressed  by 


where  (cf.  §  93,  Chap.  VI.) 

7?ln  *  7ft  £1 »  tJl-t 

0   n\       ir*  nt     A'  ^ <1 

/.  7)(D.  Ill  2,,  HJj  *B_T, 

f=vp      —  v        — —  v 


189]  GENERALIZED   THETA   FUNCTION.  283 

189.  Before  concluding  this  chapter  it  is  convenient  to  introduce  a 
slightly  more  general  function  *  than  that  so  far  considered  ;  we  denote  by 
^  (u  ;  q,  q'),  or  by  S-  (u,  q),  the  function 

&  (u  ;  q,  q')  =  2eaw2+2AM<w+9'>+&(n+9')2+2"r9(ri+5'>, 

wherein  the  summation  extends  to  all  positive  and  negative  integer  values  of 
the  p  integers  wn  ...,np,a  is  any  symmetrical  matrix  whatever  of  p  rows  and 
columns,  h  is  any  matrix  whatever  of  p  rows  and  columns,  in  general  not 
symmetrical,  b  is  any  symmetrical  matrix  whatever  of  p  rows  and  columns, 
such  that  the  real  part  of  the  quadratic  form  bm2  is  necessarily  negative 
for  all  real  values  of  the  quantities  m1,  ...,  mp,  other  than  zero,  and  q,  q 
denote  two  sets,  each  of  p  constant  quantities,  which  constitute  the  character 
istic  of  the  function.  In  the  most  general  case  the  matrix  b  depends  on 
?p(p+  1)  independent  constants  ;  if  however  we  put  iirr  for  b,  r  being  the 
symmetrical  matrix  hitherto  used,  depending  only  on  3p  -  3  constants,  and 
denote  the  p  quantities  hu  by  U,  we  shall  obtain 

*(M;  q,  q')  =  eau*  ®  (U  ;  q,  q'). 

We  make  consistent  use  of  the  notation  of  matrices  (see  Appendix  ii.). 
If  u  denote  a  row  (or  column)  letter  of  p  elements,  and  h  denote  any  matrix 
of  p  rows  and  columns,  then  hu  is  a  row  letter  ;  we  shall  generally  write 
huv  for  hu.v;  and  we  have  huv  =  hvu,  where  h  is  the  matrix  obtained  from 
h  by  transposition  of  rows  and  columns.  Further  if  k  be  any  matrix  of  p  rows 
and  columns,  hu  .  kv  =  hkvu  =  khuv.  For  the  present  every  matrix  denoted  by 
a  single  letter  is  a  square  matrix  of  p  rows  and  columns. 

Now  let  o>,  w',  r),  T/  be  any  such  matrices,  and  P,  P'  be  row  letters  of 
elements  Pl}  ...,  Pp,  P/,  ...,  Pp.  Then,  by  the  sum  of  the  two  row  letters 
a>P  +  oa'P'  we  denote  a  row  letter  consisting  of  p  elements,  each  being  the 
sum  of  an  element  of  o>P  with  the  corresponding  element  of  &>'P'.  This 
row  letter,  with  every  element  multiplied  by  2,  will  be  denoted  by  flp, 
so  that 


in  a  similar  way  we  define  a  row  letter  of  p  elements  by  the  equation 

HP  =  2r)P  +  27/P'  ; 
then  u  +  flp  will  denote  a  row  letter  of  p  elements,  like  u. 

The  equation  we  desire  to  prove,  subject  to  proper  relations  connecting 
&),  a/,  77,  77',  is  the  following, 

*  (u  +  ft,,,  q)  =  effp(«+sn,)-Wip/'+2«  (Pq'-p-q)  e-z«iPV'  §  (W)  p  +  9)}          (L^ 

which  is  a  generalization  of  some  of  the  fundamental  equations  given  for 
©  (u). 

*  Schottky,  Abrias  einer  Theoric  der  Abehchen  Functionen  von  drei  Variabeln,  Leipzig,  1880. 
The  introduction  of  the  matrix  notation  is  suggested  by  Cayley,  Math.  Aniuil.  (xvn.),  p.  115. 


284  THE   FUNDAMENTAL   EQUATIONS.  [189 

In  order  that  this  equation  may  hold  it  is  sufficient  that  the  terms  on  the 
two  sides  of  the  equation,  which  contain  the  same  values  of  the  summation 
letters  %,  ...,  np,  should  be  equal  ;  this  will  be  so  if 


a  (u  +  dp)2  +  2h(u  +  flp)  (n  +  q')  +  b(n  +  q'f  +  2iriq  (n  +  q) 
=  HP(u  +  £flp)  -  TriPP'  -  ZTriP'q  +  an"  +  2hu  (n  +  q'  +  P')  +  b  (n  +  q'  +  PJ 


picking  out  in  this  conditional  equation  respectively  the  terms  involving 
squares,  first  powers,  and  zero  powers  of  n1}  ...,  np,  we  require 

6  =  6, 

h  (u  +  tip)  +  bq  +  Triq  =  hu+b  (q  +  P')  +  Tri(P  +  q), 
and 

a  (u  +  Hp)3  +  2/i  (u  +  Hp)  q  +  bq'2  +  2-rriqq'  =  HP  (u  +  £HP)  -  TriPP'  -  liriP'q 
+  cm2  +  2/m  (q'  +  P')  +  6  (q  +  P')2  +  Ziri  (P  +  q)  (q'  +  P'). 

190.  In  working  out  these  conditions  it  will  be  convenient  at  first  to 
neglect  the  fact  that  a  and  6  are  symmetrical  matrices,  in  order  to  see  how 
far  it  is  necessary. 

The  second  of  these  conditions  gives 

MIP  =  TriP  +  6P', 

and  therefore  gives  the  two  conditions  hw  =  ^TTI,  hw  =  ^5,  whereby  o>,  &>' 
are  determined  in  terms  of  the  matrices  h,  b.  In  particular  when  h  =  iri 
and  6  =  i7TT,  as  in  the  case  of  the  function  ®(V),  we  have  2a>  =  l,  2&>'  =  T, 
namely  2o>,  2o>'  are  the  matrices  of  the  periods  of  the  Riemann  normal 
integrals  of  the  first  kind,  respectively  at  the  first  kind,  and  at  the  second 
kind  of  period  loops. 

The  third  condition  gives 

ZauSlp  +  aO2P  +  2/tOp^'  =  HP  (u  +  ^flp) 

-  iriPP'  -  ZiriP'q  +  ZhuP'  +  b  (2q'P'  +  P'2)  +  2™  (qP'  +  Pq  +  PF), 
that  is 

-Hp-  IhP1)  u  +  (aflp  -$HP)  flp  -  TriPP'  -  6P'2 

+  2  (AnP  -  triP  -  6P')  q'  =  0  ; 


in  order  that  this  may  be  satisfied  for  all  values  of  n1}  ...,  UP)  we  must  have, 
referring  to  the  equation  already  obtained  from  the  second  condition, 


and 

6P')  P'  ; 


from  the  first  of  these,  by  the  equation  already  obtained,  we  have 

kttpP'  =  (-rriP  +  bP')  P  ; 


190]  THE   RELATIONS   FOR   THE   PERIODS.  285 

subtracting  this  from  the  second  equation,  there  results 


and  in  order  that  this  may  hold  independently  of  the  values  assigned  to 
P,  P'  it  is  necessary  that  d  =  a,b=b',  when  this  is  so,  these  two  equations 
give,  in  addition  to  the  one  already  obtained,  only  the  equation 


leading  to 

77  =  2a&>,  V}'  =  2aw'  —  2h, 

which  express  the  matrices  77  and  r[  in  terms  of  the  matrices  a  and  h.     These 
equations,  with 


or 

hca  =  \irit  ha*'  =  ^b, 

are  all  the  conditions  necessary,  and  they  are  clearly  sufficient.     When  they 
are  satisfied  we  have 


-  q  +  P),  (L), 

where 

XP  (w)  =  HP  (u  +  |  Hp)  -  -rriPP. 

Ex.     Weierstrass's  function  cru  is  given  by 


where  A  is  a  certain  constant. 

The  equations  obtained  express  the  4>p-  elements  of  the  matrices  &>,  to',  77,  77' 
in  terms  of  the  pz  +  p  (p  4-  1  )  quantities  occurring  in  the  matrices  a,h,b\ 
there  must  therefore  be  2p2  —  p  relations  connecting  the  quantities  in  o>,  «', 
v),  77'.  The  equations  are  in  fact  of  precisely  the  same  form  as  those  already 
obtained  in  §  140,  Chap.  VII.,  equation  (A),  and  precisely  as  in  §  141  it 
follows  that  the  necessary  relations  connecting  G>,  &>',  77,  77'  may  be  expressed 
by  either  of  the  equations  (B),  (C)  of  §  140.  Using  the  notation  of  matrices 
in  greater  detail  we  may  express  these  relations  in  a  still  further  way. 

For 

-  hP)  0Q  -  (ang  -  hF)  ftp 


=  hflp  .  Q'  -  h£lQ  .  P' 

=  (viP  +  bP)  $  -  (iriQ  +  bQ')  P, 
so  that 

-  PQ)  ; 


this  relation  includes  all  the  2p2  —  p  necessary  relations  ;  for  it  gives 

(rjP  +  rj'P)  (a>Q  +  u'Qf)  -  (r,Q  +  rj'Q')  (a>P  +  to'P)  =  ^-rri  (PQ'  -  PQ), 


286  CASE   WHEN    THE    FUNCTION    IS    ODD   OR   EVEN.  [190 

or  (using  the  matrix  relation  already  quoted  in  the  form  hu.kv=  7ikvu  = 
(wrj  -  tjto)  PQ  -f  <W  -  ^o>')  P'Q  +  (W'T;  -  rj'w)  PQ'  +  (m'rj'  -  ijV)  P'Q' 


and  expressing  that  this  equation  holds  for  all  values  of  P,  Q,  P',  Q',  we 
obtain  the  Weierstrassian  equations  ((B)  §  140). 

Similarly  the  Eiemann  equations  ((C)  §  140)  are  all  expressed  by 

')  -  (2a>P  +  2rjQ)  (2«'P'  +  2ij'Q/)=  27rt  (PQ'  -  P'Q). 


Ex.  i.  If  we  substitute  for  the  variables  u  in  the  ^  function  linear  functions  of  any  p 
new  variables  v,  with  non-vanishing  determinant  of  transformation,  and  LP  be  formed  from 
the  new  form  of  the  ^  function,  regarded  as  a  function  of  v,  just  as  HP  was  formed  from 
the  original  function,  prove  that  LPv  =  HPu,  and  that  XP  (u)  remains  unaltered. 

Ex.  ii.     Prove  that 

XP  (u  +  n.v)  +  X.v  (u)  -  2TriM'P=  Xfi  (u  +  fl.v)  +  X.v  (u}  - 
provided 

The  equation  (L)  is  simplified  when  P,  P'  both  consist  of  integers.  For 
if  M,  M'  be  rows  of  integers,  it  is  easy  (putting  a  new  summation  letter, 
m,  for  n  +  M',  in  the  exponent  of  the  general  term  of  ^  (u  ;  q  +  M,  q'  +  M'),) 
to  verify  that 

$(u;  q  +  M,  q'  +  M')  =  &™M<t  ^  (u  ;  q,  q'). 

Therefore,  if  m,  m'  consist  of  integers,  we  find 

S-  (u  +  Slm,q)  =  eKm^  +***(«*'  -m'q]  ^  (Wj  3)} 
and  in  particular 

S(w  +  ftm)  =  eAm(M)Sr(*0> 

where  ^  (u)  is  written  for  ^r  (u  ;  0,  0).  The  reader  will  compare  the  equations 
obtained  at  the  beginning  of  this  chapter,  where  a  =  0,  77  =  0,  vf  =  —  2m, 
a,  =  £,  a'  =£T,  flp  =  P  +  rP',  HP=-  2-rriP',  \P  (u)  =  -  MF  (u  +  %P  +  %rP) 
-  TriPP'. 

One  equation,  just  used,  deserves  a  separate  statement  ;  we  have 

*(u;  q  +  M)  =  e*"iMi'  %  (u  ;  q), 
where  M  stands  for  a  row  of  integers  M1}  ...,  Mp,  MJ,  ...,  Mp'. 

191.  Finally,  to  conclude  these  general  explanations  as  to  the  function 
^  (u),  we  may  enquire  in  what  cases  ^  (u)  can  be  an  odd  or  even  function. 

When  m,  m'  are  rows  of  integers  the  general  formula  gives 
^(-11  +  flm,  q)  =  &»  (-»)  +2™  (?»<?'  -*»'<?)  ^  (-  u,  q)  ; 


192]  INTRODUCTION    OF   THE    £  FUNCTIONS. 

hence  when  ^ (u,  q)  is  odd,  or  is  even,  since  \,n(—  u)  =  \-m (u),  we  have 

<\  /?/  _  O        n}  —  /jA_m(M)  +  2m'(mo'—  m'q)  «\  /».    n\  . 

,J    \IV  *I"Hl)   <£)  t/  rJ    \U,    »//    , 

therefore,  by  equation  (L), 

j  (u  +  i.im,  q),  =  j  (u  —  ±lm,  q) .  e^~"  , 

while  also,  by  the  same  equation, 


Thus  the  expression 

^SOT  (u  —  i  ft™)  +  X_m  (u)  —  \m  (u)  +  kin  (mq  —  m'q) 

must  be  an  integral  multiple  of  2?™'.  This  is  immediately  seen  to  require 
only  that  2  (mq'  —  m'q  —  mm')  be  integral  for  all  integral  values  of  m,  m'. 
Hence  the  necessary  and  sufficient  condition  is  that  q  and  q'  consist  of  half- 
integers.  In  that  case  we  prove  as  before  that  ^  (u,  q)  is  odd  or  even 
according  as  4>qq'  is  an  odd  or  even  integer. 

192.     In  what  follows  in  the  present  chapter  we  consider  only  the  case  in 
which  b  =  ITTT,  r  being   the   matrix   of  the    periods   of  Riemann's   normal 

integrals  at  the  second  kind  of  period  loops.  And  if  if  a,...,  wj  a  denote 
any  p  linearly  independent  integrals  of  the  first  kind,  such  as  used  in  §§  138, 
139,  Chap.  VII.,  the  matrix  h  is  here  taken  to  be  such  that 


7  ,  a  ,  x,  a 

=hi>1ul     +  ......  +  hitpup  ,        (i-l,  2,  ..., 

so  that  h  is  as  in  §  139,  and 

•  (u*>  a,  q)  =  eauz  ©  0*'  «  q), 


where  u  =  ux>  a. 

From  the  formula 

S-  (u  +  flm)  =  ea»(«+jo»)-««w»'  ^  (w), 

wherein  m,  m'  denote  rows  of  integers,  we  infer,  using  the  abbreviation 

a 

£(w)  =  ^.logS-O)> 
that 

&  (u  +  flm)  -  &  (u)  =  2  (rjit  1  m,  +  ......  +rjiiltmp  +  iifiilm1t+  ......  -i-^.^ 

particular  cases  of  this  formula  are 

f  /  (M,  +  2a>lf  ,.,    .  .  .  ,  up  +  2a,pt  ,.)  =  £  (u)  +  2^  r, 
&  (w,  +  20)',,  r,  ...,  up  +  2a)'p!  r)  =  Si  CM)  +  2i/i,  r> 


288  THE   DIFFERENCE   OF   TWO    f   FUNCTIONS  [192 

Thus  if  us  be  the  argument 


where  MI  ,  ...,?4'a  are  any  P  linearly  independent  integrals  of  the  first 
kind,  and  the  matrix  a  here  used  in  the  definition  of  &  (u)  be  the  same  as 
that  previously  used  (Chap.  VII.  §  138)  in  the  definition  of  the  integral 

L^  ,  so  that  the  matrices  ?;,  rf  will  be  the  same  in  both  cases,  then  it 
follows  that  the  periods  of  the  expression 


regarded  as  a  function  of  x,  are  zero. 

193.     And  in  fact,  when  the  matrix  a  is  thus  chosen,  there  exists  the 
equation 


—  £;•  (ux>  m  —  ux>  '  m'  —  ......  -  ux">  mt>)  +  &  (ua>  m  —  ux»  Wi  -  ......  -  ux">  m*) 

TX.  &    .      ^*     ~         r  /  \          /  \T 

=  L'   +2  vr>i  [(xr,  x)  -  (xr,  a)] 


r=l 


=-  , 


wherein  vr>  i  denotes  the  minor  of  the  element  /^-  (xr)  in  the  determinant 
whose  (r,  i)th  element  is  pi(xr),  divided  by  this  determinant  itself;  thus 
vr,i  depends  on  the  places  xlt  ...,  xp  exactly  as  the  quantity  vr>  {  (Chap.  VII. 
§  138)  depends  on  the  places  c1}  ...,  cp. 

For  we  have  just  remarked  that  the  two  sides  of  this  equation  regarded  as 
functions   of  x  have  the  same  periods  ;   the  left-hand  side   is  only  infinite 

at  the  places  xlt  ...,xp;  if  in  Lfa,  which  does  not  depend  on  the  places 
GI,  ...,  Cp  used  in  forming  it  (Chap.  VII.  §  138),  we  replace  c1}  ...,  cp  by 
x1,  ...,  xp,  it  takes  the  form 

-p,a;,  a  -^x,  a       _  .  x,  a  x,  a, 


and  becomes  infinite  only  at  the  places  acl}  ...,acp.  Hence  the  difference 
of  the  two  sides  of  the  equation  is  a  rational  function  with  only  p  poles, 
#j,  ...,  xp,  having  arbitrary  positions.  Such  a  function  is  a  constant  (Chap. 
III.  §  37,  and  Chap.  VI.)  ;  and  by  putting  x  =  a,  we  see  that  this  constant  is 
zero. 

194.     It  will  be  seen   in   the   next   chapter  that  in   the   hyperelliptic 
case  the  equation  of  §  193  enables  us  to  obtain  a  simple  expression   for 
£i  (ux>  m  —ux»m>  —  ......  —  u^'  mp)  in  terms  of  algebraical  integrals  and  rational 

functions  only.     In  the  general  case  we  can  also  obtain  such  an  expression*  ; 

*  See  Clebsch  und  Gordan,  Abels.  Functnen.  p.  171,  Thomae,  Crelle,  LXXI.  (1870),  p.  214, 
Thomae,  Crelle,  ci.  (1887),  p.  326,  Stahl,  Crelle,  cxi.  (1893),  p.  98,  and,  for  a  solution  on  different 
lines,  see  the  latter  part  of  chapter  XIV.  of  the  present  volume. 


194]  EXPRESSED    BY   ALGEBRAICAL    INTEGRALS.  289 

though  not  of  very  simple  character  (§  196).     In  the  course  of  deriving  that 
expression  we  give  another  proof  of  the  equation  of  §  193. 

The  function  of  x  given  by  &  (%*•»«;  |/3,  |a)  will  have  p  zeros,  unless 
^  (ux>  m  +  £ft0,  a)  vanish  identically  (§§  179,  180)  ;  we  suppose  this  is  not  the 
case.    Denote  these  zeros  by  m/,  ...,  mpf.    Then  (Prop.  X.  §  184)  the  function 
^  (u*>  m  -  «*•  '  '«•'  -  ......  -  U*P>  'V  ;  £/3,  £a)  will  vanish  when  as  coincides  with 

#1,  a?2,  ...,  or  xp.     Determining  mlt  ...  ,  mp  so  that 


ump,mp'  = 


and  supposing  the  exact  value  of  the  left-hand  side  to  be  £  flftt  „  +  £lk>  h> 
where  k,  h  are  integral,  this  function  is  equal  to 

%(u*,m_ux>,mi  _  ......  _  uXp,mit  _  in^a  -  nt>h  ;  ££.  |  a), 

and  this,  by  equation  (L)  is  equal  to 


where  u  =  ux>  m  —  ux>  >  m>  —  ......  —  uxi»  mv  —  £lk  h. 

Therefore  (§  190)  the  expression 


-W^.^/-  ......  _w^,rV;     /9, 

is  equal  to 


we  may  write  this  in  the  form 


the  expression  is  therefore  equal  to 

;,  m  _    ^,  mt  _ 


,  m  _       ,,  m,  _ 

where 

is  equal  to 

or 

-2a(U-V)(r-s), 
that  is 


B-  19 


290  DEDUCTION   OF   A   FORMULA  [194 

which  denotes 

£     vv  x,  M     *,,  nr. 

—  2,  (2S2af,j«,-     w;      ). 

T  =  1       1 ,  j 

Hence,  by  Prop.  XIII.  §  187,  supposing  that  the  matrix  a,  here  used,  is  the 
same  as  that  used  in  §  138,  Chap.  VII.,  and  denoting  the  canonical  integral 

TT  a;,  a     ~  J}    Ji  x,  a    z,  c 

_  •/     >        ^      /f  -jy  -i/ 

J-J.,y      ^»  A<    — W        ^W      U.J-      J     tt-j«  tfr^f  j 

r=ls=l 

which  has  already  occurred  (page  194),  by  Rxz'>c  ,  we  have 


195.     From  the  formula 
p     x,p  <bux'm-ux» 


X,  *  <^Sux,  m_  WMI,  Wi  —  ...  —  ufp>  mP 

since 

Xr,    Mr  *r.^  £      /V.^r*,* 

-n-ar,  /a      =  f  x,  /x      +  ^  ui          Li      ' 

t  =  l 

we  obtain 

P    D^.,^       P  ^     •+*;*.*"',      *(u*-m-U)  /*(u»>™-  U) 
A     *"     ^-ir-l^  10g^(^---  J70)/  ^(^'Wl-  Z/o) 

where 


and  therefore 

U-U0=%  u*"»*. 

r  =  l 

Hence,  differentiating, 

5  |^f  [(*,,  «)  -  (av,  A*)]  +  Lr  -  -  Si  (**•  m  -  U]  4-  C,  (^  -  -  IT), 

r=ldC'i 

where 


but,  from 


where  rfa?1;  ...,  rf^  denote  the  infinitesimals  at  xlt  ...,  xp,  we  obtain 

9a;r  _         dxr 

dwr^^' 

thus 

P 

-  ?i  (w*-  m  -  U)  +  &  (M*  m  -  t^)  =  4'  m  +  2  J>r,  {  [(xr  ,  x)  -  fa,  /*) 

r=l 

which  is  the  equation  of  §  193. 


196]  TO   EXPRESS   A   SINGLE   £  FUNCTION.  291 

196.     From  the  equation 


differentiating  in  regard  to  a;,  we  obtain  an  equation  which  we  write  in 
the  form 


F?  ^=ft  (x)  [f  ,  («*.  »  -  17)-  f  r  (M*.  »  -  £T0)], 

r=l  r=l 


where   U= 


Thus,  if  we  take  for  ft  ,  .  .  .  ,  ft,  places  determined  from  a;  just  as  mlt  ...,  mp 
are  determined  from  m,  so  that 

(m,  ft,  ...,ft)  =  (x,  TOJ,  ...,  mp), 

the  arguments  ux>  m-  U0  will  be  =  0  ;  as  the  odd  function  £V  (u)  vanishes  for 
zero  values  of  the  argument,  we  therefore  have  (§  192),  writing  Hp  for  the 
exact  value  of  ux>  m  -  U0) 


r=l 
P 


C)  £V  (lix'  m  —  llz> '  w>  —  ...  —  UZP  >  mr>  —  ftp) 
r=l 

V        /   \r   i    z 

=  —    Z,  ft-  (X)  %r  (Wz»  ^  +  . . .  +  MZP'  **»), 
r=l 

If  in  this  equation  we  put  x  at  TO  we  derive 

p 

1Tfzii  ™i     .  |^    Jp^P'  'm^ V  /       \  y    /     Z      Wl      i  Zm\  /TVT\ 

where  ^1;  ...,  zp  are  arbitrary. 

If  however  we  put  x  in  turn  at  p  independent  places  clt  ...,  cp,  and 
denote  the  places  determined  from  a,  as  ml}  ...,  TOP  are  determined  from 
m,  by  c^  !,  ...,  Citp,  so  that 

(\  /  \ 

/•  •     fjfYl                   nffl     i  —  I  /yi")      /^ .  /* .        i 

f  1  J       »»H    )        •   •   •    y      IIVipI     I     f/(/j      (y-^       J  j        .    ,    .     ;       C/^       ?>/» 

we  obtain  p  equations  of  the  form 


Suppose  then  that  x,  xl,  ...,  xp  are  arbitrary  independent  places;   for 
z-i,  ...,  zp  put  the  places  xijly  ...,  xiif  determined  by  the  congruence 

(x,  xit  j,  .  .  .  ,  xit  p)  =  (d,  xl}  ...,xp)\ 

then,  if  ftQ  denote  a  certain  period,  —  uXi'  1J  Ci)i  —  ...  —  uXi'*»  C<)P  is  equal  to 
HQ  +  ux>  m  -  uxi  '  mi  -  ......  -  ux»>  m",  and  we  have 

j»*<.  i  -  ci,  i    ,  ,  JJT  *i,  P,  cf,  P  _    ^         ,    }  L, 

t'i  '  *       fc  ~    —  A4/'  X6'/'  br 


xp, 


19—2 


292  INTRODUCTION    OF   THE    $>   FUNCTIONS;  [196 

therefore 


X>  «. 

-u       -...-          = 


V      .         rvxr,l 

=  2,  vr>  i  [t  Cr 


where  vr>  i  is  the  minor  of  ^i  (cr)  in  the  determinant  whose  (r,  s)th  element  is 
fa  (0^,  divided  by  the  determinant  itself. 

In  particular,  when  the  differential  coefficients  ^  (x),  .  .  .  ,  pp  (x)  are  those 

r  x 
already  denoted  (§  121,  Chap.  VII.)  by  wl  (x),  ...,wp  (x},  and  Vf  a  =  I  wi(x)dtx, 

J  a 

and  the  paths  of  integration  are  properly  taken,  we  have* 


*' 


(  V*'  m  -  Vl>    l 


197.  A  further  result  should  be  given.  Let  #,  x1}  ...,  xp  be  fixed 
places.  Take  a  variable  place  z,  and  thereby  determine  places  ziy  ...,zp, 
functions  of  z,  such  that 

(x,  zlt  ...,  Zp)  =  (z,  «i,  ....  a?P). 
Then  from  the  formula 


z,  a 


i  r/  *        *  *.-,      Zg 

+2  vs>  i  [(zs,  z)  -  (zs,  a)]  -=-  , 


=i 


=- 


wherein  vs,  i  is  formed  with  zl}  .  .  .  ,  zp  ,  we  have,  by  differentiating  in  regard 
to  z  and  denoting  —  —  ^  (M)  by  g)^  j  (w), 


3  =  1 


'  dt 
where  U=uz'  m  —  uz"  m>  — _u2*'mp,   U  =  ua<  m  —  MZ»  w-  — —  ifr-  mv. 

In  this  equation  a  is  arbitrary.     Let  it  now  be  put  to  coincide  with  z  ; 
hence 


*  This  form  is  used  by  Noether,  Math.  Annal.  xxxvn.  (1890),  p.  488. 


197]  THEIR  ALGEBRAICAL   EXPRESSION.  293 

Therefore 

ft,  (IT) 


f=l 


=  D;     I  ^  (A)  /if'  B  +  I  ««  (A;)  [(*„  ^)  -  (^  a)]       1  , 


where  A'  means  a  differentiation  taking  no  account  of  the  fact  that  zl}  ...,  zp 
are  functions  of  z, 


U=i 


,  «  ;    k,  Z,,   .  .  .  ,  Zp)l, 


in  which  form  the  expression  is  algebraically  calculable  when  the  integrals 
L*'a  are  known  (Chap.  VII.  §  138), 

=  D'z  \  rj  a  -  ty  (z,  a  ;  k,  zlt  .  .  .  ,  zp)  -  22Sar>  ,  /*.,  (/.;)  w 
where  c  is  an  arbitrary  place  ;  and  this  (cf.  Ex.  iv.  §  125) 


p    P 


=  -  W(z;  k,  zlf  ...,  fp)-2  S    S 

r=l*=l 

If  now 


so  that 


=  Uk>  m  -  Uk>  '  7ni  -  ......  —  U*l» 

and 

(a?,  ^,  ...,  fp)  =  (^,  a?lf  ...,  a^), 

(ar,  A-j,  ...,  kp)=  (k,  ar1}  ...,  ajp), 
then  the  formula  is 


1   3  r=l«-l 


by  Ex.  iv.  §  125. 


=  W(k-  z,k1,...ikp)  +  2  I   I  ar, 

r=ls=l 


294  EXAMPLES.  [197 

By  the  congruences 


Uz»'  ^  =  Uz>  x 


the  places  zl}  ...,zp  are  algebraically  determinable  from  the  places  x,  xl  ,  .  .  .,  xp,  2, 
and  therefore  the  function  W  '  (z;  k,  zl}  ...,  zp)  can  be  expressed  by  x,  xlt  ..., 
xv,  k,  z  only.  In  fact  we  have 


/  \       r\ 

The  interest  of  the  formula  lies  in  the  fact  that  the  left-hand  side  is  a 
multiply  periodic  function  of  the  arguments  U1)  ...,  Up. 

A  particular  way  of  expressing  the  right-hand  side  in  terms  of  x,  xlt ...,  xp,  2,  k  is  to 
put  down  %p(p  +  l}  linearly  independent  particular  cases  of  this  equation,  in  which  the 
right-hand  side  contains  only  x,  xlt  ...,  xp,  z,  k,  and  then  to  solve  for  the  \p(p  +  l) 
quantities  j^y.  Since  ^  (z,  a  ;  k,  z1}  ...,  zp)  vanishes  when  k  =  zp,  we  clearly  have,  as  one 
particular  case, 

22J0-  •  (uz>  m—  uZl'  mi  —          —  uss>'''m''']u-(z}iLt(z}  =  DD    Rz' a 
ij  *»    «/-.  c' 

and  therefore 

n")  fH  (x)  H  fa)  =  DXDX  Rx>  a  ,          (N) 

'        i)"i.  »   C 

and  there  are^>  equations  of  this  form,  in  which  xlt  ...,  xp  occur  instead  of  xr. 
If  we  determine  ,%\',  ... ,  x'p_l  by  the  congruences 

so  that  $1,  ...,  xfp,1  are  the  other  zeros  of  a  ^-polynomial  vanishing  in  xlt  ...,  a?7,_1, 
we  can  infer  p  —  1  other  equations,  of  the  form 

i  j  *i- ,  a ' 

where  r=l,  2,  ...,(/»- 1).     Here  the  right-hand  side  does  not  depend  upon  the  place  x. 
And  we  can  obtain  p  such  sets  of  equations. 

We  have  then  sufficient  *  equations.  For  the  hyperelliptic  case  the  final  formula  is 
given  below  (§  217,  Chap.  XL). 

198.     Ex.  i.     Verify  the  formula  (N)  for  the  case  p  =  1. 
Ex.  ii.     Prove  that 


is  a  rational  function  of  x,  xly  ...,  xp. 
Ex.  iii.     Prove  that  if 


then 


Deduce  the  first  formula  of  §  193  from  the  final  formula  of  §  196. 

*  The  function  %\j(u),  here  employed,   is  remarked,  for  the  hyperelliptic  case,  by  Bolza, 
Gottinger  Nachrichten,  1894,  p.  268. 


198]  ALGEBRAICAL  THEORY   OF   THE  THETA   FUNCTIONS.  295 

Ex.  iv.     Prove  that  if 

ei=r£i.«i  +  ......  +  rxc>;»'\ 

where  a^  ,  .  .  .  ,  at>  are  arbitrary  places,  and 

V  =  Vx>  m-  VX}>  mi—         -  Vx>"m>'  =  VCi'  m  -  Vx'-1'  ™l  -      ...  -  VXi>>"  m>' 
v       f  r  ,.  r  ,.  r 

then 

VJ—  Wff   •    f      v  -r       ^ 

017  —   "  Vct  >    c/r>-*'t,  1>  •••>  •*%  p/> 

where  W  denotes  the  function  used  in  Ex.  iv.  §  125  ;  it  follows  therefore  by  that  example, 

that  „  ;;*  =  ^J£  .     Hence  the  function 
o  Vr     o  YI 

<^F1  +  ......  +  QpdVv 

is  a  perfect  differential  ;  it  is  in  fact,  by  the  final  equation  of  §  196,  practically  equivalent 
to  the  differential  of  the  function  log  6  (  Vx>  m  -  VXl<  m'  -  ......  -  VXf'  '"").     Thus  the  theory 

of  the  Riernann  theta  functions  can  be  built  up  from  the  theory  of  algebraical  integrals. 
Of.  Noether,  Math.  Annal.  xxxvu.  For  the  step  to  the  expression  of  the  function  by  the 
theta  series,  see  Clebsch  arid  Gordan,  Abelsche  Functionen  (Leipzig,  1866),  pp.  190  —  195. 

Ex.  v.     Prove  that  if 

(m2,  Xi,  j,  ...,  x\p,  zlt  ...,zp)  =  (a2,  m*,  ..  ,  mj(2) 
then 


Ex.  vi.     Prove  that 

-  2  w(2)[^(^'m-^"m'-  ......  -ux»m')-Ci(ua'm-v*l'mi-  ......  -ux"'m^] 

i  =  l 

f-,x,  a       ,   ,  \ 

=  FZ     -^(x,a;  z,xlt  ...,  xp). 

Ex.  vii.     If 


prove  that 

log  ^  (ux'm-  ux»  m>  -  ......  -ux"  m>) 

=  A+Alu*'a  +  ......  +ApUp'a+  I 

where  A,  Alt  ...,  Ap  are  independent  of  x. 

Ex.  viii.     Prove  that 

-  2  Mr  (oO  pf,  r(«*'w  -«*''"'>-  ......  -M*>.»")=  2  tr 

»•  =  !  r  =  1 

where  a,  c  are  arbitrary  places  and  the  notation  is  as  in  §  193. 


[199 


CHAPTER  XL 

THE   HYPERELLIPTIC   CASE   OF   RlEMANN's   THETA   FUNCTIONS. 

199.  WE  have  seen  (Chap.  V.)  that  the  hyperelliptic  case*  is  a  special 
one,  characterised  by  the  existence  of  a  rational  function  of  the  second 
order.  In  virtue  of  this  circumstance  we  are  able  to  associate  the  theory 
with  a  simple  algebraical  relation,  which  we  may  take  to  be  of  the  form 

7/2  =  4  (as-  fll)  ...  (x  -  ap)  (x  -  c,}...(x-  cp+l}. 

We  have  seen  moreover  (Chap.  X.  §  185)  that  in  the  hyperelliptic  case,  when 
p  is  greater  than  2,  there  are  always  even  theta  functions  which  vanish 
for  zero  values  of  the  argument.  We  may  expect,  therefore,  that  the  investi 
gation  of  the  relations  connecting  the  Riernann  theta  functions  with  the 
algebraical  functions  will  be  comparatively  simple,  and  furnish  interesting 
suggestions  for  the  general  case.  It  is  also  the  fact  that  the  grouping  of 
the  characteristics  of  the  theta  functions,  upon  which  much  of  the  ultimate 
theory  of  these  functions  depends,  has  been  built  up  directly  from  the 
hyperelliptic  case. 

It  must  be  understood  that  the  present  chapter  is  mainly  intended  to 
illustrate  the  general  theory.  For  fuller  information  the  reader  is  referred  to 
the  papers  quoted  in  the  chapter,  and  to  the  subsequent  chapters  of  the 
present  volume. 

*  For  the  subject-matter  of  this  chapter,  beside  the  memoirs  of  Bosenhain,  Gopel,  and 
Weierstrass,  referred  to  in  §  173,  Chap.  X.,  which  deal  with  the  hyperelliptic  case,  and  general 
memoirs  on  the  theta  functions,  the  reader  may  consult,  Prym,  Zur  Theorie  der  Functionen 
in  einer  zweiblattrigen  Flache  (Zurich,  1866) ;  Prym,  Neue  Theorie  der  ultraellip.  Funct. 
(zweite  Aus.,  Berlin,  1885);  Schottky,  Abriss  einer  Theorie  der  Abel.  Functionen  von  drei 
Variabeln  (Leipzig,  1880),  pp.  147 — 162  ;  Neumann,  Varies,  iiber  Riem.  Theorie  (Leipzig,  1884)  ; 
Thomae,  Summlung  von  Formeln  welche  bei  Amvendung  der . .  Roscnhaiii'schen  Functionen  gebraucht 
u-erden  (Halle,  1876) ;  Brioschi,  Ann.  d.  Mat.  i.  x.  (1880),  andt.  xiv.  (1886) ;  Thomae,  Crelle,  LXXI. 
(1870),  p.  201 ;  Krause,  Die  Transformation  der  hyperellip.  Funct.  erster  Ordnung  (Leipzig,  1886); 
Forsyth,  "  Memoir  on  the  theta  functions,"  Phil.  Trans.,  1882  ;  Forsyth,  "  On  Abel's  theorem," 
Phil.  Trans.,  1883  ;  Cayley,  "Memoir  on  the  .  .  theta  functions,"  Phil.  Trans.,  1880,  and  Crelle, 
Bd.  83,  84,  85,  87,  88;  Bolza,  Gottinger  Nachrichten  1894,  p.  268.  The  addition  equation  is 
considered  in  a  dissertation  by  Hancock,  Berlin,  1894  (Bernstein).  For  further  references  see  the 
later  chapters  of  this  volume  which  deal  with  theta  functions. 


200] 


THE   ZEROS. 


297 


200.  Throughout  this  chapter  we  suppose  the  relative  positions  of  the 
branch  places  and  period  loops  to  be  as  in  the  annexed  figure  (4),  the  branch 
place  a  being  at  infinity. 

Fig.  4. 


In  the  general  case,  in  considering  the  zeros  of  the  function  S  (ux>  m  —  e), 
we  were  led  to  associate  with  the  place  m,  other  p  places  mlt  ...,  mp,  such 
that  *b(ux>  m)  has  ml,  .,.,  mp  for  its  zeros  (Chap.  X.  §  179).  In  this  case  we 
shall  always  take  m  at  the  branch  place  a,  that  is  at  infinity.  It  can  be 
shewn  that  if  6,  6'  denote  any  two  of  the  branch  places,  the  p  integrals 

Hi    ,  ... ,  Up     are  the  p  simultaneous  constituents  of  a  half-period,  so  that 

ur'     =  ni!  &>r,  i  + +  mpa>,.t  p  +  m^w'r^  l  + +  WpVr,  p,     (r  =  1 ,  2,  . . . ,  p), 

wherein  mly  ...,  nip,  m/,  ...,  mp  are  integers,  independent  of  r ;  this  fact  we 
shall  often  denote  by  putting  w&'6'  =  £fl.  It  can  further  be  shewn  that  if, 
6  remaining  any  branch  place,  6'  is  taken  to  be  each  of  the  other  2p  +  l  branch 
places  in  turn,  the  2p  + 1  half-periods,  ub>  v,  thus  obtained,  consist  of  p  odd 
half-periods,  and  p  +  1  even  half-periods.  Thus  if  the  branch  places,  &',  for 
which  ub'b'  is  an  odd  half-period  be  denoted  by  61}  ...,  bp,  we  have,  necessarily, 
S-  (?i&.  &i)  =  0, ... ,  S-  (ub'  V)  =  0,  and  we  may  take,  for  the  places  m,  mlt  ...,  mp, 
the  places  b,  b1}  ...,  bp.  In  particular  it  can  be  shewn  that,  when  for  6  the 
branch  place  a  is  taken,  and  the  branch  places  are  situated  as  in  the  figure 
(4),  each  of  ua>  ai,  ...,  ua>  ap  is  an  odd  half-period.  We  have  therefore  the 
statement,  which  is  here  fundamental,  the  function  <&(ux> a  —  ux*>  a>  — . . .  —  uxv  ap) 
has  the  places  xl}  ...,  xp  as  its  zeros.  It  is  assumed  that  the  function 
S-  (ux< a)  does  not  vanish  identically.  This  assumption  luill  be  seen  to  be 
justified. 

For  our  present  purpose  it  is  sufficient  to  prove  (i)  that  each  of  the 
integrals  ub> y  is  a  half-period,  (ii)  that  each  of  the  integrals  ua>  a>,  . . . ,  ua'  "P  is 
an  odd  half-period.  In  regard  to  (i)  the  general  statement  is  as  follows:  Let 
the  period  loops  of  the  Riemann  surface  be  projected  on  to  the  plane  upon 
which  the  Riemann  surface  is  constructed,  forming  such  a  network  as  that 
represented  in  the  figure  (4)  ;  denote  the  projection  of  the  loop  (ar)  by  (Ar), 
and  that  of  (br)  by  (Br),  and  suppose  (Ar),  (Br)  affected  with  arrow  heads,  as  in 


298 


THE   ZEROS. 


[200 


the  figure,  whereby  to  define  the  left-hand  side,  and  the  right-hand  side  ; 
finally  let  a  continuous  curve  be  drawn  on  the  plane  of  projection,  starting 
from  the  projection  of  the  branch  place  b'  and  ending  in  the  projection  of  the 
branch  place  b  ;  then  if  this  curve  cross  the  loop  (Ar)  mr  times  from  right  to 
left,  so  that  mr  is  either  +  1  or  —  1,  or  0,  and  cross  the  loop  (Br)  mr'  times 
from  right  to  left,  we  have 


b,b' 

ur     =  wijft),^  j  4- 


-f 


mptor>p. 


Thus,  for  instance,  in  accordance  with  this  statement  we  should  have 

«r  *  —  —  »'r,  u  and  uCr'ai  =  a>ri  1  —  a)r>  2,  and  it  will  be  sufficient  to  prove 
the  first  of  these  results  ;  the  general  proof  is  exactly  similar.  Now  we  can 
pass  from  cx  to  a1;  on  the  Riemann  surface,  by  a  curve  lying  in  the  upper 


Fig.  5. 


sheet  which  goes  first  to  a  point  P  on  the  left-hand  side  of  the  loop  (6j), 
and  thence,  following  a  course  coinciding  roughly  with  the  right-hand  side  of 
the  loop  (ttj),  goes  to  the  point  P',  opposite  to  P  on  the  right-hand  side  of 
(61),  and  thence,  from  P',  goes  to  au.  Thus  we  have 


=u       — 


On  the  other  hand  we  can  pass  from  d  to  ax  by  a  path  lying  entirely  in  the 
lower  sheet,  and  consisting  of  two  portions,  from  ca  to  P,  and  from  P'  to  Oj, 
lying  just  below  the  paths  from  cx  to  P  and  from  P'  to  Oj,  which  are  in 
the  upper  sheet.  Thus  we  have  a  result  which  we  may  write  in  the  form 


1(  c,        ,    P, 

ur      =  (u 


/    &i,  -P\/ 

(ur      )  . 


f(x  1)  _ 
But,  in  fact,  as  the  integral  ux>  a  is  of  the  form  I   *    —  ?~l  dx,  and  y  has 

different  signs  in  the  two  sheets,  we  have 

P, 


, 

(u 


P,CI 


,    ,    a^P'.,  a-i,  P" 

}  and  (ur      )  =  —  ur 


201]  THE   HALF-PERIODS.  299 

Therefore,  by  addition  of  the  equations  we  have 


u.       =  —  a) 


r,  It 


which  proves  the  statement  made. 

In  regard  now  to  the  proof  that  ua-  °»,  .  .  .  ,  ua>  "v  are  all  odd  half-periods,  we 
clearly  have,  in  accordance  with  the  results  just  obtained, 

tf  ai  =  <oft  i  -  (t»rt  i+l  +  a>'r>  i+1)  -  ......  -  («,._  p  +  a,',,  „)  +  (0,',,  j  +  ......  +  m'fi  p), 

which  is  equal  to 

(m'r,  1  +  to'r,  2  +  ......  +  0)'r>i)  +  (ft,,,  i  —  ft)rj  i+1  -  ......  —  ft),;  p\ 

and  if  this  be  written  in  the  form 

Wjft),.,  j  +  ......  +  mpco,.t  p  +  mi'to'r,  i  +  ......  -1-  m'pto'r,  p 

we  obviously  have  WjW/  +  ......  +  mpmp'  =  1. 


Ex.  i.  We  have  stated  that  if  b  be  any  branch  place  there  are  p  other  branch  places 
&!,  62,  ...,  bp,  such  that  ub'  \  ub<  6%  ...,  ub>  b*  are  odd  half-periods,  and  that,  if  b'  be  any 
branch  place  other  than  6,  6,  ,  ...  ,  6P>  w6'  6'  is  an  even  half-  period.  Verify  this  statement  in 
case  p  =  2,  by  calculating  all  the  fifteen,  =£6  .  5,  integrals  of  the  form  w6-6',and  prove  that 
when  b  is  in  turn  taken  at  a,  c,  c1?  c2,  «1}  a.2  the  corresponding  pairs  bly  b2  are  respectively 


Prove  also  that 


Ex.     ii.     The  reader  will  find  it  an  advantage  at  this  stage  to  calculate  some  of  the 
results  of  the  second  and  fifth  columns  in  the  tables  given  below  (§  204). 

201.     Consider   now  the   2^  +  1   half-periods  ub>a  wherein  b   is   any  of 

the  branch  places  other  than  a.     From  these  we  can  form  (  ^  +    j   half- 

V     2     / 
periods,  of  the  form  ub-  a  +  ub>>  a,  wherein  b,  bf  are  any  two  different  branch 

places,  other  than  a,  and  (  ^  j  half-periods  of  the  form  ub<  a  +  uv'  a  +  uv,  «, 
where  b,  b',  b"  are  any  three  different  branch  places  other  than  a,  and  so 
on,  and  finally  we  can  form  tP~  J  half-periods  by  adding  any  p  of  the 
half-periods  ub>  a.  The  number 


is  equal  to  -1 +*[(*  + 1)*+']^,  or  to  2»-l,  and  therefore  equal  to  the 
whole  number  of  existent  half-periods  of  which  no  two  differ  by  a  period,  with 


300  THE   ASSOCIATION   OF   THE   HALF-PERIODS  [201 

the  exclusion  of  the  identically  zero  half-period  ;  we  may  say  that  this  number 
is  equal  to  the  number  of  incongruent  half-periods,  omitting  the  identically 
zero  half-period. 

And  in  fact  the  22^  —  1  half-periods  thus  obtained  are  themselves  incon 
gruent.     For  otherwise  we  should  have  congruences  of  the  form 


'  ft 


wherein  any  integral  ubK>a  that  occurs  on  both  sides  of  the  congruence  may 
be  omitted.  Since  every  one  of  these  integrals  is  a  half-period,  and  therefore 
ub«>  a  =  —  ub«'  a,  we  may  put  this  congruence  in  the  form 

llb>  '  a  +  M6"  a  +  ......  +  M&"1'  a  =  0, 


and  here,  since  we  are  only  considering  the  half-periods  formed  by  sums  of 
p,  or  less,  different  periods,  m  cannot  be  greater  than  2j>>.  Now  this  con 
gruence  is  equivalent  with  the  statement  that  there  exists  a  rational  function 
having  a  for  an  w-fold  pole  and  having  b^  ...,  bm  for  zeros  of  the  first  order 
(Chap.  VIII.  §  158).  Since  a  is  at  infinity,  such  a  function  can  be  expressed 
in  the  form  (Chap.  V.  §  56) 

(as,  l)r  +  y(as,  !)„, 

and  the  number  of  its  zeros  is  the  greater  of  the  integers  2r,  2p  +  1  +  s.  Thus 
the  function  under  consideration  would  necessarily  be  expressible  in  the 
form  (x,  l)r.  But  such  a  function,  if  zero  at  a  branch  place,  would  be 
zero  to  the  second  order.  Thus  no  such  function  exists. 

On  the  other  hand  the  rational  function  y  is  zero  to  the  first  order  at  each 
of  the  branch  places  alf  ...,  ap,clt  ...,  cp,  c,  and  is  infinite  at  a  to  the  (2p+  l)th 
order  ;  hence  we  have  the  congruence 

ua"a+  ......  +  uap>  a  +  uc>  -a+  ......  +  UCP>  a  +  uc>  a  =  0. 

202.     With  the  half-period  of  which  one  element  is  expressed  by 


,  p, 
we  may  associate  the  symbol 


(KI  ,  K%  ,  .  .  .  ,   kp  \ 
KI  ,     A?2  ,     .  .  .  ,     Kp  I 


wherein  kg,  equal  to  0  or  1,  is  the  remainder  when  m,  is  divided  by  2.  The 
sum  of  two  or  more  such  symbols  is  then  to  be  formed  by  adding  the  2p 
elements  separately,  and  replacing  the  sum  by  the  remainder  on  division 


202]  WITH   THE    BRANCH    PLACES.  301 

by  2.     Thus  for  instance,  when  p=  2,  we  should  write  (      I  +  (m  ]  =  I    _)  . 

If  we  call  this  symbol  the  characteristic-symbol,  we  have  therefore  proved, 
in  the  previous  article,  that  each  of  the  22p  —  1  possible  characteristic-symbols 
other  than  that  one  which  has  all  its  elements  zero  can  be  obtained  as  the  sum 
of  not  more  than  p  chosen  from  2p  +  1  fundamental  characteristic-symbols, 
these  2p  +  I  fundamental  characteristic-symbols  having  as  their  sum  the  symbol 
of  which  all  the  elements  are  zero.  In  the  method  here  adopted  p  of  the 
fundamental  symbols  are  associated  with  odd  half-periods  (namely  those  given 
by  ua>  °'  ,  .  .  .  ,  ua'  ap),  and  the  other  p+  1  with  even  half-periods.  It  is  manifest 
that  this  theorem  for  characteristic-symbols,  though  derived  by  consideration 
of  the  hyperelliptic  case,  is  true  for  all  cases*.  We  may  denote  the  funda 
mental  symbols  which  correspond  to  the  odd  half-periods  by  the  numbers 
1,  3,  5,  ...,  2p  —  1,  and  those  which  correspond  to  the  even  half-periods 
by  the  numbers  0,  2,  4,  6,  ...,  2p,  reserving  the  number  2/>  +  1  to  represent 
the  symbol  of  which  all  the  elements  are  zero.  Then  a  symbol  which  is 
formed  by  adding  k  of  the  fundamental  symbols  may  be  represented  by 
placing  their  representative  numbers  in  sequence. 

Thus  for  instance,  for  p  =  2,  Weierstrass  has  represented  the  symbols 


H 

\uj 


H  H  H 

oi/  ui/  vou  vooy  voo 


respectively  by  the  numbers 

1         3024         5; 

j-     i  11  /10\  /00\      /10 

and,  accordingly,  represented  the  symbol  I      J,  which  is  equal  to  (       j  +  ( 

/5\ 

by  the  compound  number  02.     The  (       =  10  combinations  of  the  symbols 

\AJ 

1,  3,  0,  2,  4  in  pairs,  represent  the  2-^  —  6  symbols  other  than  those  here 
written.     Further  illustration  is  afforded  by  the  table  below  (§  204). 

In  case  p  =  3,  there  will  be  seven  fundamental  symbols  which  may  be 
represented  by  the  numbers  0,  1,  2,  3,  4,  5,  6.  All  other  symbols  are 
represented  either  by  a  combination  of  two  of  these,  or  by  a  combination  of 
three  of  them. 

It  may  be  mentioned  that  the  fact  that,  for^  =  3,  all  the  symbols  are  thus  represen  table 
by  seven  fundamental  symbols  is  in  direct  correlation  with  the  fact  that  a  plane  quartic 
is  determined  when  seven  proper  double  tangents  are  given. 

*  The  theorem  is  attributed  to  Weierstrass  (Stahl,  Crelle,  LXXXVIII.  pp.  119,  120).  A  further 
proof,  and  an  extension  of  the  theorem,  are  given  in  a  subsequent  chapter. 


302  NOTATION    FOR   THE    FUNCTIONS.  [203 

203.     If  in  the  half-period  ^flm>  m-,  of  which  an  element  is  given  by 


>  p  ^  i        ......  tr,  p, 


we  write  \mg  =  Mit  +  ^ks,  ^ms'  =  MS'  +  ^ks',  where  Ms,  M,'  denote  integers, 
and  each  of  ks,  ks'  is  either  0  or  1,  we  have  (cf.  the  formulae  §  190,  Chap.  X.) 


where 

X  =  [277  (M  +  W  +  2r/  (M'  +  IF)]  [it  +  to  (M  +  P)  -f  to'  (M'  +  P' 


and  therefore 

*  (u  ;  P,  £  k')  =  e-  *--«*•  *  (u  +  J  Hm,  ,„)• 

The  function  represented  by  either  side  of  this  equation  will  sometimes  be 
represented  by  *t(u  \^flm,^)  ;  or  if  inw,TO'  =i*6"  °-f  *^'«  +  ......  +w&"«,  the 

function  will  sometimes  be  represented  by  ^  (u  \  w&"  a  +  ......  +ub*<a),  or  by 


We  have  proved  in  the  last  chapter  (§§  184,  185)  that  every  odd  half- 
period  can  be  represented  in  the  form 


and,  when  there  are  no  even  theta  functions  which  vanish  for  zero  values  of 
the  argument,  that  every  even  half-period  can  be  represented  in  the  form 


in  the  hyperelliptic  case  every  odd  half-period  can  be  represented  in  the 
form 


and  every  even  half-period  ^fT,  for  which  ^(£fl')  does  not  vanish,  can  be 
represented  in  the  form 


and  (§  182,  Chap.  X.)  the  zeros  of  the  function  *t(ux'z  |fl)  consist  of  the 
place  z  and  the  places  n1}  ...,  np,  while  the  zeros  of  the  function  ^  (ux>  a  \  ^O') 
are  the  places  blt  ...,  bp.  In  case  p  =  2  there  are  no  even  theta  functions 
vanishing  for  zero  values  of  the  argument  ;  in  case  p  =  3  there  is  one  such 
function  (§  185,  Chap.  X.),  and  the  corresponding  even  half-period  £  fl"  is 
such  that  we  can  put 


204] 


TABLE. 


303 


wherein  a?,  is  an  arbitrary  place  and  xz  is  the  place  conjugate  to  xl.     Since 
then  ux<"  °2  =  —  uXi>  a*,  this  equation  gives 


now,  as  in  8  200.  we  easily  find 

O  J 

Ur'      =  —  (tor,  3  +  to'r,  i  +  &> 

and  therefore 


r,  2 


r,  a 


Thus  the  even   theta   function  which   vanishes  for   zero   values  of  the 


argument  is  that  associated  with  the  characteristic  symbol 

In  the  same  way  for  ^>  =  4,  the  10  even  theta  functions  which  vanish  for 
zero  values  of  the  argument  are  (§  185,  Chap.  X.)  associated  with  even  half- 
periods  given  by 


where  b  is  in  turn  each  of  the  ten  branch  places. 

204.     The  following  table  gives  the  results  for  p  =  2.     The  reader  is  recommended 
to  verify  the  second  and  fifth   columns.     The  set  of  p  equations  represented  by  the 

equation  (%Q.\  =  ml«>r>  l  +  m2<or,  2  +  m/w',,  i  +  «!•>',.,  2  is  denoted  by  putting  fcQ  =  $  f™1  ^  \  . 

\mlmzj 

/.     Six  odd  theta  functions  in  the  case  p  =  Z. 


Function 

We  have 

Weierstrass's 
number  asso 
ciated  with 
this  symbol 

Putting  the  corresponding  half- 
have  for  HI  respectively 

W> 

*"*  -*(   $ 

02 

(1) 

«2 

WiO 

**-»'(  Jl) 

24 

(3) 

;      •        - 

««,«» 

*"<«-i(_*}) 

04 

(13) 

a 

w> 

—  K-n) 

1 

(24) 

c 

9cei  (u) 

«c"c^(_!o) 

13 

(02) 

c* 

Sec,  (U) 

M  -»(?.}) 

3 

(04) 

- 

304 


VERIFICATION   OF   THE   THEORY 


[204 


77.     Ten  even  theta  functions  in  the  case  p  =  2. 


Function 

We  have 

Weierstrass's 
number  asso 
ciated  with 
this  symbol 

Putting  the  corresponding  half- 
period  ^w6!'  ai  +u62>  az,  we 
have  for  fcj  ,  fc2 

s«0 

k(     °°] 

*(   oo) 

5 

.       «,,«,        ' 

*.(*) 

ua'c  ~*\   oo) 

23 

(0) 

VOO 

1  /  °°\ 
***-*(    io) 

12 

(2) 

C  ,     C.J 

W<0 

1  /"   10\ 

~H  oij 

2 

(4) 

C  ,    Cj 

wo 

I/   10\ 

5v  oo; 

01 

(12) 

•,.    «2,C1  „ 

fetf* 

,  /o   o\ 

0 

(14) 

;     «2)C2 

V,  00 

^'—  *(-n) 

14 

(23) 

«1)tfl 

V*M 

/     01  \ 

~*\  ooy 

4 

(34) 

*x 

W«) 

«c,0i    =|^      Qij 

34 

(03) 

«n  « 

•Sea,  00 

1  ^-^ 

wc'ai=Hi  o) 

03 

(01) 

The  numbers  in  brackets  in  the  fourth  column  might  be  employed  instead  of  the 
Weicrstrass  numbers  ;  they  are  based  on  the  branch  places  according  to  the  corre 
spondence 


1      302 


But  the  Weierstrass  notation  is  now  so  fully  established  that  it  will  be  employed  here 
whenever  any  such  notation  is  used. 

It  should  be  noticed  that  the  letter  notation  for  an  odd  function  consists  always 
of  two  a's  or  two  c's  ;  the  letter  notation  for  an  even  function  contains  one  a  and  one  c. 

The  expression  of  the  half-period  associated  with  any  function  as  a  sum  of  not  more 
than  two  of  the  integrals  ub- a,  which  has  been  described  in  §  202,  is  of  course  immediately 
indicated  by  the  letter  notation  employed  for  the  functions. 


Ex.     Prove  that  if  a  = 


.=«.<». 


These  equations  effect  a  correspondence  between  five  of  the  odd  functions  and  the  branch 
places. 


205] 


OF   THE    LAST   CHAPTER 


305 


205.  Next  we  give  the  corresponding  results  for  p  =  3.  Each  half-period  can  be  formed 
as  a  sum  of  not  more  than  3  of  the  seven  integrals  ub-  a  (§  202)  ;  the  proper  integrals 
are  indicated  by  the  suffix  letters  employed  to  represent  the  function.  We  may  also 
associate  the  branch  places  with  the  numbers  0,  1,  2,  3,  4,  5,  6,  say,  in  accordance  with  the 
scheme 


!>       3,       5,       0,     2,      4,      6; 

then  the  functions  ^  (w),  &s(u),36(u)  will  be  odd,  and  the  functions  30(u),  92(u),  3t(u),S6(u) 
will  be  even  ;  and  every  function  will  have  a  suffix  formed  of  1  or  2  or  3  of  these  numbers. 
There  is  however  another  way  in  which  the  64  characteristics  can  be  associated  with  the 
combinations  of  seven  numbers,  and  one  which  has  the  advantage  that  all  the  seven 
numbers  and  their  21  combinations  of  two  are  associated  with  odd  functions,  while  all 
the  even  functions  except  that  in  which  the  associated  half-period  is  zero  are  associated 
with  their  35  combinations  of  three.  It  will  be  seen  in  a  later  chapter  in  how  many  ways 
such  a  scheme  is  possible.  One  way  is  that  in  which  the  numbers 

1,     2,     3,     4,     5,     6,     7 
are  associated  respectively  with  the  half-periods  given  by 


,  a  +  Uc3  ,  a 


uc, 


Uci> 


By  §  201  the  sum  of  these  integrals  is  =  0.  The  numbers  thus  obtained  are  given  in  the  second 
column.  Further  every  odd  half-period  can  be  represented  by  a  sum  u^,a-  u^ ,  «,  -  «w2,  «2) 
and  all  the  even  half- periods  except  one  as  a  sum  w^i,  OI  +  M&S,  «2  +  M^3)  «3  ;  the  positions  of 
nlt  n2  or  of  b^  b2,  63  are  given  in  the  fourth  column. 

7.     28  odd  theta  functions  for  p  =  3. 


»•.(«) 

^ttia.2  (U) 
°ata3  (u) 


1 

2 

3 

12 

13 

23 

74 

75 


001, 

010 
110 


- 


B, 


20 


306 


(tt) 


(«) 


BY   ACTUAL   CALCULATION 
Table  I.  (continued.} 


[205 


76 
56 
64 
45 


37 

27 
17 
14 
24 
34 
15 
25 
35 
16 
26 
36 
4 


uc,a 


/100 


110 

101 


001 
. 


010 
010 

101 


101\ 
10()  1 


i 
a  4.  Ma,  ,  a  +  w«2,  «  =  f  I          1 


001 

iioj 

) 


c  , 


c  ,  a3 


c  , 


C/7 
3>    W3 

a  ,  ^ 

a  ,  c2 

a  ,  c3 

a  ,  c 


205] 


OF   THE    FUNCTIONS. 

//.     36  even  characteristics  for  p  =  3. 


307 


bi      bz     b3 

»(„) 

,  /000\ 

a,     «2     a3 

Ba^w 

123 

^•^.«+^.-iQ 

*«       r       r 
"J     ^j      * 

MH) 

456 

uc>a                     =i(ooo) 

ct     c2     c3 

3Cl  (u) 

567 

Mc,,a                               =$(0°°} 

C        Ctf        Co 

**(«) 

647 

s*(oio) 

C        C3        Cj 

KM 

457 

UCi'a                   sKooi) 

1          2 

W) 

237 

z«c,  a  +  l<«i,«                   =1/^011\ 

2    \    1  AA   / 

\xuwy 

c      a2     «3 

v.<») 

317 

^,a  +  Ma2)a                    ^|(°01) 

C         Q>q       Oti 

&*(•) 

127 

uo,a  +  ua3,a                  ^t™} 

c      a,     «2 

3clfll  00 

234 

=^  \oooj 

**%*«) 

314 

»*H«-             si(JJJ) 

W«0 

124 

U0,a  +  Ua3,a                 ^iQ 

Cl     at     a2 

V,  («) 

235 

Mc2)  a  +  MBl,  a                 ^(°00) 

c,     o,     «3 

Q           /,,\ 
*!%•,  V'4,' 

315 

W%,.+^,a               =i(^) 

o.2     03     fll 

Sen  (u) 

125 

Mfi.,a  +  M«,,«                 -i^01^ 

5  \oiiy 

c2     «!     a2 

*w,  (») 

236 

^..^-            si(JJJ) 

i*M 

316 

««„«  +  ?<«,    a                  -if00°^ 

c3     a3     «j 

»W) 

126 

=^  \oooy 

3          1       ^2 

^«lC2C3  (M) 

156 

76a,,a  +  w(;2,a  +  ^3>«   =i(J}J) 

ft         f*         f* 
1          1 

SM^W 

164 

^.a  +  ^a  +  ^^Q 

Cti       Co      C 

5ftlClC,(«) 

145 

*..+*,.+*..  .jQ 

5-'(M) 

147 

Ma1,a  +  7/c,a  +  „<-,  ,  a  =  ^^  j 

20—2 


308 


METHODS   OF   NOTATION. 


[205 


Table  II.  (continued). 


V»H 

157 

ft_     /111\ 
=  *  \110J 

•9a,cc3  («) 

167 

*••+*•  +«fc.«iQ 

•satc.£3  (U) 

256 

-^-^--iQ 

«2      ^       C 

*W>(«0 

264 

^,.+^..+^.•4^ 

•J(l2C]C.2  (^) 

245 

a  4-                  c     rt-4^°10\ 

~^  yiooy 

«2      C3      C 

5a       (w) 

247 

2^(12  )   ^  -^-  ^C,   (I     -1-  1(C\  ,  (1  =  i    I                    j 

S«.2cc.2  («) 

257 

•^<l-2  ,  d  -|-  ^C,  rt     -i-  1(,C'2  j  &  =  -4  I 

V^M 

267 

7^CE-2  »  ^  -|-  ?£C,  Ct    -J-  ^^3  ,  (I  =  i  [                J 

AM.M 

356 

""•'••H"»*<H*'««*(J?J) 

a3     Cj     c 

*W.  0) 

364 

^•+—+-..s  *Q 

rto       <^2       " 

VMM 

345 

-'^-^—  Km') 

v_ei 

347 

^.^^.a+^.a^lQ 

Ct  0             CtJ             ^?0 

*M«<>) 

357 

•%.•+«•  VM.«-I^) 

**(.) 

367 

«...+«.  +—iQ 

It  is  to  be  noticed  that  every  odd  theta  function  is  associated  with  either  (i)  any 
single  one  of  at,  a2,  «3  or  (ii)  any  pair  of  ax,  a2,  a3  or  any  pair  of  c,  Cj,  c2,  c3,  or  (iii)  a 
triplet  consisting  of  one  of  c,  cu  c2,  c3  and  two  of  an  a2,  a3  or  consisting  of  three  from 
c,  c1?  c2,  c3.  This  may  be  stated  by  saying  that  odd  suffixes  are  of  one  of  the  forms 
or,  a2,  c2,  a2c,  c3.  Similarly  an  even  suffix  is  of  one  of  the  forms  c,  ac,  ac2,  a3. 

In  the  tables  just  given  the  fundamental  characteristic-symbols,  denoted  by  the  num 
bers  1 ,  2,  3,  4,  5,  6,  7,  are  those  associated  with  sums  of  integrals  which  may  be  denoted  by 


206]  EXPRESSION   OF   THETA   QUOTIENTS.  309 

We  can  equally  well  choose  seven  fundamental  odd  characteristic-symbols,  associated  with 
the  integrals  denoted  by  any  one  of  the  following  sets  : 

c  Cj  ,     c  c2  ,     c  c3  ,     c  «2«3,     c  aza^     c  «1a2>     Ciczc3 


e2c  ,     CgCj,     c2c3, 


The  general  theorem  is  —  it  is  possible,  corresponding  to  every  even  characteristic  «  ,  to 
determine,  in  8  ways,  7  odd  characteristics  a,  /3,  y,  *,  A,  /z,  v,  such  that  the  combinations 

a,  ft  y,  *,  A,  M,   «*,   f«j3,   ea/c,   eX/x 

constitute  all  the  28  odd  characteristics,  and  the  combinations 

f,  a/3y,  a*X,  /3y*c 

constitute  all  the  36  even  characteristics.     In  the  cases  above  f  =0.     The  proof  is  given  in 
a  subsequent  chapter. 

206.     Consider  now  what  are  the  zeros  of  the  functions 
^  (w),  &  («|  lA  •  «  +  ......  +  M6*'  a), 

where  blt  ...  ,bk  denote  any  k  of  the  branch  places  other  than  a  (k  $-p),  and  u 
is  given  by 


the  functions  being  regarded  as  functions  of  xl. 

The  zeros  of  S-  (u)  are  the  places  zlt  ...,  zp  determined  by  the  congruence 


or,  by 


Provided  the  places  a,x2,  ...,  xp  be  not  the  zeros  of  a  ^-polynomial,  that  is, 
provided  none  of  the  places  x2>  ...,xp  be  at  a,  and  there  be  no  coincidence 
expressible  in  the  form  #»  =  #;,  the  places  zlf  z2,  ...,zp  cannot  be  coresidual 
with  anyp  other  places  (Chap.  VI.  §  98,  and  Chap.  III.)  and  therefore  (Chap. 
VIII.  §  158)  this  congruence  can  only  be  satisfied  when  the  places  z1}  ...,zp 
are  the  places 

Cl,  X%  ,  X3  ,  .  .  .  ,  Xp  , 

these  are  then  the  zeros  of  ^  (u),  regarded  as  a  function  of  x^ 

The  two  places  for  which  .r  has  the  same  value,  and  y  has  the  same  value  with  opposite 
signs,  are  frequently  denoted  by  x  and  x. 


310  EXPRESSION   OF  THETA  QUOTIENTS  [206 

The   zeros   of  *b(u\ub>'a  +  ......  +  ubk>a)   are    to   be   determined   by   the 

congruence 

Ux"ai  +  ......  +Uxi»a"  +  Ubl>  a  +  ......  +  Ubk'a  =  Ux"  a  —  Mz"  a>  —  ......  —  Uzi»  ai>, 

or,  by 

w*i,  &i  +  W*2,  x*  +  ......  +  u*p,  *i>  +  M6«,  «  4.  ......  4.  M6fc,  a  =  0, 

which  we  may  write  also 

(z1}  z,,  ...,  zp,  a*"1)  =  (blt  .  .  .  ,  bk,  x.2)  .  .  .  ,  xp)  ; 
in  particular  the  zeros  of  S-  (u  ub>  a)  are  the  places  b,  x.2,  ...,xp. 

207.  Now,  in  fact,  if  the  sum  of  the  characteristics  qly  ...,  qn  differs  from 
the  sum  of  the  characteristics  r1}  .  ..,  rn  by  a  characteristic  consisting  wholly 
of  integers,  n  being  an  integer  not  less  than  2,  then  the  quotient 


;  rO  ......  *(*;  rn) 

is  a  periodic  function  of  w. 

For,  by  the  formula  (§  190,  Chap.  X.) 

^  (w  +  n,n;  g)  =  ex»(w)  +  27rz'()ft9'  -  m'«>  ^  (it  ;  q), 
where  m  denotes  a  row  of  integers,  we  have 

f(u  +  flm)  _  2iri  [wi(2(?,  _  2r/)  _  m,  (2  _  2r)-j 

755 

and  if  S^'  —  Sr',  Sg  —  2r,  each  consist  of  a  row  of  integers  the  right-hand 
side  is  equal  to  1. 

Hence,  when  the  arguments,  u,  are  as  in  §  206,  the  function  f(u)  is  a 
rational  function  of  the  places  xlt  ...,  xp. 

208.     It  follows  therefore  that  the  function 


*•(*) 

is  a  rational  function  of  the  places  xl,  ...,xp.  By  what  has  been  proved 
in  regard  to  the  zeros  of  the  numerator  and  denominator  it  has,  as  a  function 
of  a?!,  the  zero  b,  of  the  second  order,  and  is  infinite  at  a,  that  is,  at  infinity, 
also  to  the  second  order.  Thus  it  is  equal  to  M  (b  —  x^,  where  M  does  not 
depend  on  xv  As  the  function  is  symmetrical  in  xlt  x.2,  ...,xp,  it  must 
therefore  be  equal  to  K  (b  —  x^)  ...  (b  —  xp),  where  K  is  an  absolute  constant. 
Therefore  the  function 


may  be  interpreted  as  a  single  valued  function  of  the  places  xl}  ...,xp, 
on  the  Riemann  surface,  dissected  by  the  *2p  period  loops.  The  values  of 
the  function  on  the  two  sides  of  any  period  loop  have  a  quotient  which  is 
constant  along  that  loop,  and  equal  to  +  1. 


209]  BY   MEANS  OF   RATIONAL   FUNCTIONS.  311 

The  function  has  been  considered  by  Rosenhain*,  Weierstrass  f,  RiemannJ  and 
Brioschi§.  We  shall  denote  the  quotient  3  (u\u!>- *} I S  (u}  by  qb  (u).  There  are  2p  +  l  such 
functions,  according  to  the  position  of  b.  Of  these  ^  (u),  ...,  qaj>  (u)  are  odd  functions, 
and  q  (u),  qc  (u},  ...,  qc  (u)  are  even  functions.  The  functions  are  clearly  generalisations 
of  the  functions  \/x  =  sn  u,  \A~ #  =  cn  u,  \/l  —  fctx  =  dn  u,  obtained  from  the  consideration 
of  the  integral 

dx 


209.     Consider  next  the  function 

b»  a 


*  (111 1  ->ib, ,  a\  ^V  ( ii  i  -i/fyfcj  a\ 

r  \  *»I«F»*  / »j  \ M" ,  "<      / 

wherein  61;  ...,  6jfc  are  any  A;  branch  places  other  than  a.     We  consider  only 
the  cases  k  <  p  +  1.     By  what  has  been  shewn,  the  function  is  rational  in  xlt 

and  if  zlt  ...,  zp  denote  the  zeros  of  ^  (u  ub»a+ +&*.«)  the  zeros  of  the 

numerator,  as  here  written,  consist  of  the  places 

j_j  k—\ 

y  IV  fjK      1       nn  /y 

--  I  ,    .  .  •  ,    ^  i/ 1  U  ,    '     J         ,    •  •  •  >         /> 

and  the  zeros  of  the  denominator  consist  of  the  places 


Thus  the  rational  function  of  xl  has  for  zeros  the  places  zlt  ...,  zp,  ak~l, 
and,  for  poles,  the  places  blt  ...,  &&,  x.2,  ...,  xp.  It  has  already  been  otherwise 
shewn  that  these  two  sets  of  p  +  k  -  1  places  are  coresidual.  Now  any 
rational  function,  of  the  place  x,  which  has  these  poles,  can  (Chap.  VI.  §  89) 
be  written  in  the  form 

uy  +  v  (x  -  6Q  .  .  .  (x  -  bk) 
(x  —  &i)  .  .  .  (x  —  bk)  (x  —  x.^...(x  —  xp)  ' 

wherein  u,  v  are  suitable  integral  polynomials  in  x,  so  chosen  that  the 
numerator  vanishes  at  the  places  x2,  ...,  xp.  The  denominator,  as  here 
written,  vanishes  to  the  second  order  at  each  of  blt  ...,  bk,  and  also  vanishes 
at  the  places  x2,  x2,  ...,  xp,  xp. 

Let  X,  //,  be  the  highest  powers  of  x  respectively  in  u  and  v.  Then,  in 
order  that  this  function  may  be  zero  at  the  place  a,  that  is,  at  infinity,  to  the 
order  &—  1,  it  is  necessary  that  the  greater  of  the  two  numbers 


*  Memoires  par  divers  savants,  t.  xi.  (1851),  pp.  361  —  468. 

t  By  Weierstrass  the  function  is  multiplied  by  a  certain  constant  factor  and  denoted  by  al(u). 
£  In  the  general  form  enunciated,  as  a   quotient  of  products  of  theta  functions,    Werke 
(Leipzig,  1876),  p.  134  (§  27). 

§  Annali  di  Mat.  t.  x.  (1880),  t.  xiv.  (1886). 


312  DEDUCTION   OF   RELATIONS  [209 

(wherein  2  (  p  +  k  -  1)  is  the  order  of  infinity,  at  infinity,  of  the  denominator) 
should  be  equal  to  —  (&  —  !).  Since  one  of  these  numbers  is  odd  and  the 
other  even,  they  cannot  be  both  equal  to  —(&-!).  Further  in  order  that 
the  ratios  of  the  A,  +  /*  +  2  coefficients  in  u,  v  may  be  capable  of  being  chosen 
so  that  the  numerator  vanishes  in  the  places  x.2,  ...,  xp,  it  is  necessary  that 
X  +  M  +  1  should  not  be  less  than  p—  1.  And,  since  a  rational  function 
is  entirely  determined  when  its  poles  and  all  but  p  of  its  zeros  are  given, 
these  conditions  should  entirely  determine  the  function. 

In  fact  we  easily  find  from  these  conditions  that  the  case  2\+2p+  1  >2(/i-f&) 
can  only  occur  when  k  is  even,  and  then  X  =  %k  —  1,  /M  =p  —  1  —  ^k,  and 
that  the  case  2X  +  2p  +  1  <  2yu,  +  2k  can  only  occur  when  k  is  odd,  and  then 
X  =  £  (k  —  3),  p  =  p  —  ^  (k  +  1).  In  both  cases  X  +  /*  +  2  =p. 

By  introducing  the  condition  that  the  polynomial  uy  +  v(x-b1)  ...  (a  -  bk) 
should  vanish  in  the  places  #2,  ...,  xp  we  are  able,  save  for  a  factor  not 
depending  on  #,  y,  to  express  this  polynomial  as  the  product  of  (x—  ^^...(x—  &*) 
by  a  determinant  of  p  rows  and  columns  of  which,  for  r  >  1,  the  rth  row  is 
formed  with  the  elements 


A-l 

r  yr          yr 


wherein    $(x)   denotes  (x  —  b^  .  .  .  (x  —  bk),  the  first  row  being  of  the  same 
form  with  the  omission  of  the  suffixes. 

Therefore,  noticing  that  F  is  symmetrical  in  the  places  asl}  ...,  a;p,  we 
infer,  denoting  the  product  of  the  differences  of  ar1}  ...,  xp  by  A(#i,  ...,  xp), 
that 

lavy,      £jfr  Vr        M     M-I        J 

*-1>  ""'' 


where  (7  is  an  absolute  constant,  and  the  numerator  denotes  a  determinant 
in  which  the  first,  second,  ...  rows  contain,  respectively,  xlt  x2>  ...;  and  here 

when  &  is  even,  \  =  ^k  —  1,      p=p  —  1  —  1& 

and  when  k  is  odd,  X  =  ^(&  —  3),  /*  =  jj  —  ^  (k  +  1). 


210.  By  means  of  the  algebraic  expression  which  we  have  already 
obtained  for  the  quotients  ^  (u  ub<  a)/^  (u),  we  are  now  able  to  deduce  an 
algebraic  expression  for  the  quotients 


(u)  ; 

since  it  has  already  been  shewn  that  by  taking  k  in  turn  equal  to  1,  2,  ...,p, 
and  taking  all  possible  sets  b1}  ...,  bk  corresponding  to  any  value  of  k,  the 
half-  periods  represented  by  ubi>a+  ......  -\-ub*>a  consist  of  all  possible  half- 

periods  except  that  one  which   is  identically  zero,  it  follows   that,  in   the 


210]  CONNECTING   THE   THETA   FUNCTIONS.  313 

hyperelliptic  case,  if  u  denote  ux><a>  +  ......  +  uxi»a»,  and  q  denote  in  turn  all 

possible  half-integer  characteristics  except  the  identically  zero  characteristic, 
all  the  2^-1  ratios  ^  (u  ;  q)^  (u)  can  be  expressed  algebraically  in  terms  of 
xl}  ...,  xp,  by  the  formulae  which  have  been  given. 

The  simplest  case  is  when  k  =  2  ;  then  we  have  A,  =  0,  //,  =  p  -  2,  and 


_ 

:  : 


_ 

-  bj  (xr  -  6,)  jRT^)  ' 
where   ^  (a?)  =  (x  -  x^  (x  -  #2)  .  .  .  (x  -  xp},   and    C  is   an   absolute   constant. 
Denoting  the  quotient  ^  (u  ub»a  +  ifr,  •)$  (u)  by  qbii  &2,  we  have 


=i 


-—   - 

-  &i)  (a?r  -  62)  .R'  («r) 


where    ^Ilj2    is    an    absolute    constant;    and    there    are    p(2p  +  l)    such 
functions. 

When  k  =  3,  we  have  X  =  0,  n  =p  -  2,  and,  if  qbl>bl>bt  denote  the  quotient 
£  (u\ub»a  +  ifa  a  +  ub»  a)/^  (u),  we  obtain 

^>  v  1 

=  —       —  --- 


where  BJt  2i  3  is  an  absolute  constant.     It  is  however  clear  that 

<?&! ,  62  <?&i,&3        _  /;  7    x        g&,  ,62,63 

so  that  the  functions  with  three  suffixes  are  immediately  expressible  by  those 
with  one  and  those  with  two  suffixes. 


More  generally,  the  2*  -  1  quotients  %(u;  q)/$  (u),  depending  only  on 
the  p  places  xlt  ...,xp,  must  be  connected  by  22P-p-l  algebraical  rela 
tions;    and  since  (Chap.  IX.)  any  argument  can  be  expressed  in  the  form 
was"°'  +  ......  +M*P.«P,  it  follows  that   these    may  be   regarded  as   relations 

connecting  Riemann  theta  functions  of  arbitrary  argument.     This  statement 
is  true  whether  the  surface  be  hyperelliptic  or  not. 

Of  such  relations  one  simple  and  obvious  one  for  the  hyperelliptic  case  under  con 
sideration  may  be  mentioned  at  once.     We  clearly  have 


and  therefore 

^^5M3  (u)  3bl  (w)  +  ^-l^3&1  (u)  \(u)  +  b-^*  3blbtW3bt(u),=  0. 

It  is  proved  below  (§  213)  that  A'^  :  A\  :  A'\2  =  (b.,~b3)  :  (b3~bj  :  (b^bj. 

Other  relations  will  be  given  for  the  casesjo  =  2,  p  =  3.  A  set  of  relations  connecting 
the  y's  of  single  and  double  suffixes,  for  any  value  of  p,  is  given  by  Weierstrass  (Crelle  LII 
Werke  I.  p.  336). 


314  CASE   WHEN   THE   ARGUMENT   IS  [211 

211.    Ex.  i.     Prove  that  the  rational  function  having  the  places  xlt  ...,  xp,  a,  as  poles, 
and  the  branch  place  b  as  one  zero,  is  given  by 


where  R  (£)  =  (£  —  x}  ({-  —  x^ (^-^p)>  and,  in  the  summation,  x0,  y0  are  to  be  replaced 

by  x,  y. 

Prove  that  if  u  denote  the  argument 

then 

52  (M  u<>- «)  Z2 

— ^.>  /  v —  —  A 


(b~x)(b-x1)  ......  (b-xvy 

where  A  is  an  absolute  constant. 

Prove  for  example,  in  the  elliptic  case,  with  Weierstrass's  notation,  that 


Ex.  ii.     If  Zr  denote  the  function  Z  when  the  branch  place  br  is  put  in  place  of  6,  and 
R  (br)  denote  (br  —  x)  (br-  Xj)  ......  (br  —  xp\  and  we  put 


= 
prove  that 


-r  A  (A',   ^j,    ...,  ^p), 

where  B  is  an  absolute  constant,  A  (A;  xlt  ...,  xp)  denotes  the  product  of  all  the  differences 
of  the  (p  +  l)  quantities  x,  x^  ...,  xp,  <j)  (xr)  =  (xr  —  b^)  ......  (xr—bk),  and  the  determinant  is 

one  of  p  +  l  rows  and  columns  in  which,  in  the  first  row,  x0,  y0  are  to  be  replaced  by  x,  y. 

Prove  that,  when  k  is  even,  X  =  J(£-2).  /*=  P~\k,  and,  when  k  is  odd,  X  =  |(£  —  1), 


Ex.   iii.     Hence    prove   that  the   function 
multiple  of 


A(.r,  j?ls  ...,  J7P) 
This  formula  is  true  when  k  =  \. 

Ex.  iv.     A  particular  case  is  when  £  =  2.     Then  the  function  5  (M  ubl>a  +  ub2'  a)/3(u)  is 
a  constant  multiple  of 


wherein  /2  ( 

Ex.  v.  Verify  that  the  formula  of  Ex.  iii.  includes  the  formulae  of  the  text  (§  210)  ; 
shew  that  when  x  is  put  at  infinity  the  values  of  X,  /x  in  the  determinant  of  §  209  are 
properly  obtained. 


211]  A   SUM   OF  p  +  l    INTEGRALS.  315 

Ex.  vi.     Verify  that  the  expression  ^(x^b;  a,x1,  ...,  xp)  of  §  130,  Chap.  VII.,  takes 
the  form  given  for  the  function  Z  of  Ex.  i.  when  a  is  the  place  infinity. 

Ex.  vii.     If  f(x~)  denote  the  polynomial 


prove  that  any  rational   integral  polynomial,  F(x,  z),  which  is  symmetric   in   the  two 
variables  x,  z  and  of  order  p  +  l  in  each  of  them,  and  satisfies  the  conditions 


is  of  the  form 

F(x,z)=f(x,z)  +  (x-z)*+(x,z), 

where  (cf.  p.  195),  with  A0  =  A,  A2,)  +  3  =  0, 

P+I 
f  (x,  z)=-S  x^zi  (2A2i  +  X2i  +  1  (x+z)}, 

t=0 

and  ^  (x,  z)  is  an  integral  polynomial,  symmetric  in  x,  z,  of  order/)-  1  in  each*. 

In   case  jo  =  2,  and  f(x)  =  (x-a1)  (x  —  a^)(x  —  c)  (x-c1)(x  —  c2),  prove  that  a  form  of 
F(x,  z)  is  given  by 

F  (x,  z)  =  (x-  ctj)  (x  -  02)  (z  -c)(z-  Cj)  (z  -  c2)  +  (z  -  at)  (z  -  «2)  (x  -  c)  (x  -c^(x-  c2). 
Ex.  viii.     If  for  purposes  of  operation  we  introduce  homogeneous  variables  and  write 


prove  that  a  form  of  F(x,  z)  is  given  by 


\P     /      3 

A* 


where,  after  differentiation,  jclt  x2,  zlt  z2  are  to  be  replaced  by  x,  1,  z,  1  respectively. 

This  is  the  same  as  that  which  in  the  ordinary  symbolical  notation  for  binary  forms  is 

J  1     J    1-        J/  \         n    P+1    P+l      j-/     \    1       •  2^+2 

denoted  by/  (x,  z)  =  2ax    az     ,  f(x)  being  ax     . 

Ex.  ix.     Using  the  form  of  Ex.  viii.  for  F(x,  z),  prove  that  if  elt  e2,  x,  xly  ...,  xp 
be  any  values  of  x,  we  have 

s     f^     i  ^s     f(x"  x*>  /(ei)  /C^)  7(gi>  %) 

r=0  [0'  S3F"1"  ™  G"  (o?r)  6r"  (j?.)     [(?'  (6l)]2  T  [>"  (e2)]2  *  »'  (6l)  G'  (ej  ' 


where  G'(^)  =  (^-e1)  (£  -  e.2)  (g  -  x)  (i-  —  xj  ......  (^  —  xp),and  the  double  summation  on  the 

left  refers  to  every  one  of  the  \p  (p  +  l)  pairs  of  quantities  chosen  from  x,  xlt  ...,  xp. 


Ex.  x.     Hence  it  follows!,  when  yz=f(x\  yr2=/(-*V)>  etc.,  and  R(£)  =  (£-$)  (^-^1)... 
(I  -  XP\  that 

R(^Rif^*-       Jfe_      -  T  -  / 

W       ^  ^  L  0  («i  -  '^r)  (*2  -  «r)  ^  (ir)  J         '(«!  -  e 

is  equal  to 


*  It  follows  that  the  hyperelliptic  canonical  integral  of  the  third  kind  obtained  on  page  195 
can  be  changed  into  the  most  general  canonical  integral,  -R*1  a  (p.  194),  in  which  the  matrix  a 

has  any  value,  by  taking,  instead  of/(x,  z),  a  suitable  polynomial  F(x,  z)  satisfying  the  conditions 
of  Ex.  vii. 

t  The  result  of  this  Example  is  given  by  Bolza,  Gotting.  Nachrichten,  1894,  p.  268. 


316  A   SOLUTION    OF   THE   INVERSION    PROBLEM  [211 

where  the  summation  refers  to  every  pair  from  the  p  +  l  quantities  x,  x±,  ...,  zp,  and 
/(#,  2)  denotes  the  special  value  of  F(x,  2)  obtained  in  Ex.  viii. 

Ex.  xi.     It  follows  therefore  by  Ex.  iv.  that  when  bt  ,  b.2  are  any  branch  places  of  the 
surface  associated  with  the  equation  y*-f(%)  =  0,  there  exists  an  equation  of  the  form 

V  (u\ub»a  +  ub»a)_  2yryg-f(xr,xg)     f  (blt  b,} 

&W~  (l)  '    G'(xr}G'(xg}    ~(V-~^?' 

where   C  is   an    absolute   constant,    (*(£)  =  (£  —  bj  (£  -  b2)  (g  —  a;)  (g  -  x^)  ......  (%-Xp),    and 

u  =  ux>  a  +  uXl'cll  +  ......  +UXP'  aP.     The  importance  of  this  result  will  appear  below. 

212.     The  formulae  of  §§  208,  210  furnish  a  solution  of  the  inversion 
problem  expressed  by  the  p  equations 

*!,<*!  Xp,dp  /  *  -I         C»  \ 

Ui      +  ......  +Ui       =ut;  (»—  1,  2,  ...,  j>> 

For  instance  the  solution  is  given  by  the  2p  +  1  equations 


from  any  p  of  these  equations  xl}  ...,xp  can  be  expressed  as  single  valued 
functions  of  the  arbitrary  arguments  ult  ...,  up. 

And  it  is  easy  to  determine  the  value  of  A2.  For  let  blt  ...,  bp,  6/,  ...,  bp' 
denote  the  finite  branch  places  other  than  6.  As  already  remarked  (§  201) 
we  have 

\c,  GI,  .  .  .  ,  Cp)  =  (ft,  a/1,  .  .  .  ,  Up) 
and  therefore 

(b,  b1}  ...,bp)  =  (ft,  bi,  ...,  bp'). 

Now  we  easily  find  by  the  formulae  of  §  190,  Chap.  X.  that  if  P  be  a  set 
of  2p  integers,  Plt  ...,  Pp,  P/,  ...,  P/, 


^(u) 


n.pp, 


hence,  if  ub'  a  =  %  ^  v  ,  and  u0  =  w6'  -  a  +  ......  +  ubp<  a,  we  have,  by  the  formula 

under  consideration,  writing  b1}  ...,  bp  in  place  of  xl}  ...,  xp,  the  equation 


and,  writing  &/,  ...,  bp  in  place  of  xlt  ...,  xp,  we  have 

^•2  /,/     i    n.b,  a  »,b,  a\ 

r*    \uo  ^  It  '     \lt  '    )  .    n         ,   ,.  n 

^(^  +  ^'g)  /i(6"6l)-'(6 

thus,  by  multiplication 

e-«pi>  =  A*  (&  _  &i)  .  .  .  (6._  bp)  (b  _  6;)  .. 


213]  IN   THE   HYPERELLIPTIC   CASE.  317 

and  hence 

W(u\ub>  a)         (b-xl)(b-x^...(b-xp) 


where/(#)  denotes  (x  —  a^)  ...  (x  —  ap)  (x  —  c}(x  —  cl}...(x  —  cp),  and  eirit>p  =  ±  1 
according  as  ub>a  is  an  odd  or  even  half-period. 

The  reader  should  deduce  this  result  from  the  equation  (§  171,  Chap.  IX.) 

U  •  t     •*,  \  V(TT  TT  •  £     -.,  \  —  ^  ~~^(xi)}  ......  (^  ~^(xv)} 

....  UP,  &,yi)  ......  r(»V-i  V*  **>y*>- 


by  taking  Z  to  be  the  rational  function  of  the  second  order,  x. 

'a>  +  ......  +  uxv>  aP,  we  deduce  (see  Ex.  i.  §  211) 

yr         1 


If  in  particular  we  put  b  in  turn  at  the  places  a1}  ...,  ap,  write 
P  (x)  =  (x-al)  ...  (x  -  ap)  and  Q  (x}  =  (x  -  c)  (x  -  cx)  .  .  .  (x  -  cp),  and  use  the 
equation 

(x  -  a?x)  .  .  .  (x  -  xp}  __         |  (at  -  x^  .  .  .  (af  -  Xp) 
~P(x)  hf~  (a>-di)P(at) 

we  can  infer  that  oc1}  ...,  xp  are  the  roots  of  the  equation* 


t=i 
where  e^  is  +  1  and  is  such  that  we  have 


<&_(U  tt«.  a)  (at  -  Xj  _  (dj  -  Xp} 


Another  form  of  this  equation  for  xlt  ...,  xp  is  given  below  (§  216),  where 
the  equation  determining  yt  from  x±  is  also  given. 

213.     We   can  also  obtain   the   constant  factor  in   the   algebraic   expression   of  the 

(u\ubl'a+ub*'a)3(u)  +  3  (u  ?«6"a)  3  (u\u^'  a}. 


Let  />j  ,  b.i  denote  any  branch  places,  and  choose  zlt  ...,  zp  so  that 


then  zlt  ...,  zpta  are  the  zeros  of  a  rational  function  which  vanishes  in  ^,  ...,  .rp,  6,. 
Such  a  function  can  be  expressed  in  the  form 


*  Cf.  Weierstrass,  Math.  Werke  (Berlin,  1894),  vol.  i.  p.  328, 


318  DETERMINATION   OF   A   CONSTANT   FACTOR.  [213 

where  (x,  l^7"1  is  an  integral  polynomial  in  x  whose  coefficients  are  to  be  chosen  to  satisfy 
the  p  equations 

-yi  +  (#i-6i)fo,  IX'-^O,  (i  =  l,  2,  ...,p)  ; 

thus  the  function  is 


where  F(.r)  =  (x  —  x1)  ...  (x-x^)  ;  and,  if  the  coefficient  of  x2P  +  1  in  the  equation  associated 
with  the  Riemann  surface  be  taken  to  be  4,  we  have 

^-<*-^t*(4p[£^ 

and  therefore,  putting  bt  for  x, 

y*-         i  T 

'        ' 


Now  we  have  found,  denoting  ux>!  a>  +  ......  +  u***  '  °P  by  u,  and  uZl>  a'  +  ......  +  w2"  '  a"  by  v, 

the  results 


where  w^2'  a  =  ^Qp  p-;  hence  we  have 

1*         y*          JLT 


which,  by  the  formulae  of  §  190,  is  the  same  as 

*»  -  y< 


_ 

5  (u\ub><  a)  5  (M|M6«-  a) 

where  e  is  a  certain  fourth  root  of  unity. 

Thus  the  method  of  this  §  not  only  reproduces  the  result  of  §  210,  but  determines  the 
constant  factor. 

Ex.     Determine  the  constant  factors  in  the  formulae  of  §§  208,  210,  211. 

214.  Beside  such  formulae  as  those  so  far  developed,  which  express 
products  of  theta  functions  algebraically,  there  are  formulae  which  express 
differential  coefficients  of  theta  functions  algebraically;  as  the  second 
differential  coefficients  of  ^(w)  in  regard  to  the  arguments  u^,  ...,  up  are 
periodic  functions  of  these  arguments,  this  was  to  be  expected. 

We  have  (§  193,  Chap.  X.)  obtained*  the  formula 


-«,  I 


=  T  . 

J-*i         i    — .   ~K  »  i_\~K9  "v        \™K>  A~/J     J^ 

*=i  at 


Cf,  also  Thomae,  Crelle,  LXXI.,  xciv. 


214]  EXPRESSION   OF  THE   £  FUNCTION.  319 

we  denote  by  hr  the  sum  of  the  homogeneous  products  of  xl  ,  ...,  xp,  r  together, 
without  repetitions,  and  use  the  abbreviation 


further,  for  the  p  fundamental  integrals  MX  '  M,  .  .  .  ,  up'  M,  we  take  the  integrals 
f  *  dx      xx  dx  x  xP'1  dx 


dx    fxx  dx          fx  xP'1  dx 
y  '  Jp    y   '  '  *'/p      y 

then  it  is  immediately  verified  that 


i&k',  xl}  ...,Xp)/dxk 

~  '"* 


where  jP  (a;)  denotes  (#  —  a,-,)  ...  (x  —  xp). 

Thus,  if  p,  v  denote  the  values  of  x  and  y  at  the  place  /z,  we  have,  writing 
a,  Oj,  ...,  03,  for  w,  Wj,  ...,  w^  (§  200), 

-  &  (M*.  °  -  ux><  a'  -  ......  -  W*P.  a^)  +  §;-(t^.  «  -  «*..«.  -  ......  -UXP<  ap} 

T*>»  ,  i  gxp-'-fo*;  ^i*  •••>ay)  fy  +  y*    y*  +  H  . 
*•% 

therefore,  also,  the  function 


is  equal  to 


..    ..  _ 

t=i  JT  0*)  p,  -  xk 

which  is  independent  of  the  place  x. 

Now  let  R  (t)  denote  (t  —  x)(t—x1)  ...  (t—xp),  and  use  the  abbreviation 
given  by  the  equation 


,       -  ,  ..., 

' 


then  also 


,          ,        --          ,    .-  _  ,       , 

1^  (xp)  Jp-{~1  ^  l  '  •  •  •  ' 


Now 
is  equal  to 


(«,  A-'i  4-  A-2)  - 


320  EXPRESSION   OF   THE    f  FUNCTION.  [214 

wherein   kr  denotes  the  sum   of  the  homogeneous  products  of  x2,  ...,  xp, 
without  repetitions,  r  together,  and  is  therefore  equal  to 


or  to 

(Xi        X)  J£p_i_i  {Xi  ',    X2>  '••  >  xy>}' 

Hence 


(x,  -  x)  Ff  (x,) 


_ 

F'(x,)  x-Xi  F'  '(a?,) 

While,  also, 


Thus 


^_t      ,     !,...,    y   -        -  „,  ,     . 

k=l  *      \-'k/ 

Therefore  the  expression 


is  equal  to 


In  this  equation  the  left-hand  side  is  symmetrical  in  x,  x1}  ...,  xp,  and  the 
right-hand  side  does  not  contain  x.  Hence  the  left-hand  side  is  a  constant 
in  regard  to  x,  and,  therefore,  also  in  regard  to  x1}  ...,  xp.  That  is,  the  left- 
hand  side  is  an  absolute  constant,  depending  on  the  place  /*.  Denoting  this 
constant  by  —  C  we  have 


'  a 


i,-->  Xp-l     ,    „ 


_  _  _ 

2R'  (x)  2R'  (xp) 

215.     From  this  equation  another  important  result  can  be  deduced.     It 
is  clear  that  the  function 


does  not  become  infinite  when  x  approaches  the  place  a,  that  is,  the  place 
infinity.  If  we  express  the  value  of  this  function  by  the  equation  just 
obtained,  it  is  immediately  seen  that  the  limit  of 


215]  BY   ALGEBRAICAL   INTEGRALS   AND   RATIONAL   FUNCTIONS.  321 

and  that  the  expression 


when  expanded  in  powers  oft  by  the  substitutions  ac  =  -,y  =  —^  (1  +  At2  +  ...), 

" 


t 

where  A  is  a  certain  constant,  contains  only  odd  powers  of  t.  Hence  the 
limit  when  t  is  zero  of  the  terms  of  the  expansion  of  this  expression  other 
than  those  containing  negative  powers  of  t,  is  absolute  zero,  and  therefore, 
does  not  depend  on  the  places  xl}  ...,xp.  The  terms  of  the  expansion  which 
contain  negative  powers  of  t  are  cancelled  by  terms  arising  from  the  integral 

L^  .  Since  this  integral  does  not  contain  xl}  ...,  xp  we  infer  that  the 
difference 

rx  *  _  yxp-j(®',  BI,  --,  a?) 

2R'  (x) 
has  a  limit  independent  of  xl}  ...,  xp,  and,  therefore,  that 


no  additive  constant  being  necessary  because,  as  &  (u)  is  an  odd  function, 
both  sides  of  the  equation  vanish  when  xlt  ...,  xp  are  respectively  at  the 
places  Oj,  ...,ap.  As  any  argument  can  be  written,  save  for  periods,  in  the 
form  ux»  a>  +  .  .  .  +UXP>  av,  this  equation  is  theoretically  sufficient  to  enable  us  to 
express  £  (w)  for  any  value  of  u. 

Ex.  i.     It  can  easily  be  shewn  (§  200)  that 

uc'a  +  uc>'a<  +  ......  -\-uc*»aP  =  Q. 

Thus  the  final-  formula  of  §  214  immediately  gives 


......  ...... 

fc=i          2  (xjc-  c)  F'  (xk) 

Ex.  ii.     In  case  p  =  \  we  infer  from  the  formula  just  obtained,  and  from  the  final 
formula  of  §  214,  respectively,  the  results 


where  D  is  an  absolute  constant.     Thus 


X      96  1 

This  is  practically  equivalent  with  the  well-known  formula 


The  identification  can  be  made  complete  by  means  of  the  facts  (i)  The  Weierstrass 
argument  u  is  equal  to  ua>  x,  in  our  notation,  so  that  y=-$>'  (u),  (ii)  ux<  a'  =  (a  +  o>'-u,  so 

that    ^(ux-  "0  =  ^  («  +  «'-«)=  -4'"'=-  r*£^?  ,   as  we   easily  find   when   Z*'M  is 

7  rti    y 
B.  21 


322  EXAMPLES.  [215 

chosen  as  in  §  138,  Ex.  i.,  (iii)  d£u  =  ——  ,  (iv)  therefore  fx  (ux'  a>)  =  -  £u,  (v)  the  branch 

i7 

places  clt  alt  c  are  chosen  by  Weierstrass  (in  accordance  with  the  formula  ^+62  +  63=0) 
so  that  the  limit  of  $>u  —  ^,  when  u  =  0,  is  0.  The  effect  of  this  is  that  the  constant 
D  is  zero. 

Ex.  iii.     For  p  =  2  we  have 

-  f,  (ux>  a+uXl'  ai  +  ux*>  a*)  =  Lx'  »  +  L*»  ^+Z*"  * 


-2  i--g  *t--i        c 

A-  -  #2)      2  (#!  —  x}  fa  —  #2)      2  (#2  -  x)  (xz  -  x^)       l 


and 


-t  *~  *     o  *  « 

where  with  a  suitable  determination  of  the  matrix  a  which  occurs  in  the  definition  of  the 
integrals  Lx'  M  and  in  the  function  3  (u),  we  may  take  (§  138,  Ex.  i.  Chap.  VII.) 


For  any  values  of  p  we  obtain 

-fP0«*i>0l  +  ......  +  uxP<ai>)=Lx»a>  +  ......  +  Za!P>aP=-^±1I    fx 

4    *=ijak    y 

Ex.  iv.     We  have  (§  210)  obtained  22"  -  1  formulae  of  the  form 
$(u\ub"a  +  ......  +ubk>a) 

~~ 


where  Z  is  an  algebraical  function,  and  the  arguments  ult  ...,  ut)  are  given  by 


the  integrals  being  taken  as  in  §  214,  these  equations  lead  to 


Hence  we  have 


For  instance,  when  £  =  1,  and  Z  is  a  constant  multiple  of  ^(b^—x-^  ......  (bl  —  xp\  we 

obtain 


so  that 


a\_/*i,  «i  i  -L/^I^P-V         &r  (r  •   r  r} 

/"•*'|       +  ......  +    ,-  *  aJp/vT   Jfi»-*-iw«  *i'  '"»*i»^ 

,.=1^^   ^r;  [_ 


xr-b 

_TXl,al   ,  .TXp.Op         |          ^  Xp-i^r?    ^,  #1,   ...,^p) 

~  +  ......  +  ---  " 


216]  ANOTHER  SOLUTION   OF  THE   INVERSION   PROBLEM.  323 

By  means  of  the  formula 


which  is  easily  obtained  from  the  formulae  of  §  190,  we  can  infer  that  the  formula  just 
obtained  is  in  accordance  with  the  final  formula  of  §  214. 

(2»-f-l\ 
/ 

even  theta  functions  which  do  not  vanish  ;  and  the  corresponding  half-periods  are  con 
gruent  to  expressions  of  the  form 


It  may  be  shewn  in  fact  that  these  half-periods  are  obtained  by  taking  for  xv  ,  .  .  .  ,  xv  the 

(  P       ]  possible  sets  of  p  branch  places  that  can  be  chosen  from  o15  ...,  ap,  c,  c1?  ...,  cp. 

V    P    ) 

Hence  it  follows  from  the  formula  of  the  text  (p.  321)  that  if  $Qk  be  any  even  half-period 

corresponding  to  a  non-  vanishing  theta  function,  we  have 


This  formula  generalises  the  well-known  elliptic  function  formula  expressed  by  fw  =  ^. 
To  explain  the  notation  a  particular  case  may  be  given  ;  we  have 

£,(«,,,.,    <*2,r,    ..-,    *P,r)=r,i,r,   ™  &<1*t*f)=  -Z****' 

and 

fi(»',,r,«'2,r,  ».,  »'ftr)=«?'<,r,or   W*  "*)      =  -  L*'  «*. 

Thus  each  of  the  2p2  quantities  ^  ,.,  7?'f,  r  can  be  expressed  as   ^-functions  of  half- 
periods. 

Ex.  vi.     The  formula  of  the  text  (p.  321)  is  equivalent  to 


where 

For  example  when  p  = 


216.     It  is  easy  to  prove,  as  remarked  in  Ex.  iii.  §  215,  that  if 


and  the  matrix  a  (§  138,  Chap.  VII.)  be  determined  so  that  the  integrals 
L*'*  have  the  value  found  in  §  138,  Ex.  i.,  then 


|  [*ta?dx 

i        —  -    . 

=lJ  a        y 


a 

Therefore,  if  -  —  %r  (u)  be  denoted  by  $>r,  i  (u),  we  have 


21—2 


324  SOLUTION   OF   THE   INVERSION   PROBLEM  [216 

and  thus,  as  follows  from  the  definition  of  the  arguments  u, 


where  F  (x)  denotes  (x  —  x^)  ...  (x  —  xp). 

Whence,  if  a;  be  any  argument  whatever, 

XP  |  xi_, 

T?      j i  /     \    i-x  <c  t  =  l 

^         y  Pi  i  \^)>  —  4  ^2p+l    —    ~ 
i=l  k=l 


but  we  have 

P  p     ._. 

" 


Thus 

p    2  i-l      ,  . 

V/c  =  Z  Xk      K>PI  i  (u). 


Thus,  if  we  suppose  Xap+i  =  4,  the   values  of  a?1}  ...,  a?p  satisfying  the 
inversion  problem  expressed  by  the  equations 

M  =  w*"  a'  -f  ......  +  w^'  °v 

are  the  roots  of  the  equation 

F  (x)  =  XP-  XV-*  ppf  p  (M)  -  a^9fi  ^(u)-  ......  -p^  (u)  =  0. 

In  other  words,  if  the  sum  of  the  homogeneous  products  of  r  dimensions, 
without  repetitions,  of  the  quantities  xl}  ...,xp  be  denoted  by  hr,  we  have 

hr  =  (-y-1$>p>p-r+i(u). 

Further,  from  the  equation 

-i  fa',  ^i  .....  XP) 


fat  F'(xk) 

putting  p  for  i,  we  infer  that 


,    -     . 

dup  \_   ditp  }x=Xk 

because  F(xk}  =  0.     Thus,  if  we  use  the  abbreviation 


we  obtain 


216]  BY   THE   ip-  FUNCTIONS.  325 

These  equations  constitute  a  complete  solution  of  the  inversion  problem. 
In  the  ^-functions  the  matrix  a  is  as  in  §  138,  Ex.  i.,  and  the  integrals  of  the 
first  kind  are  as  in  §  214. 

We  have  previously  (§  212)  shewn  that  xl}  ...,  xp  are  determinable  from 
p  such  equations  as 

^  (u  |  M«<  >a)=v  (at  -  ap  .  .  .  (en-  xp)    _(ai-xl)...(ai-xp) 
V(u)  ^-p'-^Qla,)  K  Say" 

Thus  we  have  p  equations  of  the  form 


Ex.  i.     For  p  =  1  we  have 


This  is  equivalent  to  the  equation  which  is  commonly  written  in  the  form 


•  3  9  /  / \  * 

sn2  (u  v  e1  —  es) 
v.  ii.     For  p  =  2  we  have 


We  may  denote  the  left-hand  sides  of  these  equations  respectively  by  /i^2,  Mq£. 

Ex.  iii.    Prove  that,  with  AflS^~<%IV»i(«)-ft.'t<4«ll^  MI=  ±  V^/K),  we  have 


]  +  «1«2  [^22  («)  ~  ^22  00]- 

-.  iv.     Prove  that 


^.  v.     If,  with  P  (^)  to  denote  (x-a^  ......  (x  -  «p),  we  put 

F  =  /"*•  P(a?)  0^'  r«p  P  (a:)  d 

Jaix-ar2y  ]at>x-ar2 

prove  that 

3  a  _0  3 

o'y/  T  ......  ~r  oT?"  —  *  5  —  • 

o  ^  i  9  Vp       dup 

Ex.  vi.     With  the  same  notation,  shew  that  if 


then 


326  EXAMPLES.  [216 

The  arguments  Vl,  ...,  Vp  are  those  used  by  Weierstrass  (Math.  Werke,  Bd.  i.  Berlin, 
1894,  p.  297).  The  result  of  Ex.  iv.  is  necessary  to  compare  his  results  with  those  here 
obtained.  The  equation  yr  =  \js(xr)  is  given  by  Weierstrass.  The  relation  of  Ex.  vi. 
is  given  by  Hancock  (Eine  Form  des  Additionstheorem  u.  s.  w.  Diss.  Berlin,  1894, 
Bernstein). 

With  these  arguments  we  have 


Ex.  vii.     Prove  from  the  formula 

-(i(ux 
where 

that  the  function 


F(x) 
is  independent  of  the  place  x.     Here  c  is  an  arbitrary  place  and  F  (x)  =  (x  -  x-^)  ......  (x  -  x^). 

Ex.  viii.  If  ^ac  denote  the  integral  if  '  *  -  222^,  ,•  uz:  c  uf  a,  obtained  in  §  138,  and 
F^  a  denote  -D^'  ",  prove  that  in  the  hyperelliptic  case,  with  the  matrix  a  determined  as 
in  Ex.  i.  §  138,  when  the  place  a  is  at  infinity, 


2      ;/*    y 

Hence,  when  A2P+1  =  4,  shew  that  the  equation  obtained  in  §  215  (p.  321)  is  deducible 
from  the  equation  (Chap.  X.  §  196) 


Ex.  ix.  We  can  also  express  the  function  £p(u+v)-  £,,(11)  -  £p(v),  which  is  clearly  a 
periodic  function  of  the  arguments  u,  v,  in  an  algebraical  form,  and  in  a  way  which 
generalizes  the  formula  of  Jacobi's  elliptic  functions  given  by 


)  =  k*  sn  wsn  vsn  (u  +  v). 
For  if  we  take  places  xlt  ...,  £,„  such  that 


these  3p  places  will  be  the  zeros  of  a  rational  function  which  has  alt  ...,  at,  as  poles,  each 
to  the  third   order.     This  function  is  expressible  in  the  form  (My  +  NP)/P2,  where  P 
denotes  (x  —  ax)  ......  (x  —  ap\  Mis  an  integral  polynomial  in  x  of  order  p  —  l,  and  A7  is  an 

integral  polynomial  in  x  of  order  p.     Denoting  this  function  by  Zt  we  have 


dl     1 

=  ay> 


217]  EXAMPLES.  327 

[X  T^f/T 

by  §  154,  Chap.  VIII.,  where  1=1%  '*  =  iXa>  +  ,  I         -  .     Writing  Z  in  the  form 

.'  M   y 


and  taking  X2p  +  1  =  4,  we  find  the  value  of  the  integral  K  to  be  -  2A. 
But  from  the  equation 

N*P-4JPQ  =  (x-xJ  ......  (x-xp)(x-zl}  ......  (#-*p)(A'-fi)  ......  (*-W, 

where  Q  =  (x  —  c)  (x  —  q)  ......  (#  -  cp),  we  have,  putting  «;  for  x, 

=  2  V  -  Q  (<j  (Aa*-1  +  ...),  (i  =  l,  2,  ..., 


where  pi=\/(ai-xl)  ......  («»-#,,),   ft—^(«r-*i)  ......  K-^),  ^i  =  V(a»-fi)  ......  («»-&>); 

solving  these  equations  for  A  we  eventually  have* 


=  5 


Ex.  x.     Obtain,  for  jo  =  2,  the  corresponding  expression  for  ^  (u~)  +  f  j  (v)  - 

Ex.  xi.     Denoting  -  7-=  —  =.  by  (7v,  the  equation 

' 


=  2 


gives 

W=  2  <7i[pSr)fc-.Ptfir)]  OT»  (r=l,  2,  ...,  p), 


where  p/  denotes  x—  V(«i  —  *'i)  ......  («i  -  ^P)-     It  has  been  shewn  that  pt  is  a  single  valued 

function  of  u  and  it  may  be  denoted  by  pi  (u).  Similarly  Wi  is  a  single  valued  function 
of  u  +  v,  being  equal  to  Pi(  —  u  —  v).  The  equation  here  obtained  enables  us  therefore  to 
express  pi(u+v]  in  terms  of  Pi(u],  Pi(v),  and  the  diflferential  coefficients  of  these;  for 
we  have  obtained  sufficient  equations  to  express  |ppi  ,.  (u\  ^>;)>  r  (v)  in  terms  of  the  functions 
Pi  (u\  pi  (v).  A  developed  result  is  obtained  below  in  the  case  p  =  2,  in  a  more  elementary 
way. 

217.     We  have  obtained  in  the  last  chapter  (§  197)  the  equation 
S%  j  (ux'  m  -  u*»  ">  -  ......  -  U*P>  «P)  in  (x)  &  (xp)  =  DxDXpRxx'p°c. 

i  j 

Hence,  adopting  that  determination  of  the  matrix  a,  occurring  in  the 
integrals  L*'  *,  and  the  function  S-  (u)  (§  192,   Chap.  X.),  which  gives  the 

particular  forms  for  L*'  *  obtained  in  §  138,  Ex.  i.,  we  have  in  the  hyperellip- 
tic  case 

(M*.  «  +  w*.«  •»  +  ..    ..+U*P>  tyaf-W-1 


4  (a?  -  serf 

P+I 
where  f(x,  z)  =  S  xlzl  [2^  +  \^+1  (x  +  z}\     This   equation   is,  however,  in- 

t  =  0 

*  This  equation,  with  the  integrals  Lx<  a  on  the  left-hand  side,  is  given  by  Forsyth,  Phil. 
Trans.  1883,  Part  i. 


328  RATIONAL   EXPRESSION  [217 

dependent  of  the  particular  matrix  a  adopted.     For  suppose,  instead  of  the 
particular  integral 


Tx,n        (xdx^~i 

Li     ,  =      —     2,     Xjfc+i+i  (k+l-i)  &, 

J  H    y       k  =  i 

we  take 

TX>  *       v  n       x>  * 
IH     -  2,  Ci>kuk    , 

k=l 

where  Cijk  =  Ckji;  then  (§  138)  this  is  equivalent  to  replacing  the  particular 
matrix  a  by  a  +  \  C,  where  C  is  an  arbitrary  symmetrical  matrix,  and  we 
have  the  following  resulting  changes  (p.  315) 


R%c  (p.  194)     becomes  changed  to  Rx^  *  -  S2C^  kuf  °%  °,  so  that, 
f(x,  z)  (p.  195)  becomes  changed  to/(#,  z)  -  4  (x  —  z)-  22(7;,  kO?-1?*-1, 
S-(w)  (§  189)      becomes  multiplied  by 


and  thus  ^(u)  is  increased  by  Cit  1itl  +  ......  +  Ciipup,  and  instead  of  $>ij(u) 

we  have  ^  j  (u)  —  Cti  j. 

Since  now  ux>  a  +  ux*>  a«  =  ux»>  a  +  ux>  a«,  we  have  \p  (p  +  1)  equations  of  the 
form 


where   u=  ux>a+  ux"  a>  +  ......  +uxp'ap,  r  =  Q,  I,  ...,  p,   and   6'  =  0,  1,  ...,  p. 

Hence,  if  e1}  e2  denote  any  quantities  we  obtain  by  calculation 


*   - 


here  the  matrix  a  is  arbitrary,  the  polynomial  f(xr,  xs)  being  correspond 
ingly  chosen,  and 


Suppose    now    that   f(x,  z)  =f(x,  z)  +  4  (#  —  ^)2  SS^i,  j«r    ««    ,    where 

i  i 
f(x,  z)  is  the  form  obtained  in  Ex.  viii.  §  211  ;  then  we  obtain 

ss  EM»)  -  A  J  •!-'.*-•  -  ' 

and  by  Ex.  x.  §  211  this  is  equal  to 


_ 

4  (&1  -  e#  R  (« 


4  (6l  -  e2)2  ^  (e2)     4  (e,  - 


217]  OF  THE   FUNCTIONS   |>.  329 

and  therefore 


4  (e,  -  e,J  R  («,)     4  (e,  -  etf  R  (<?2)  **(*-  etf 
This  is  a  very  general  formula*  ;  in  it  the  matrix  a  is  arbitrary. 

It  follows  from  Ex.  xi.  §  211  that  if  blt  b2  be  any  branch  places,  we  have 


where  E  is  a  certain  constant  (cf.  §§  213,  212).     This  equation  is  also  inde 
pendent  of  the  determination  of  the  matrix  a. 


By  solving  %p(p  +  l)  equations  of  this  form,  wherein  61}  62  are  in  turn 
taken  to  be  every  pair  chosen  from  any  p  +  1  branch  places,  we  can  express 
22%>i,j  (w)  e\  eJ2  as  a  linear  function  of  \p  (p  +  1)  squared  theta  quotients, 
el,  e2  being  any  quantities  whatever. 

By  putting  62  at  a,  that  is  at  infinity  (first  dividing  by  6f  ~1),  and  putting 
x  also  at  a,  this  becomes  the  formula  already  obtained  (§  216) 


Ex.  i.     When  jo  =  1,  taking  the  fundamental  equation  to  be 

the  expression  >-**-**-*, 

p+i 
/(o;,4  =2^[2X2i  +  X2i 

and 


Therefore,  by  the  formula  at  the  middle  of  page  328,  taking  the  matrix  a  to  have  the 
particular  determination  of  §  138,  Ex.  i., 


*  \x-xj  ' 
this  is  a  well-known  result. 

Ex.  ii.     When  p  =  2,  we  easily  find 


It  is  given  by  Bolza,  Gottinger  Nachrichten,  1894,  p.  268. 


330  FORMULAE   FOR   THE   FUNCTIONS   |jf>.  [217 

and  thus  the  expression 


i      2     i.  2  i2    s,  2 

is  equal  to 

,  a?g)     (^  -  e^  (^  -  e2) 


4(a?-a?2)2 


_ 
(#2  —  a?)  (a?2  -  a?x)      4  (a:  —  a^)2 

Herein  the  matrix  a  is  perfectly  general.  Adopting  the  particular  determination  of 
§  138,  Ex.  i.,  we  have,  since  the  term  in  f(x,  z)  of  highest  degree  in  x  is  A2p  +  1#p  +  12p,  =4ar3s2, 
say,  by  putting  the  place  x  at  a,  that  is  at  infinity,  the  result 


Pi,  1  («)  +  («1  +  62)  Pi,  2  00  +  *1*2  £>2>  2  («)  = 

,  —   2 
where  u=uXl'  ai  +  ux-'  a2. 

^r.  iii.     Prove,  for  jo  =  2,  when  the  matrix  a  is  as  in  §  138,  Ex.  i.,  that 

).^ 

—  — 


where  e^  e2  are  any  quantities,  u  =  uXl'  ai  +  ux*'  tt2,  and  ^19  /a2  are  as  in  §  216  (cf.  §  213). 
Ex.  iv.     From  the  formula,  for£>  =  2  (§§  217,  216,  213), 


where  a1}  cr2  are  the  branch  places  as  before  denoted,  infer  (§  216,  Ex.  iii.)  that 

Pll  (*0  -  Pll  ('0  +  Pl2  W  P22  («')  -  Pl2  («')  P22  («)  =  ^T  [?122  ~  ?'l22  -  ?!2?2'  2  + 

Ct-j  —  W2 

Prove  also  that,  for  any  value  of  u,  and  any  position  of  x, 

ff>u  (M*.  «  +  u)  -  pu  (w)  +  ^>12  (M*-  «  +  M)  ^>22  (M)  -  g>22  (u*>  « 


.  v.     If  61}  ...,  6P  +  1  be  any  (p  +  1)  branch  places,  and  e1?  e2  any  quantities  whatever, 
=  (#-&i)  ......  (^-&P+i),  J/'(^)  =  (^-e1)(^-e2)(^-61)  ......  (^-&p  +  1),  prove  that 


where  the  matrix  a  has  a  perfectly  general  value,  r,  s  consist  of  every  pair  of  different 
numbers  from  the  numbers  1,  2,  ...,  (p  +  1),  and  Er,  8  are  constants. 

218.  We  conclude  this  chapter  with  some  further  details  in  regard  to 
the  case  p  =  2,  which  will  furnish  a  useful  introduction  to  the  problems  of 
future  chapters  of  the  present  volume.  We  have  in  case  p  =  1  such  a  formula 
as  that  expressed  by  the  equation 

<r(u  +  u')  a-(u  —  u')          .  ,.          ,   . 

.•ooVoo    -tw-tw> 

we  investigate  now,  in  case  p  =  2,  corresponding  formulae  for  the  functions 

-  u') 


218] 


CONSIDERATION    OF   THE   CASE    IN    WHICH  p   IS   TWO. 


331 


by  division  of  the  results  we  obtain  a  formula  expressing  the  theta  quotient 
^(M+W'  ub'a)+^(u+u'}  by  theta  quotients  of  the  arguments  u,  u'  ;  this  formula 
may  be  called  the  addition  equation  for  the  theta  quotient  ^  (u  ub>  °)  -r-  S-  (u). 
Though  we  shall  in  a  future  chapter  obtain  the  result  in  another  way,  it  will 
be  found  that  a  certain  interest  attaches  to  the  mode  of  proof  employed  here. 

Determine  the  places  aclt  xz,  a?/,  xz  so  that 


u  = 


then,  in  order  to  find  where  the  function  <&  (ux"ai  +  ux*>a* 
vanishes,  regarded  as  a  function  of  a^,  we  are  to  put 


i>ai  +  uXi'>a*) 


thus  the  places  z1}  z2  are  positions  of  xl  for  which  the  determinant 
=     ~D ~/ir\ '    ~~D~T^\  t  **it    -'- 


,   x2 ,    1 


wherein  P  (x)  denotes  (x  —  a^)  (x  —  a2),  vanishes.  By  considerations  analogous 
to  those  of  §  209  we  therefore  find,  V  denoting  the  determinant  derived 
from  V  by  changing  the  sign  of  y±,  y2, 

—  ii'\  VVPfr  ^  P(r  \  P(r  '\  P(<r  '\ 

/A  V    V  JL      li//|  /  -L      I  a/2  /  J-      \^1  )  -»-     \*v-2  / 


S-2  (u)  ^2  (u')  "  (a?!  -  x^f  (a?/  -  a;2')2  (x-,  -  a?/)  (^  -  a?/)  (ara  -  a;/)  (a?.,  -  <) ' 

where  -4  is  an  absolute  constant. 

Now,  ifrjl=y1/P  (tfj),  etc.,  we  find  by  expansion  and  multiplication, 
V V  =  (vi»?2 + 'hV)2 (#1  ~ *'i)2 (x  ~ *? ~ 


and,  if  a  =  (x^  -  x^)  (x2'  -  x2),  /3= (x-[  -  x,2)  (x%  -  Xj),  a  -  j3= (x-{  -  x2')  (^\  -  .t'2),  this  leads  to 
but,  putting  y2  =  4P (x)  Q (x),  =<i(x-al)(x- «2)  (x - c)  (x - ct)  (x - c2),  we  have 
16 


332  ADDITION   FORMULA.   OF   THE   ELLIPTIC   CASE  [218 

and  this  expression  is  equal  to 


+  Q*L(a-x)(a-x)(a-x')(a-x')\, 
P'ttj 

as  may  be  proved  in  various  ways  ;  now  we  have  proved  (§§  208,  212,  213)  that 

(«j  -  ^)  («!  —  3?2)  =  +  \/  -  P'  («j)  §  (ttj)  gl2,   (a2— ^j)  («2  -  #2)  =  ±  V  —  P'  i 
and 


where  gl  =  3  (u  \  ua>  '  a)  -r  5  (tt),  y2  =  5  (w  |  Ma2'  a)  -^  5  (M),  ^,  2  =  5  (M  |  wa'  '  a  +  ?ttt2-  °)  -f.  5  (w)  ;  thus 

P(ae^P(s^P(x^f(x^ 

as  qi*q£q,zq«z=      7>  ,,    N  „,    >\4     ^          ,  we  have 

' 

8)  P  fa')  P  (argQ 


. 

2 

where  however  we  have  assumed  that  the  sign  to  be  attached  to  the  quotient 


is  the  same  for  the  places  x^  x2'  as  for  the  places  xlt  x.2.     The  product  V  -  P'  (GJ)  §  (at 
V  -  P'  («i)  §  («!>  is,  of  course,  here  equal  to  -  P'  (o^)  §  (e^).     Now, 

P  '  (ai)  =  (^  _  a2)  =  _  p'  («2)  . 
thus  we  obtain 

^  (M  +  w')  ^  (w  -  ^t/) 

^ 


the  value   of  the  constant  multiplier,  S-2,  =  [S-  (O)]2,  being  determined  by 
putting  u'  =  0,  in  which  case  <?/,  qs'}  q^  2  all  vanish. 


If  in  this  formula  we  write  v  =  u  +  ua"  a  +  ua*'  a  in  place  of  M,  we  obtain,  from  the 
formulae 


which  are  easy  to  verify  from   the  formulae    of  §    190,   Chap.  X.   and   the  table    of 
characteristics  given  in  this  chapter,  that 


= 

^ 


and  therefore 


219]  GENERALISED  TO   THE  CASE   IN   WHICH  p  IS  TWO.  333 

where  3  (u)  denotes  3  (u  \  «0"  a  +  ua*'  a).     But  we  can  use  the  result  of  Ex.  iv.  §  217,  to  give 
the  right-hand  side  a  still  further  form,  namely 


Further  if  u"1'  a  +  ua*'  a=$Qm>  TO,,  where  m,  m'  consist  of  integers  each  either  0  or  1, 
we  find,  by  adding  |iim,  m,  to  u  and  u'  and  utilising  the  fact  (§  190)  that 


\m  (u  +  u')  =  2A  j™  («)  +  2X^TO  (u'\ 
that 


where  v = u  + £  Qm>  m, ,  y'  =  u'  +  %  flm>  m, .     It  should  be  noticed  that 

Pi,  i  (v)  =  ~  g^.Q     log  •?  ('«  ;  i  TO,  |w') ;  hence 

*        j 

this  formula  can  be  expressed  so  as  to  involve  only  a  single  function  in  the 
form 

J2/ijyU.2     ff  (u -\- 1?)  <T  (u,  —  v) 

where    a-  (u)    denotes    ^  (u  ^  (•,•,))•    and    caij(u)=  — W  cr  (u\     In 

V  \J-J- //  •"»•/»'  c)u '  nit  •  * 

i      j 

Weierstrass's  corresponding  formula  for  p  =  l,  the  function  <r(7^)  is  de 
termined  so  that  cr  (u)/u  =  1  when  u  =  0.  To  introduce  the  corresponding 
conditions  here  would  carry  us  further  into  detail.  (See  §§  212,  213.) 

Ex.     Prove  that  if  «3  denote  any  one  of  the  branch  places  c,  c15  c2,  a  =  (o2-«3), 
^  =  («3-a1),  y=(a1-a2),  P1=-(a1-xl)  (a-^-x^  etc.,  Pi'  =  (al-a:l")  (a^-xj),  etc.,  and 


with  similar  notation  for  A',  B',  then  the  determinant  A  can  be  expressed  in  the  form 


where 


-  A' 
In  this  form  A  can  be  immediately  expressed  in  terms  of  theta  quotients. 

219.     Consider,  nextly,  the  function 


334 


ADDITION    FORMULA    FOR   CERTAIN 


[219 


This  is  not  a  periodic  function  of  u,  u .     Thus  we  take  in  the  first  place 
the  function 


Put 


^  (u)  ^  (u\ua»  a)  ^  (u')  %  (u  ua><  «) ' 
u  =  ux> >  a>  +  ux*>  "»,  u'  =  uxi'  ai  +  u**' 


then,  as  functions  of  x1}  the  zeros  of  ^  (u),  *b(u\ua"a)  respectively  are  a,  x2 
and  Oj,  a;2,  the  zeros  of  ^(u  +  u'\uai1  a)  are  found  in  the  usual  way  to  be  zeros 
of  a  rational  function  of  the  fifth  order  having  af,  a.2s  as  poles,  and  xz,  a?/,  #2' 
as  zeros;  such  a  function  of  #j  is  AX/P  (a^),  where  P  (#1)  =  (xl  —  a^  (xl  —  a2)  and 

i/!  (a^  -  cO,    x?  ,    xl  ,  1   ! 

'?2    (^2  ^h  )>      «^2    >      ^2  >    •*• 

%'  (a?/  -  ax),   ar/2,   a;/,  1 


wherein  ^  =  yx/P  (a?,),  etc.  ;  the  zeros  of  *b(u  -  w')>  as  a  function  of  xlt  are 
similarly  zeros  of  a  function  of  the  sixth  order  having  a^,  a23  as  poles  and 
a,  tf2,  x±,  x2'  for  its  other  zeros  ;  such  a  function  of  xl  is  A/P(a?i),  where 


A  = 


hence  we  find 


^2 


-  77j  V,      - 


-772V,    -773',    a?/,    1 


*t  (u) ^  (u\ua> >  a)  ^ (u') ^ (u' | M°« •  a) 


=  (7 


!  A  (a^  —  «2)  (a?2  —  q2)  (a?!7  -  a2)  (#/  —  a2) 


#2)2  (a?!  —  a?/)  (a;x  —  #/)  (a;2  —  a;/)  (x2  —  x£)  (a;/  —  a;2')2  ' 

wherein  C  is  an  absolute  constant  ;  for  it  is  immediately  seen  that  the  two 
sides  of  this  equation  have  the  same  poles  and  zeros. 

We  proceed  to  put  the  right-hand  side  into  a  particular  form;  for  this  purpose  we 
introduce  certain  notations;  denote  the  quantities  c,  cl5  c2,  which  refer  to  the  branch 
places  other  than  ax,  a2  by  a3,  a4,  «6  in  any  order;  denote  («i  -  x^)  («j  -  #2)  by  pi, 
(cti  -  x{]  («j  —  x2')  by  p^  ;  denote  by  TTJ,  $  the  expression 


i  f  ^1  .  ff2  1      1 

L(^i  -  «i)  (^i  -  «>)     (*»  ~  «i)  («a  -  %)  J  *«  -  ^i  ' 


and  write  jo^y  for  pipjiri,  y,  with  a  similar  notation  n'i,  y,  ?)'i,  y  ;  also  let  P  (x)  =  (.v-  a:)  (^  -  a2)> 
1i=yilp(xi)>  etc- 

Then,  by  regarding  the  expression 


(„         V  \  (n         f  '\  (ft    —  T  '\ 

(a%  —  &%)  ^c*2  —  o-j )  ^«2     ^2  < 


219]  HYPERELLIPTIC   FUNCTIONS   OF  THE   FIRST   ORDER.  335 

as  a  function  of  «2,  and  putting  it  into  partial  fractions  in  the  ordinary  way,  we  find  that 
it  is  equal  to 

-1-  (*/  -.<)*  (x.  -  «3)  iaz^azf^  +  .  _!_,  K  _  Xtf  (x  _  ^  (*i'-«0(«i'-«j? 

~  "--  -  3' 


using  then  the  identities 

-  (*a  -  «s)  (*/  -  #2')  =  fo'  -  #2)  to'  -  «3)  -  «  ~  #a)  (**  ~  «s)> 
to  -  «3)  «  -  #2')  =  to'  -  a?2)  to'  -  03)  -  to'  -  a?2)  (x{  -  03), 

we  are  able  to  give  the  same  expression  the  form 


. 

1   —     2 

where  1  1;^  =  (Xl  -  «3)  (^  -  a4)  (^  -  «.),  etc.  ;  thus 


=  -  («2  -  a4)  («2  -  «5)  (^'  -  ^2')2  (^/  -  *z)  (^2'  ~  ^2)  (xi  ~  az)  (x*  ~  «s)  —3—79 

f*2  J?2"' 
+  ^1  ^l'  ~  ^2)  W  ~  #2)  ((^2'  ~  «2)  (^2'  ~  «3)  (*'/  ~  «4)  «  -  «5) 

+  (•»/  -  «2)  (^i'  -  «3)  (#2'  -  a4)  (a:2'  - 
Now  we  have,  by  expansion, 

^  =     (J?i'?2+I?i'W)  (^1-^2)  (•^I'-^ 


and  in  the  product  AA  there  will  be  two  kinds  of  terms 

(i)  -  »h  V  (»7i  -  172)  y  (*i  -  xj  «  +^2'  -  2«!), 

where  y  denotes  to'  -a?,)  to'-a?2)  to'-^Jto'-^g),  there  being  four  terms  of  this  kind 
obtainable  from  this  by  the  interchange  of  the  suffixes  1  and  2,  and  the  interchange  of 
dashed  and  undashed  letters, 

(ii)    77,  (^2'  -  Xl)  to'  -  xj  to  -  j?s)  {,,'«  (^'  -  «,)  (^  -  xtf  +  r,^  (^  -  04)  «  -  .r2)2 

-^2to-a,)to'-.r2')2}, 
there  being  three  other  terms  similarly  derivable  from  this  one. 

Consider  now  the  expression 


and,  of  this,  consider  only  the  terms 

(a.-,  -  at)  (og  -  o6 


336  ADDITION   FORMULA   FOR   CERTAIN  [219 

by  substitution  of  the  values  for  pls  etc.,  and  arrangement,  we  immediately  find  that  these 
terms  are  equal  to 


this  expression,  as  we  see  by  utilising  an  identity  which  was  developed  at  the  commence 
ment  of  the  investigation,  is  equal  to 


w  ,  —  SJT, 

-     g         1  -     2  -     2     -1  -     2  ~     2)  (^8  ~  -^2) 

where  K  denotes 

>7i  th'  2  (^/  -  «i)  (xi  ~  xtf  +  12  2  (•<  -  «i)  «  -  #2)  -  "722  (*a  -  «i)  (^i'  -  ^2')2] 


Comparing  this  form  with  the  terms  occurring  in  the  expansion  for  AAj,  we  obtain  the 
result 


Now  we  have  (§§  216,  213,  212)  the  formulae  p?=ntf,        {=±(ai-aj}         2  ;   we 

2t  9^  /*t  ^y 

shall  therefore  pui  pt  =  Mfqi,  Pi,j  =  -^i,jqi,j  ;  hence  by  the  formula  (p.  334)  the  quotient 

"tt)^  (u  -  u') 


is  a  certain  constant  multiple  of  the  function 


Also  we  have  M2=m,  N\tj=  +  /xiW/(a,--o>-),  where  m  =  ±  V -/'  («i)  when  i=l  or  2, 
and  /xj=±\//'(ai)  when  i=3,  4,  5.  Hence  it  is  easy  to  prove  that  the  fourth  powers 
of  the  quantities  (a2  -  «4)  («2 -  a5)  M1M3N13,  NnN^N^Mz  are  equal. 

Hence  we  have 


where  ^4.  is  a  certain  constant,  and  e  a  certain  fourth  root  of  unity.     The 
value  of  e  is  determined  by  a  subsequent  formula. 

220.     The  equation  just  obtained  (§  219)  taken  with  a  previous  formula 
gives  the  result 

a»a)  _  e  (guggg/  -f  gVsg/fr)  -I-  qi^q'^q'^  +  q'nq^'q^q^ 


V2 


221]  HYPERELLIPTIC    FUNCTIONS   OF   THE   FIRST   ORDER.  337 

and  limiting  ourselves  to  one  case,  we  may  now  take  the  places  az,  «4,  as  to 
be,  respectively,  c1}  c2,  c,  and  introduce  Weierstrass's  theta  functions; 
defining*  the  ten  even  functions  ^s(u),  ^.23(u),  ...,^03(u)  to  be  respectively 
identical  with  the  functions  ^(u),  ^ac(u),  ...,  ^cai(u),  and  the  six  odd  functions 
X_>  (u),  .  .  .,  ^3  (u)  to  be  respectively  the  negatives  of  the  functions  ^(MI  (u),  ...,  ^-CCi  (u), 
the  right-hand  side  of  the  equation  is  equivalent  to 

-  /(X.  <\.     <X>     Ci.'        i    CW     CL.     CL    \    i    (X.    C^.     <y     <\  '  -U  V     V     *V     ^V 

fc  ^  rJg  JQ2  ~01~   12    i     '•'S  ~  0-2  ~01  rJ12/     i     '-'04  '-'24  «  14  *->3    ~T  ~  04  ~  24  '•'H  '•*3  . 


here  ^-  denotes  ^-(w),  V  denotes  *b(u'),  and  (7  is  an  absolute  constant. 
This  equation  may  be  called  the  addition  forrnula  for  the  function  ql}  and  is 
one  of  a  set  which  are  the  generalisation  to  the  case  p  =  2  of  such  formulae 
as  that  arising  for  p  =  1  in  the  form 

,.      sn  u  en  u'  dn  u'  +  sn  u'  en  u  dn  u 

l-frsn'ttBn'u' 

By  interchanging  the  suffixes  1  and  2  we  obtain  an  analogous  expression 
for  (b(u  +  u'\ua*>a)-7-'&(u  +  u');  if  in  this  expression  we  add  the  half-period 
ua»a  to  u  we  obtain  an  expression  for  the  function  *&(u  +  u  ua"a  +  ua*'a) 
-r-*b(ii  +  u'\uai>  °);  and  if  this  be  multiplied  by  the  expression  just  developed 
for  the  function  ^(u  +u'\uai>  a)  -r-  S-  (u  +  u)  we  obtain  an  expression  for 
S-  (u  +  u  uai-a  +  ua*>  a)  -r-  ^f  (u  +  u'),  and  it  can  be  shewn  that  the  form  obtained 
can  be  reduced  to  have  the  same  denominator  as  in  the  expression  here 
developed  at  length.  The  formulae  are  however  particular  cases  of  results 
obtained  in  subsequent  chapters,  and  will  not  be  further  developed  here. 
For  that  development  such  results  as  those  contained  in  the  following 
examples  are  necessary;  these  results  are  generalisations  of  such  formulae 
as  sn  (u  +  K}  =  en  w/dn  u  which  occur  in  the  case  p  =  1. 

Ex.     Prove,  if  qt  (u)  =  3(u\uai>  a)  +  9  (u\   qitj(u)  =  3(u\uai'a  +  uai>a)  +  3(u\  etc.,  that 
(see  the  table  §  204,  and  the  formulae  Chap.  X.  §  190) 


f/i 


and  obtain  the  complete  set  of  formulae. 

221  .  In  case  p  =  2  there  are  five  quotients  of  the  form  S-  (u\  ub<  a)  -=-  ^  (u), 
and  ten  of  the  form  ^(u\ub><  a+  ub*<a)  +  S-(w),  wherein  b,  blt  b.2  denote  any 
finite  branch  places.  Since  the  arguments  u  may  be  written  in  the  form 
ux»  a>  +  ux*>a*,  the  fifteen  quotients  are  connected  by  thirteen  algebraic 
relations.  In  virtue  of  the  algebraic  expression  of  these  fifteen  quotients, 
they  may  be  studied  independently  of  the  theta  functions.  We  therefore 
give  below  some  examples  of  the  equations  connecting  them. 

*  Konigsberger,  Crelle,  LXIV.  (1865),  p.  22.  In  the  letter  notation  (§  204)  the  reduced  charac 
teristic  symbols  are  such  (§  203)  that  each  of  k,,  k',  is  positive,  or  zero,  and  less  than  2.  In 
Weierstrass's  notation  the  reduced  symbols  have  the  elements  A;',  positive,  or  zero,  and  the  elements 
k,  negative,  or  zero. 

B.  22 


338  FORMULAE  CONNECTING  THE   THETA  FUNCTIONS  [221 

Ex.  i.  There  is  one  relation,  known  as  Gopel's  biquadratic  relation,  which  is  of 
importance  in  itself,  in  view  of  developments  that  have  arisen  from  it,  and  is  of  some 
historical  interest. 


I      (±4- 


be  three  functions  whose  suffixes,  together,  involve  all  the  five  finite  branch  places.  Then 
these  three  functions  satisfy  a  biquadratic  relation,  which,  if  the  functions  be  regarded  as 
Cartesian  coordinates  in  a  space  of  three  dimensions,  represents  a  quartic  surface  with 
sixteen  nodal  points. 


In  fact,  if  pa  denote  \/(«  -  #1)  («  —  #2)*  an<^  Pb    b  denote  the  function 


we  have 


where  6U  62,  elt  e2,  es  are  the  finite  branch  places  in  any  order  ;  and  if  this  be  denoted  by 


it  is  immediately  obvious  that  ^  (^,  ^)  =  2^2,  =2/(.r),  say,  and    x-  ^(.r,  2)         =  ^—  ;  tnus 
there  is  (§  211,  Ex.  vii.)  an  equation  of  the  form 


where  /(^1}  ^2)  ^s  a  certain  symmetrical  expression  of  frequent  occurrence  (cf.  §  217),  the 
same  whatever  branch  places  6n  62  may  be,  and  A,  B,  C  are  such  that  ^  (#x,  #2)  vanishes 
when  for  xlt  x2  are  put  any  one  of  the  four  pairs  of  values  (6lt  &2),  (e2,  e3),  (e3,  ej,  (elt  ez)  ; 
therefore  the  difference  between  any  two  expressions  such  as  y?b  b  ,  formed  for  different 
pairs  of  finite  branch  places,  is  expressible  in  the  form  Z#1#2  +  M  (xl+.v^)  +  N  ;  thus  there 
must  be  an  equation  of  the  form 


where  X,  /*,  v,  p  are  independent  of  the  places  #u  xz. 
Similarly 


But  also  it  can  be  verified  that 

Pa,  ,  a,PCl  ,  c,  -Pa,  ,  <A,  c, 
thus  we  have 

0, 


&,  0,  +  W.  c.+  '^c  +  P]  l>'lf  «,  +  /•>„  c2  +  ">c  +  P']  =  bai>  aA  ,  c2-^l2' 

and  when  the  expressions^    a  ,  etc.,  are  replaced  by  the  functions  qa    a  ,  etc.  (§  210),  this 
is  the  biquadratic  relation  in  question.     This  proof  is  practically  that  given  by  Gopel 
Crelle  xxxv.  1847     .  291. 


(Crelle,  xxxv.  1847,  p.  291). 


221]  WHEN  p   IS   EQUAL  TO   TWO,  339 

En:  ii.     Prove  that 


2  2 

alt  a2~Palt  c,  .     2 
~    a  _p—'+Pa 

t*o       v|  l 

2  2 


(«i  -  «i)  («i  -  c)      (cx  -  a^  (Cl  -  c)     (c  -  a,)  (c  -  GI 
and  hence  develop  the  method  of  Ex.  i.  in  detail. 


*l 


Ex.  iii.     For  any  value  of  p  prove 

(a)  that  the  squares  of  any  p 
ected  by  a  linear  relation, 

(/3)  that  the  squares  of  any  p  of  the  theta  quotients 


(a)  that  the  squares  of  any  p  of  the  theta  quotients  qb,   =  9  (u\ub-a)  +  3(u),  are 
connected  by  a  linear  relation, 


are  connected  by  a  linear  relation.     (Weierstrass,  Math.    Werke,  vol.  i.  p.  332.)     These 
equations  generalise  the  relations  of  Ex.  ii. 

Ex.  iv.     Another  method  of  obtaining  the  biquadratic  relations  is  as  follows  ;  if 

$    (v)    =^e2niv(n 


Tr=|v,  and,  in  Weierstrass's  notation, 


so  that  x  :  y  :  z  :  t  =  l  :  qa^  c^  :  qa^  Ci  :  qc,  and  if  a,  b,  c,  d  denote  the  values  of  M,  y,  z,  t 
when  v=0,  and  the  linear  function  cx  +  dy-az-bt  be  denoted  by  (c,  d,  -a,  -b),  etc., 
then  it  can  be  proved,  by  actual  multiplication  of  the  series,  that 

e32  (  V)  =  (c,  d,-a,-  b),     9142  (  T)  =  (d,  -  c,  -  b,  a),     e0./  (  F)  =  (b,  -a,d,-  c) 
Q^(V)  =  (a,b,c,d)       ,     e*  (  V)  =  (b,-a,-  d,c\     e^(V)  =  (a,b,-c,-cr). 

Relations  of  this  character  are  actually  obtained  by  Gopel,  in  this  way.  It  will  be 
sufficient,  for  the  purpose  of  introducing  the  subject  of  a  subsequent  chapter,  if  the 
method  of  obtaining  one  of  these  relations  be  explained  here.  The  general  term  of  the 
series  e^  (  F)  is  (cf.  the  table  §  204  and  §  220) 


where  g'  =  £(l,  °),  9'  =  i(lJ  0),  namely  is 
_  e"i  Oi  (Mi+i)+«2w2]  +Ji«  [TU 

thus  the  exponent  of  the  general  term  in  the  product  e^2  (  V)  is  niL,  where  L  is  equal  to 

7rt1  +  ^)m2] 

+  m^  +  ni+mi  +  l 

22—2 


340  FORMULAE   CONNECTING   THE  THETA   FUNCTIONS  [221 

there  are  therefore  four  kinds  of  terms  in  the  product  according  to  the  evenness  or 
oddness  of  the  two  integers  n^-\-m^  «a  +  m2.  Consider  only  one  kind,  namely  when 
ni+mi,  n<t  +  m-2  are  both  even,  respectively  equal  to  <2.Nl,  2JV2,  say;  then  L  is  equal  to 


•e  t.n\~m\       if     n2  —  m2       if 

if  now  we  put  -1  --  -  -l  =  Mlt    *         =M2,  we  have 


thus,  to  any  assigned  values  of  the  integers  Nlt  JV2,  Mlt  M2  there  correspond  integers 
MU  n2,  mlt  m2  such  that  n^m^  n2  +  m2  are  both  even  ;  therefore,  as 


is  a  term  of  the  series  3  (v  ;  £  (      )  J  ,  that  is,  of  B01  (v),  and 


is  a  term  of  the  series  5  (o  ;  |  ^^  ,  that  is,  of  36  («;),  and  e^<2^'+1'  =  -  l,  it  follows  that 


the  terms  of  e022  (  V)  which  are  of  the  kind  under  consideration  consist  of  all  the  terms  of 
the  product  -  55  .  501  (v),  or  -  ay.  It  can  similarly  be  seen  that  the  three  other  sorts  of 
terms,  when  Mj  +  wij  is  even  and  n2  +  m2  odd,  when  nl+ml  is  odd  and  »2+m2  odd  or  even, 
are,  in  their  aggregate  the  terms  of  the  sum  bx+dz  —  ct. 

We  can  also,  in  a  similar  way,  prove  the  equations 

©0362363  (  V)  014  (  V)  +  000,002  (  V)  Q.  (  V)  -  012001  0,  (  V)  034  (  F), 
0032  =  2  (ac  -  bd),  0232  =  2  (ad  +  be),  022  =  2  (a6  -  erf),  0012  =  2  (afe  +  erf), 


©03  denoting  003  (0),  etc. 

Hence  the  equation  of  the  quartic  surface  is  obtainable  in  the  form 
V2  (ac  -  bd)  (ad+bc)  (c,  rf,  -  a,  -  b)  (rf,  -c,  -  6~a) 
+  V(a2  -  62  -  c2  +  rf2)  (ab  -  erf)  (6,  -  a,  rf,  -  c)  (a,  b,  c,  rf) 


,  -a,  -d,c)(a,b,  -c,  -rf). 

A  relation  of  this  form  is  rationalised  by  Cayley  in  Crelle's  Journal,  LXXXIII.  (1877), 
p.  215.  The  form  obtained  is  shewn  by  Borchardt,  Crelle,  LXXXIII.  (1877),  p.  239,  to  be  the 
same  as  that  obtained  by  Gopel.  See  also  Kummer,  Berlin.  Monats.  1864,  p.  246,  and 
Berlin.  Abhand.  1866,  p.  64  ;  Cayley,  Crelle,  LXXXIV.,  xciv.  ;  and  Humbert,  Liouville,  4me  Ser., 
t.  ix.  (1893);  Schottky,  Crelle,  cv.  pp.  233,  269;  Wirtinger,  Untersuchungen  iiber  Theta- 
functionen  (Leipzig,  1895). 

The  rationalised  form  of  the  equation,  from  which  the  presence  of  the  sixteen  nodes  is 
obvious,  is  obtained  in  chapter  XV.  of  the  present  volume. 


221]  WHEN  p   IS   EQUAL   TO   TWO.  341 

Ex.  v.  Obtain  the  following  relations,  connecting  the  ratios  of  the  values  of  the  even 
theta  functions  for  zero  values  of  the  arguments  when  p  =  2.  They  may  be  obtained  from 
the  relations  (§  212) 

(&-*,)  (6-*2)  =  ±*Je"iPt"f>  (b)  V  (U\ub-  *)+&  (M) 
by  substituting  special  values  for  xl  and  x2. 

54  :  3*  :  3*    :  34    :  34       :  44       •  34       -A4       •  Q4      .  a4 
c         c,       "c2       "a^e,       ^a,Ca    •  ^a2Cl    •  ^a^    •  ^   .  9^ 

=  fa  -  c2)  (eg  -  c)  (c  -  Cl)  .  («!  -  Og)  :  (G^  -  a2)  («2  -  c)  (c  -  a,)  .  (c,  -  c2) 
:  (a,  -  og)  (ctg  -  Cj)  (cx  -  a,)  .  (c2  -  c)  :  (ax  -  a2)  (a2  -  c2)  (c2  -  ax)  .  (Cl  -  c) 
:  (eg  -  c)  (c  -  ax)  (a,  -  c2)  .  (c,  -  «2)  :  (c  -  GI)  (cx  -  a,)  (^  -  c)  .  (c2  -  «2) 
:  (c  -  cg)  (eg  -  og)  (ag  -  c)  .  (ct  -  aj  :  (c  -  cx)  (GI  -  «2)  («2  -  c)  .  (c2  -  ttl) 

•  («l-*j(e»-*d(*»-«d-(*i-o)  •  (C1-c2)(c2-a1)(a1-c1).(a2-c). 
Infer  that 

5^U  :  <A  :  ^<  =  K-ci)2  :  ("i-«,)2  :  («!-«,)'. 
We  have  proved  (§§  210,  213)  that 

-a  ^c    M  5aa    M  =  0 


and  we  have  in  fact,  as  follows  from  formulae  developed  subsequently,  the  equation 
3caA2«2-^,  fa)  Sa,Cl  (M)  +^lC25cai5a2  (M)  9aic,  (u)  =  3c3c^Cl  (u)  5a,a2  (i«). 

Ex.  vi.     Obtain  formulae  to  express  the  ratios  of  the  differential  coefficients  of  the  odd 
theta  functions  for  zero  values  of  the  arguments. 


Ex.  vii.     Prove  that 


(u)  =  f^ 

wherein  blt  62  are  any  two  finite  branch  places,  and  e  is  a  certain  fourth  root  of  unity. 

This  result  can   be  obtained  .  in   various   ways  ;    one  way  is  as  follows  :     Writing 
M  =  M*..  «.  +  #*..«.,  u  +  ub»a=v,  and  v  =  uZl>b>  +  uz*'b*,  we  find,  by  the  formula  3( 
=  e^(u)3(u;  P),  that 


and,  by  the  formula  expressing  &  (ux>  m-uXl'm<-  ......  -  uxi"  *"»)  -  fa  (u1*'  m  -  ux*  'm>- 

-  UXP<  »"P)  by  integrals  and  rational  functions,  the  right-hand  side  is  equal  to 


Sl  _s2_     -i 

-  &i)  («i  -  68)     («g  -  6,)  &  -  6g)  J ' 


where  sly  zl  are  the  values  of  y,  x  respectively  at  the  place  zly  and  s2,  z2  at  the  place  z2.' 
This  rational  function  of  «,,  22  is  however  (§  210)  a  certain  constant  multiple  of 
3  (v\ubt '  a  +  ub»  a)/3  (v),  and  hence  the  result  can  immediately  be  deduced. 

One  case  of  the  relation,  when  b19  62  are  the  places  a,,  a2,  is  expressible  by  Weierstrass's 
notation  in  the  form 


a_ 


342  FORMULA    FOR   DIFFERENTIAL   COEFFICIENTS.  [221 

and  it  is  interesting,  using  results  which  belong  to  the  later  part  of  this  volume,   to 
compare  this  with  other  methods  of  proof.     We  have* 


-v)  =  3S  (u)  5M  (tt)  $i  (v)  30  (v)  +  32  (u)  513 

(tt)  +  32  (t;)  5U  (*)  502  (tt)  5M  (tt), 


where  54,  50  denote  54(0),  50(0),  and  the  bar  denotes  an  odd  function;   if,  herein,  the 
arguments  vlt  vz  be  taken  very  small,  we  may  write  5  (u  +  v)  =  5 (tt)  +  ( vl  = — h  #2  ~—  )  5  (u). 

Thus  we  obtain,  eventually,  remembering  that  the  odd  functions,  and  the  first  differential 
coefficients  of  the  even  functions,  vanish  for  zero  values  of  the  arguments, 

where  y(u)  =  ^—3(u\  5  =  5(0),  5'  =  5'(0). 
d«2 

Thus,  by  the  formula  of  this  example,  putting  u  =  0,  we  infer  that 

-0 


or  3'o4  =  0,  and  the  result  of  the  general  formula  agrees  with  the  formula  of  this  example. 

In  the  cases  />>2  we  have  even  theta  functions  vanishing  for  zero  values  of  the 
argument ;  here  we  have  one  of  the  differential  coefficients  of  an  odd  function  vanishing 
for  zero  values  of  the  argument. 

Note.  Beside  the  references  given  in  this  chapter  there  is  a  paper  by  Bolza, 
American  Journal,  xvn.  11  (1895),  "On  the  first  and  second  derivatives  of  hyper- 
elliptic  (r-functions "  (see  A  eta  Math.  xx.  (Feb.  1896),  p.  1  :  "Zur  Lehre  von  den  hyper- 
elliptischen  Integralen,  von  Paul  Epstein"),  which  was  overlooked  till  the  chapter  was 
completed.  The  fundamental  formula  of  Klein,  utilised  by  Bolza,  is  developed,  in 
what  appeared  to  be  its  proper  place,  in  chapter  XIV.  of  the  present  volume.  See  also 
Wiltheiss,  Crelle,  xcix.  p.  247,  Math.  Annal.  xxxi.  p.  417;  Brioschi,  Rend.  d.  Ace.  dei 
Lincei,  (Rome),  1886,  p.  199;  and  further,  Konigsberger,  Crelle,  LXV.  (1866),  p.  342; 
Frobenius,  Crelle,  LXXXIX.  (1880),  p.  206. 

To  the  note  on  p.  301  should  be  added  the  references ;  Prym,  Zur  Theorie  der 
Functnen.  in  einer  zweibldtt.  FUicJie  (Ziirich,  1866),  p.  12;  Konigsberger,  Crelle,  LXIV.  p.  20. 
To  the  note  on  p.  296  should  be  added;  Harkness  and  Morley,  Theory  of  Functions, 
chapter  vin.,  on  double  theta  functions.  In  connection  with  §  205,  notations  for  theta 
functions  of  three  variables  are  given  by  Cayley  and  Borchardt,  Crelle,  LXXXVII.  (1878). 

*  Krause,  Hyperelliptische  Functional,  p.  44 ;  Konigsberger,  Crelle,  LXIV.  p.  28. 


223] 


CHAPTER  XII. 

A   PARTICULAR   FORM  OF   FUNDAMENTAL   SURFACE. 

222.  JACOBI'S  inversion  theorem,  and  the  resulting  theta  functions,  with 
which  we  have  been  concerned  in  the  three  preceding  chapters,  may  be 
regarded  as  introducing  a  method  for  the  change  of  the  independent  variables 
upon  which  the  fundamental  algebraic  equation,  and  the  functions  associated 
therewith,  depend.  The  theta  functions,  once  obtained,  may  be  considered 
independently  of  the  fundamental  algebraic  equation,  and  as  introductory  to 
the  general  theory  of  multiply-periodic  functions  of  several  variables  ;  the 
theory  is  resumed  from  this  point  of  view  in  chapter  XV.,  and  the  reader 
who  wishes  may  pass  at  once  to  that  chapter.  But  there  are  several  further 
matters  of  which  it  is  proper  to  give  some  account  here.  The  present  chapter 
deals  with  a  particular  case  of  a  theory  which  is  historically  a  development* 
of  the  theory  of  this  volume  ;  it  is  shewn  that  on  a  surface  which  is  in  many 
ways  simpler  than  a  Riemann  surface,  functions  can  be  constructed  entirely 
analogous  to  the  functions  existing  on  a  Riemann  surface.  The  suggestion  is 
that  there  exists  a  conformal  representation  of  a  Riemann  surface  upon  such 
a  surface  as  that  here  considered,  which  would  then  furnish  an  effective 
change  of  the  independent  variables  of  the  Riemann  surface.  We  do  not 
however  at  present  undertake  the  justification  of  that  suggestion,  nor  do 
we  assume  any  familiarity  with  the  general  theory  referred  to.  The  present 
particular  case  has  the  historical  interest  that  in  it  a  function  has  arisen, 
which  we  may  call  the  Schottky-Klein  prime  function,  which  is  of  great 
importance  for  any  Riemann  surface. 

223.  Let  a,  /3,  7,  8  be  any  quantities  whatever,  whereof  three  are 
definitely  assigned,  and  the  fourth  thence  determined  by  the  relation 
aS  —  /3y  =  l.  Let  £,  £'  be  two  corresponding  complex  variables  associated 
together  by  the  relation  f  =  (a£  +  /3)/(y£  +  8).  This  relation  can  be  put  into 
the  form 


Referred  to  by  Riemann  himself,  Ges.  Werke  (Leipzig,  1876),  p.  413. 


344 


FORMATION   OF   A   GROUP   OF   SUBSTITUTIONS 


[22:i 


wherein  p  is  real,  and  B,  A  are  the  roots  of  the  quadratic  equation 
£=(«£"  +  /3)/(7£+  S),  distinguished  from  one  another  by  the  condition  that 
fj,  shall  be  less  than  unity.  In  all  the  linear  substitutions  which  occur  in 
this  chapter  it  is  assumed  that  B,  A  are  not  equal,  and  that  p  is  not  equal  to 
unity.  We  introduce  now  the  ordinary  representation  of  complex  quantities 
by  the  points  of  a  plane.  Let  the  points  A,  B  be  marked  as  in  the  figure  (6), 

Fig.  6. 


and  a  point  C'  be  taken  between  A,  B  in  such  a  way  that  1  >  AC'/C'B  >  p, 
but  otherwise  arbitrarily  ;  then  the  locus  of  a  point  P  such  that  AP/PB 
=  AC'/C'B  is  a  circle.  Take  now  a  point  C  also  between  A  and  B,  such  that 
CB/A  C=  pC'SfAC',  and  mark  the  circle  which  is  the  locus  of  a  point  P' 
for  which  P'B(AP'=CB/AC;  since  P'B/AP'  is  less  than  unity,  this  circle 
will  lie  entirely  without  the  other  circle.  If  now  any  circle  through  the 
points  A,  B  cut  the  first  circle,  which  we  shall  call  the  circle  C',  in  the  points 
P,  Q,  and  cut  the  second  circle,  C,  in  Px  and  Qj  ,  P  and  Pj  being  on  the  same 
side  of  AB,  we  have  angle  AP^B  =  angle  APB,  and  P1B/APl  =  pPB/AP  ; 
therefore,  if  the  point  P  be  £,  and  the  point  Pj  be  £,  we  have 


the  argument  of  P  vanishing  when  P  is  at  the  end  of  the  diameter  of  the 
C'  circle  remote  from  C",  and  varying  from  0  to  2?r  as  P  describes  the  circle 
C'  in  a  clockwise  direction  ;  if  then  we  pass  along  the  circle  C  in  a  counter 
clockwise  direction  to  a  point  P'  such  that  the  sum  of  the  necessary  positive 
rotation  of  the  line  BP1  about  B  into  the  position  BP',  and  the  necessary 
negative  rotation  of  the  line  APl  about  A  into  the  position  AP',  is  K,  and  f 
be  the  point  P',  we  have 


-  /,I 

~ 


Thus  the  transformation  under  consideration  transforms  any  point  £  on 
the  circle  C'  into  a  point  on  the  circle  C.     If  £  denote  any  point  within  C' 


224]  IN   CONNECTION   WITH   2p   CIRCLES.  345 


the  modulus  of  (£-  B)/(£  —  A)  is  greater  than  when  £  is  on  the  circumference 
of  G',  and  the  transformed  point  £"  is  without  the  circle  C,  though  not 
necessarily  without  the  circle  C'.  If  £  denote  any  point  without  G'  the 
transformed  point  is  within  the  circle  G. 

224.  Suppose  *  now  we  have  given  p  such  transformations  as  have  been 
described,  depending  therefore  on  3p  given  complex  quantities,  whereof  3  can 
be  given  arbitrary  values  by  a  suitable  transformation  z'  =  (Pz  +  Q)/(Rz  +  $) 
applied  to  the  whole  plane  ;  denote  the  general  one  by 


.  wherein  o^  -  &••/<  =  !>          (i  =  1,  2,  .  .  .  ,  p), 


or  also  by 


the  quantities  corresponding  to  A,  B,  /A,  a  being  denoted  by  Aiy  Bi,  fj,i}  cti  ; 
construct  as  here  a  pair  of  circles  corresponding  to  each  substitution,  and 
assume  that  the  constants  are  such  that,  of  the  2p  circles  obtained,  each  is 
exterior  to  all  the  others  ;  let  the  region  exterior  to  all  the  circles  be  denoted 
by  S,  and  the  region  derivable  therefrom  by  the  substitution  ^  be  denoted 
by  *& 

If  the  whole  plane  exterior  to  the  circle  Ci  be  subjected  to  the  trans 
formation  S-;,  the  circle  C{  will  be  transformed  into  Cit  the  circle  Ct  itself 
will  be  transformed  into  a  circle  interior  to  Ci}  which  we  denote  by  ^(7;,  and 
the  other  2p  —  2  circles  which  lie  in  a  space  bounded  by  Ct  and  C{  will  be 
transformed  into  circles  lying  in  the  region  bounded  by  ^iCt  and  Cit  and, 
corresponding  to  the  region  S,  exterior  to  all  the  2p  circles,  we  shall  have  a 
region  ^S  also  bounded  by  2p  circles.  But  suppose  that  before  we  thus 
transform  the  whole  plane  by  the  transformation  ^,  we  had  transformed 
the  whole  plane  by  another  transformation  ^  and  so  obtained,  within  Gj, 
a  region  %$  bounded  by  2p  circles,  of  which  Gj  is  one.  Then,  in  the 
subsequent  transformation,  S-f  ,  all  the  2p  —  l  circles  lying  within  Gj  will  be 
transformed,  along  with  Cj,  into  2p  -  1  other  circles  lying  in  a  region,  ^fyS, 
bounded  by  the  circle  ^Cj.  They  will  therefore  be  transformed  into  circles 
lying  within  ^(7,-  —  they  cannot  lie  without  this  circle,  namely  in  S-;$,  because 
*&iS  is  the  picture  of  a  space,  S,  whose  only  boundaries  are  the  2p  funda 
mental  circles  Clt  CV,  ...,  Cp,  Gp'.  Proceeding  in  the  manner  thus  indicated 
we  shall  obtain  by  induction  the  result  enunciated  in  the  following  statement, 
wherein  S^  is  the  inverse  transformation  to  ^,  and  transforms  the  circle  Gt 
into  Ci':  Let  all  possible  multiples  of  powers  of^l}  S-f  ,  ...,  *&p,  \l  be  formed, 
and  the  corresponding  regions,  obtained  by  applying  to  S  the  transformations 

*  The  subject-matter  of  this  section  is  given  by  Schottky,  Crelle,  ci.  (1887),  p.  227,  and 
by  Burnside,  Proc.  London  Math.  Soc.  xxni.  (1891),  p.  49. 


346 


DIAGRAM   TO   ILLUSTRATE   THE   RELATIONS 
Fig.  7. 


[224 


5* 

5 

DD 

»•* 

DD 
D 

an 

D 

n 
an 

a 
an 

a 

DD 

D 

an 

an 
a 

S-^-i 

fi-a  J 
•J  "«p 

an 

D 

Inn 

Sr'f'3 

< 

&*$-$ 

na 

an 

n 

DD 

3 

an 
a 

nn 
a 

ftty* 

a 
an 

a 
an 

aa 
a 

&<!>* 

n 

an 

3'/d>3"/ 

$4* 

a 

an 

an 
a 

an 
a 

an 
a 

an 
a 

« 

a 
aa 

a 

an 

»4f 

an 
n 

a 

an 

pSr* 

t-1 

V 

(Cl 

«J,-'S-' 

n 
na 

an 
a 

an 
a 

9 

«!• 

'•3 

an 
a 

nn 
a 

n 
an 

n 
nn 

D 

an 

n 
na 

a 

an 

n 
nn 

a 
an 

a 
aa 

na 
n 

•fr'Sty 

/ 

•fr-'S-ty 

na 
a 

nn 
n 

<j>-'S<f>-J 

<j>-^<f) 

aa 
a 

n 

nn 

psfr* 

j  ^<9& 
9  "-o 

a 
aa 

nn 
n 

an 
n 

na 
a 

na 
a 

ril 

•-J 

n 
an 

n 
an 

x~ 

nn 
n 

«f>-3 

t 

224] 


BETWEEN   THE    SUBSTITUTIONS   AND    THE    REGIONS. 
Fig.  7. 


347 


3  ,:«; 

* 

y 

D 
DD 

DD 
D 

DD 

D 

DD 

D 
DD 

D 

DD 

D 
DD 

DD 
D 

W 

3-4 

DD 
D 

DD 

ty-'fr' 

*p* 

D 
DD 

a 

DD 

a*a* 

d*fi 

D 
DD 

DD 
D 

DD 
D 

DD 
D 

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D 

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n 

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n 

„- 

* 

D 
DD 

D 

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D 
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af* 

s^ 

DD 
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<|>S-2 

J.A 

-j 

«j»s2 

n 
an 

DD 
D 

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4 

)O 

an 
a 

an 
n 

0 

DD 

D 
DD 

D 

an 

a 
an 

a 
an 

a 
an 

a 
an 

n 
an 

nn 

4>^''<|>- 

<j>s-^ 

an 

D 

an 
a 

W7 

4>3<J> 

an 
a 

a 
an 

#t$ri 

<j.2d 

a 
an 

an 
a 

DD 

a 

an 
a 

an 

D 

!> 

,4 

• 

a 

DD 

n 
an 

V 

an 
a 

348  CHARACTERISTICS   OF    THE    GROUP.  [224 

corresponding  to  all  such  products  of  powers,  be  marked  out.  In  any  such 
product  the  transformation  first  to  be  applied  is  that  one  which  stands  to  the 
right.  Let  m  be  any  one  such  product,  of  the  form 


m=  ......          /*, 

formed  by 

......  +  rt  +  rj  +rk,  =h 

factors,  and  let  ^  be  any  transformation  other  than  the  inverse  of  ^,  so  that 
m^fk  is  formed  by  the  product  ofh+l,  not  h  —  I,  factors.  Then  the  region  mS 
entirely  surrounds  the  region  m^S. 

Thus,  the  region  $r{$  entirely  surrounds  the  space  ^i&jS,  and  the  latter 
surrounds  $•£•/$,  or  ^ib/b^S  ;  but  ^ftS  is  surrounded  by  ^f^^S  or  S.  The 
reader  may  gain  further  clearness  on  this  point  by  consulting  the  figure  (7), 
wherein,  for  economy  of  space,  rectangles  are  drawn  in  place  of  circles,  and 
the  case  of  only  two  fundamental  substitutions,  S-,  <f>,  is  taken. 

The  consequence  of  the  previous  result  is  —  The  group  of  substitutions 
consisting  of  the  products  of  positive  and  negative  powers  of  S-x  ,  .  .  .  ,  %  gives 
rise  to  a  single  covering  of  the  whole  plane,  every  point  being  as  nearly  reached 
as  we  desire,  by  taking  a  sufficient  number  of  factors,  and  no  point  being 
reached  by  two  substitutions. 

225.  There  are  in  fact  certain  points  which  are  not  reached  as  trans 
formations  of  points  of  S,  by  taking  the  product  of  any  finite  number  of 
substitutions.  For  instance  the  substitution  ^m  is 

%    ~  ^i  %~  •"* 


and  thus  when  m  is  increased  indefinitely  £'  approaches  indefinitely  near  to 
BI  ,  whatever  be  the  position  of  £  ;  but  Bt  is  not  reached  for  any  finite  value 
of  m.  In  general  the  result  of  any  infinite  series  of  successive  substitutions, 
K  =  a/37  .  .  .  ,  applied  to  the  region  S,  is,  by  what  has  been  proved,  a  region 
lying  within  08,  in  fact  lying  within  a/3S,  nay  more,  lying  within  a@yS,  and 
so  on  —  namely  is  a  region  which  may  be  regarded  as  a  point  ;  denoting  it  by 
K,  the  substitution  K  transforms  every  point  of  the  region  8  and  in  fact 
every  other  point  of  the  plane  into  the  same  point  K  ;  and  transforms  the 
point  K  into  itself.  There  will  similarly  be  a  point  K'  arising  by  the  same 
infinite  series  of  substitutions  taken  in  the  reverse  order. 

Such  points  are  called  the  singular  points  of  the  group.  There  is  an 
infinite  number  of  them  ;  but  two  of  them  for  which  the  corresponding 
products  of  the  symbols  ^  agree  to  a  sufficient  number  of  the  left-hand 
factors  are  practically  indistinguishable  ;  none  of  them  lie  within  regions  that 
are  obtained  from  S  with  a  finite  number  of  substitutions.  The  most 
important  of  these  singular  points  are  those  for  which  the  corresponding 


226]  COMPOSITION    OF   TWO    SUBSTITUTIONS.  849 

scries  of  substitutions  is  periodic  ;  of  these  the  most  obvious  are  those  formed 
by  indefinite  repetition  of  one  of  the  fundamental  substitutions  ;  we  have 
already  introduced  the  notation 


to  represent  the  results  of  such  substitutions. 

226.     If  S-,  <f>  be  any  two  substitutions  given  respectively  by 
„ 


8' 
wherein  <z8  —  /3y  —-  1  =  AD  —  BC,  the  compound  substitution  ^<£  is  given  by 


D)     (7A  +  BC)  Z+(yB  +  SD)' 


and  if  this  be  represented  by  £"  =  («'£+  P')/(y'£+  8'),  we  have,  in  the  ordinary 
notation  of  matrices 

(  a!    £')  =  («     P  )  (  A     B  ), 


7 


C    D 


and  of  8'  -  fi'y  =  (08  - £7) (AD- BC)  =  1.  We  suppose  all  possible  substitu 
tions  arising  by  products  of  positive  and  negative  powers  of  the  fundamental 
substitutions  S-15  ...,  *&p  to  be  formed,  and  denote  any  general  substitution  by 
£'  =  (&£+ /3)/(y£+ 8),  wherein,  by  the  hypothesis  in  regard  to  the  funda 
mental  substitutions,  a&  —  fiy  =  l.  We  may  suppose  all  the  substitutions 
thus  arising  to  be  arranged  in  order,  there  being  first  the  identical  substitution 
£'  =  (f+  0)/(0.  £+  1),  then  the  2p  substitutions  whose  products  contain  one 
factor,  ^  or  ^r1,  then  the  2p(2p-l)  substitutions  whose  products  are  of 
one  of  the  forms  ^^-,  S^-1,  ^r1^,  ^r1^"1,  in  which  the  two  substitutions 
must  not  be  inverse,  containing  two  factors,  then  the  2p  (2p  — I)2  substitutions 
whose  products  contain  three  factors,  and  so  on.  So  arranged  consider  the 
series 

2  (mod  7)"*, 

wherein  &  is  a  real  positive  quantity,  and  the  series  extends  to  every  sub 
stitution  of  the  group  except  the  identical  substitution.  Since  the  inverse 
substitution  to  ?  =  (*S+/3)/(rt+B)  is  £=(B?  -  £)/(-  7f  +a),  each  set  of 
2p  (2p-  I)"-1  terms  corresponding  to  products  of  n  substitutions  will  contain 
each  of  its  terms  twice  over. 

Let  now  ®n  denote  a  substitution  formed  by  the  product  of  n  factors, 
and  @n+1  =  @n^t-,  where  ^  denotes  any  one  of  the  primary  2p  substitutions 
^1,^1  ,  -..,  \,  %  other  than  the  inverse  of  the  substitution  whose  symbol 
stands  at  the  right  hand  of  the  symbol  @n,  so  that  @n+1  is  formed  with  n  +  1 


350  POINCARE'S  INFINITE  SERIES  [226 

factors;  then  by  the  formula  just  set  down  <yn+1  =  yn<Xi  +  Sny{,  where,  if 
*t-,  or  £'  =(OiC+  &)/(7if+8i),  be  put  in  the  form  (£'  -  Bt)/(?  -  A{) 
=  Pi(£-  Bi)l(t;-Ai),  we  have 


respectively  equal  to 

Bjpj    -Ajpi          AjBj(pi    —p^      pi    -pi          Ajpj 


the  signification  of  p^   is  not  determined   when  the  corresponding  pair  of 
circles  is  given  ;  but  we  have  supposed   that  the  values  of  Of,  &•,  7;,  Si  are 

he  value  of  pt  .     By  these  formulae 

7n+i  _     _   &/fo  _      AJ  +  8nfyn 
~ 


given,  and  thereby  the  value  of  pt  .     By  these  formulae  we  have 


Herein  the  modulus  of  pi  may  be  either  fn  or  /if1,  according  as  S;  is  one 
of  Si,  ...,  Sp  or  one  of  Si"1,  •  ••>  S^1  ;  the  modulus  of  pi  is  accordingly  either 
less  or  greater  than  unity.  If  now  ®n  =  ...  >/r<£Sr  \  where  S>  is  one  of  the 
2p  fundamental  substitutions  S1(  ...,^fpl,  and  therefore  @^1  =  Sr^>~1/^~1..., 
the  region  ®nlS  lies  entirely  within  the  region  S>$  (§  224)  or  coincides  with 
it;  wherefore  the  point  ©^(oo  ),  or  —  Sn/Vn>  lies  within  the  circle  Cr  when 
S>  is  one  of  ^1(  ...,  *&p,  and  lies  within  the  circle  Gr'  when  X  is  one  of 
Si"1,  ...  ,  S^1;  thus  the  points  Bi  and  —Sn/yn  can  only  lie  within  the  same 
one  of  the  2p  fundamental  circles  C1}  ...,  C^,'  when  r=t  and  S>  is  one  of 
Si,  ...,Sy,  and  the  points  Ai  and  —Snfyn  can  only  lie  within  the  same  one  of 
the  2p  fundamental  circles  Clt  ...,  Cp'  when  r=i  and  Sr  is  one  of  S-f1,  ...,*bpl. 
Now,  if  the  modulus  of  p{  be  less  than  unity,  and  r  =  i,  ^fr  must  be  one 

of  Sf  ,  ...,  S-p  ,  namely  must  be  Sr1,  since  otherwise  @nSi  would  consist 

g 
of  n  —  1    factors,   and   not   n  +  1    factors  ;    in   that   case   therefore   Bi  +  — 

Vn 

is  not  of  infinitely  small  modulus  ;  if,  however,  the  modulus  of  p^  be 
greater  than  unity,  and  r  =  i,  S>  must  be  ^,  namely  one  of  Si,  ...,  Sp,  and 
in  that  case  the  modulus  of  A{  +  Sn/Yn  is  not  infinitely  small.  Thus,  according 
pi  ^1,  we  may  put 


as 


I   Bi  +  Bnfvn  \>\,  I   Ai  +  8n/ 

where  X  is  a  positive  real  quantity  which  is  certainly  not  less  than  the 

distance  of  Bi}  Ai}  respectively,  from  the  nearest  point  of  the  circle  within 
which  —  8n/yn  lies. 


227]  ASSOCIATED   WITH   THE   GROUP.  351 

It  follows  from  this  that  we  have 

mod  (7n+1/7«)  >  <r,  or  mod  (y~ljy~l)  <  -  . 

where  a-  is  a  positive  finite  quantity,  for  which  an  arbitrary  lower  limit  may 
be  assigned  independent  of  the  substitutions  of  which  ©„  is  compounded,  and 
independent  of  n,  provided  the  moduli  fj,1}  ...,  fj,p  be  supposed  sufficiently  small, 
and  the  p  pairs  of  circles  be  sufficiently  distant  from  one  another. 

Ex.     Prove,  in  §  223,  that  if  C'  be  chosen  so  that  C'C  is  as  great  as  possible 

J_  C"<7=1-V^_1 
fa  Ati~l+fa  fa 

and  the  circles  are  both  of  radius  c£  V/*/(l  -/*),  where  d  is  the  length  of  AB. 

We  suppose  the  necessary  conditions  to  be  satisfied  ;  then  if  j0  be  the 


least  of  the  p  quantities  mod  [(/*rVJi"<  -  ^.^/(Bi-Ai)],  and  k  be  posi 
tive,  the  series  2  mod  7"*  is  less  than 


\f)     ,  2jp(2p-l)      2»(2«-l)2  1 

2^  +  -^  l         '  +  *  —  L+  ......    , 

|_  *  a*  o-2* 


_)     , 
70         ^  +  - 

|_  * 

and  therefore  certainly  convergent  if  ck  >  ~2p  -  1,  which,  as  shewn  above,  may 
be  supposed,  //1(  ...,  /j,p  being  sufficiently  small. 

227.  Hence  we  can  draw  the  following  inference:  Let  a-1}  ...,  <rp  be 
assigned  quantities,  called  multipliers,  each  of  modulus  unity,  associated 
respectively  with  the  p  fundamental  substitutions  ^,  ...,  \;  with  any 
compound  substitution  VV2---,  let  the  compound  quantity  trf*af*...  be 
associated:  let  f(x)  denote  any  uniform  function  of  x  with  only  a  finite 
number  of  separated  infinities;  let  f  =  (a£  +  0)/(y£  +  8)  denote  any  sub 
stitution  of  the  group,  and  cr  be  the  multiplier  associated  with  this 
substitution  :  then  the  series,  extending  to  all  the  substitutions  of  the  group, 


converges  absolutely  and  uniformly  *  for  all  positions  of  f  other  than  (i)  the 
singular  points  of  the  group,  and  the  points  f=-g/7,  namely  the  points 
derivable  from  £=  GO  by  the  substitutions  of  the  group,  including  the  point 
f  =00  itself,  (ii)  the  infinities  of  /(£)  and  the  points  thence  derived  by  the 
substitutions  of  the  group.  The  series  represents  therefore  a  well-defined 
continuous  function  of  f  for  all  the  values  of  f  other  than  the  excepted  ones. 
The  function  will  have  poles  at  the  poles  of  /(£)  and  the  points  thence 
derived  by  the  substitutions  of  the  group;  it  may  have  essential  singularities 
at  the  singular  points  of  the  group  and  at  the  essential  singularities  of 


In  regard  to  f  ;  for  the  convergence  was  obtained  independently  of  the  value  of 


352  COMPARISON   OF   THE   £  PLANE  [227 


Denote  this  function  by  F(£);  if  S-0  denote  any  assigned  substitution 
of  the  group,  and  ^  denote  all  the  substitutions  of  the  group  in  turn,  it  is 
clear  that  ^0  denotes  all  the  substitutions  of  the  group  in  turn  including  the 
identical  substitution  ;  recognising  this  fact,  and  denoting  the  multiplier 
associated  with  ^0  by  <TO,  we  immediately  find 


or,  the  function  is  multiplied  by  the  factor  (TQ~l(^+  S0)k  when  the  variable 
£  is  transformed  by  the  substitution,  &0,  of  the  group.  Thence  also,  if  G(£) 
denote  a  similar  function  to  F(g),  formed  with  the  same  value  of  k  and 
a  different  function  /(£),  the  ratio  F(£)IG(g)  remains  entirely  unaltered 
when  the  variable  is  transformed  by  the  substitutions  of  the  group.  In  order 
to  point  out  the  significance  of  this  result  we  introduce  a  representation 
whereof  the  full  justification  is  subsequent  to  the  present  investigation. 
Let  a  Riemann  surface  be  taken,  on  which  the  2p  period  loops  are  cut  ;  let 
the  circumference  of  the  circle  Ct  of  the  £  plane  be  associated  with  one  side 
of  the  period  loop  (6t-)  of  the  second  kind,  and  the  circumference  of  the  circle 
Ci  with  the  other  side  of  this  loop  ;  let  an  arbitrary  curve  which  we  shall 
call  the  t'-th  barrier  be  drawn  in  the  £  plane  from  an  arbitrary  point  P 
of  the  circle  (7/  to  the  corresponding  point  P'  of  the  circle  Git  and  let  the 
two  sides  of  this  curve  be  associated  with  the  two  sides  of  the  period  loop 
(di)  of  the  Riemann  surface.  Then  the  function  F(%)/G(£),  which  has  the 
same  value  at  any  two  near  points  on  opposite  sides  of  the  barrier,  and 
has  the  same  value  at  any  point  Q  of  the  circle  G{  as  at  the  corresponding 
point  Q'  of  the  circle  C{,  will  correspond  to  a  function  uniform  on  the 
undissected  Riemann  surface.  In  this  representation  the  whole  of  the 
Riemann  surface  corresponds  to  the  region  S  ;  any  region  ^S  corresponds  to 
a  repetition  of  the  Riemann  surface  ;  thus  if  the  only  essential  singularities 
of  JP(£)/6r(f)  be  at  the  singular  points  of  the  group,  none  of  which  are 
within  8,  F(£)/G(£)  corresponds  to  a  rational  function  on  the  Riemann 
surface.  It  will  appear  that  the  correspondence  thus  indicated  extends  to 
the  integrals  of  rational  functions  ;  of  such  integrals  not  all  the  values  can 
be  represented  on  the  dissected  Riemann  surface,  while  on  the  undissected 
surface  they  are  not  uniform  ;  for  instance,  of  an  integral  of  the  first  kind, 
ut,  the  values  in,  Mi+2a>i>r,  w;  +  2&>'iir,  m  +  2a>f)  r  +  2a)'it  r  may  be  repre 
sented,  but  in  that  case  not  the  value  u{  +  4<w,:)  r  ;  in  view  of  this  fact  the 
repetition  of  the  Riemann  surface  associated  with  the  regions  derived  from 
8  by  the  substitutions  of  the  group  is  of  especial  interest  —  we  are  able  to 
represent  more  of  the  values  of  the  integral  in  the  %  plane  than  on  the 
Riemann  surface.  These  remarks  will  be  clearer  after  what  follows. 

228.  In  what  follows  we  consider  only  a  simple  case  of  the  function 
F(Q,  that  in  which  the  multipliers  alf  ...,  <rp  are  all  unity,  k  =  2,  and 
/(£)  =  !/(£—  a),  a  being  a  point  which,  for  the  sake  of  definiteness,  we 


228]  WITH    A   RIEMANN   SURFACE.  353 

suppose  to  be  in  the  region  S,  We  denote  by  &  =  ^  (£)  =  (a£  +  &)/(7i(T  +  ^<) 
all  the  substitutions  of  the  group,  in  turn,  and  call  £f  the  analogue  of  £  by 
the  substitution  in  question.  The  function 


has  essential  singularities  at  the  singular  points  of  the  group,  and  has  poles 
at  the  places  %=a,  £=  oo  and  at  the  analogues  of  these  places.  Let  the 
points  oo  ,  a  be  joined  by  an  arbitrary  barrier  lying  in  S,  and  the  analogues  of 
this  barrier  be  drawn  in  the  other  regions.  Then  the  integral  of  this 
uniformly  convergent  series,  from  an  arbitrary  point  £,  namely,  the  series 


is  competent  to  represent  a  function  of  f  which  can  only  deviate  from  uniformity 
when  £  describes  a  contour  enclosing  more  of  the  points  a  and  its  analogues 
than  of  the  points  oo  and  its  analogues  ;  this  is  prevented  by  the  barriers. 
Thus  the  function  is  uniform  over  the  whole  f  plane;  it  is  infinite  at  £=a 

like  log(f  —  a),  and  at  £=oo  like  —  log  (-^  I,  as  we  see  by  considering  the 


term  of  the  series  corresponding  to  the  identical  substitution  ;  its  value  on 
one  side  of  the  barrier  0.00  is  2?™'  greater  than  on  the  other  side  ;  it  has 
analogous  properties  in  the  analogues  of  the  points  a,  oo  ,  and  the  barrier  aoo  ; 
further,  if  £n  =  ^n(Z)  be  any  of  the  fundamental  substitutions  S-j,  ...,  <&p, 


where  £in  is  obtained  from  £  by  the  substitution  S^n  ;   since  the  first  and 
last  of  these  sums  contain  the  same  terms,  we  have 


and  the  right-hand  side  is  independent  of  £,  being  equal  to  II  «^f;  in  order 
to  prove  this  in  another  way,  and  obtain  at  the  same  time  a  result  which 
will  subsequently  be  useful,  we  introduce  an  abbreviated  notation  ;  denote 
the  substitution  S>  simply  by  the  letter  r;  then  if  j  be  in  turn  every  sub 
stitution  of  the  group  whose  product  symbol  has  not  a  positive  or  negative 
power  of  the  substitution  n  at  its  right-hand  end,  all  the  substitutions  of  the 
group  have  the  symbol  jnh,  h  being  in  turn  equal  to  all  positive  and  negative 
integers  (including  zero)  ;  hence 

2  [log  (£»  -  a)  -  log  (£  -  a)],  =  2  S  [log  (£M*  *  ,  -  a)  -  log  (&»*  -  a)], 

i  j    h 

is  equal  to 


B.  23 


I  D  R  A  FJ  y~ 

OF   THF 
TT-XTTTT-T-^-n  ^,-r  --,  , 


354  THE   KIEMANN    INTEGRALS  [228 

where  N  =  nx,  M  =  n"x>  ;  but,  in  fact,  £v  is  Bn,  and  £„  is  An  ;   thus  H^"^  is 
independent  of  £  ;  and  if  we  introduce  the  definition 


where  S-?l  is  one  of  the  £>  fundamental  substitutions,  and,  as  before,  j  denotes 
all  the  substitutions  whose  product  symbols  have  riot  a  power  of  n  at  the 
right-hand  end,  we  have 


a,  oo  a, 

If  for  abbreviation  we  put 


prove  that 

pf«-  f  _  2_  p£  £  =  7>c»>  c 

O.,  oo         (Tn       «.  °°  «,  =0 

c  being  an  arbitrary  point. 


229.     Introduce  now  the  function  Ua,b  defined  by  the  equation 


then,  because  a  cross  ratio  of  four  quantities  is  unaltered  by  the  same  linear 
transformation  applied  to  all  the  variables,  we  have  also 

_v.     /^-f/a.- 

-   log 


where  r,  denoting  S>,  =^~1,  becomes  in  turn  every  substitution  of  the  group. 
Thus  we  have 


where 


•   -  2  ~-        „,  6  , 


j  denoting  as  before  every  substitution  whose  product  symbol  has  not  a 
positive  or  negative  power  of  n  at  the  right-hand  end  and  £  being  arbitrary  ; 
hence  also 


where  ?*,  =  t"1,  denotes  every  substitution  of  the  group. 


230]  CONSIDERED   ON   THE    £  PLANE.  355 

There  are  essentially  only  p  such  functions  v»  °,  according  as  ^n  denotes 
^i,  ^2,  ...,  ^,;  for,  taking  the  expression  given  last  but  one,  and  putting 
n  =  st,  that  is,  ^n  =  &,&«,  we  have 

'a        *"'*  —     f»"^        *"* 


-  n  v  *"  -4-  n  "  * 
1  &«  H     £«  » 

where  r)  =  %t,  so  that 


and  in  particular,  when  st  is  the  identical  substitution,  as  we  see  by  the 

formula  itself, 

n       f  ,  a  .    £  « 
0  =  vg    +  v>  J 

thus,  if  r  denote  SY  &•/  .  .  .        .  .  .  ,  we  obtain 


V       = 


so  that  all  the  functions  v^  a  are  expressible  as  linear  functions  of  v\    ,  ...,  Vp     . 
230.     It  follows  from  the  formula 


that  the  function  vn'  rt  is  never  infinite  save  at  the  singular  points  of  the 
group.  But  it  is  not  an  uniform  function  of  £;  for  let  £  describe  the  circum 
ference  of  the  circle  Cn  in  a  counter  clockwise  direction  ;  then,  by  the  factor 

%—Bn,  v^a  increases  by  unity;  and  no  other  increase  arises;  for,  when  the 
region  within  the  circle  Cn,  constituted  by  *bnS  and  regions  of  the*  form 
^n</»S,  contains  a  point  S-j(5n),  the  product  representing  the  substitution  j  has 
a  positive  power  of  ^-n  as  its  left-hand  factor,  and  in  that  case  the  region 
contains  also  the  point  §j(An).  Similarly  if  £  describe  the  circle  Cn'  in  a 

clockwise  direction,  v^  increases  by  unity.  But  if  %  describe  the  circum 
ference  of  any  other  of  the  2p  circles,  no  increase  arises  in  the  value  of 

Vn  a,  for  the  existence  of  a  point  Sj  (Bn)  in  such  a  circle  involves  the  existence 
also  of  a  point  Sj  (An). 

It  follows  therefore  that  the  function  can  be  made  uniform  in  the  region 
S  by  drawing  the  barrier,  before  described,  from  an  arbitrary  point  P  of  Cn'  to 

the  corresponding  point  P'  of  Cn.  Then  v^,  a  is  greater  by  unity  on  one  side 
of  this  barrier  than  on  the  other  side.  Further  if  in  denote  any  one  of 
the  substitutions  ^1(  ...,  *$rp,  we  have 


*  Where  0  denotes  a  product  of  substitutions  in  which  ^~!  is  not  the  left-hand  factor. 

23—2 


356  THE  RIEMANN   INTEGRALS  [230 

where  £  is  arbitrary;  thus  as  nf'"'f  =  Ilf"')f,  the  difference  is  also  indepen 
dent  of  £  and  we  have,  introducing  a  symbol  for  this  constant  difference, 


It  follows  therefore  that  if  the  p  barriers,  connecting  the  pairs  of  circles 
Cn',  Cn,  and  their  analogues  for  all  the  substitutions,  be  drawn  in  the 

interiors  of  the  circles,  the  functions  Vi  °,  .  .  .  ,  vp  a  are  uniform  in  the  region  S, 
and  in  all  the  regions  derivable  therefrom  by  the  substitutions  of  the  group. 

The  behaviour  of  the  functions  Vi'a,  ...,  vpa  in  the  region  S  is  therefore 
entirely  analogous  to  that  of  the  Riemann  normal  integrals  upon  a  Riemann 
surface,  the  correspondence  of  the  pair  of  circumferences  Cn,  Cn'  and  the  two 
sides  of  the  barrier  P'P,  to  the  two  sides  of  the  period  loops  (bn),  (an),  on  the 
Riemann  surface,  being  complete.  And  the  regions  within  the  circles 
C\,  ...,  Cp  enable  us  to  represent,  in  an  uniform  manner,  all  the  values  of  the 
integrals  which  would  arise  on  the  Riemann  surface  if  the  period  loops  (bn) 
were  not  present.  Thus  the  £  plane  has  greater  powers  of  representation 
than  the  Riemann  surface.  Further  it  follows,  by  what  has  preceded,  that 
the  integral  IT0')6  is  entirely  analogous  to  the  Riemann  normal  elementary 
integral  of  the  third  kind  which  has  been  denoted  by  the  same  symbol  in 
considering  the  Riemann  surface.  On  the  Riemann  surface  the  period  loops 
(an)  are  not  wanted  for  this  function,  which  appears  as  a  particular  case  of  a 
more  general  canonical  integral  having  symmetrical  behaviour  in  regard  to 
the  first  and  second  kinds  of  period  loops  ;  but  the  loops  (bn)  are  necessary  ; 
they  render  the  function  uniform  by  preventing  the  introduction  of  all  the 
values  of  which  the  function  is  capable.  In  the  £  plane,  however*,  the 
function  is  uniform  for  all  values  of  £,  and  the  regions  interior  to  the  circles 
enable  us  to  represent  all  the  values  of  which  the  function  is  susceptible. 
Thus  the  introduction  of  Riemann's  normal  integrals  appears  a  more  natural 
process  in  the  case  of  the  £  plane  than  in  the  case  of  the  Riemann  surface 
itself. 

231.     We  may  obtain  a  product  expression  for  Tn>m  directly  from  the 
formula 

Cm  -*/(£«)       £»  -  %  (4 


let  k  denote  in  turn  every  substitution  whose  product  symbol  neither  has  a 
power  of  ^rm  at  its  left-hand  end  nor  a  power  of  S>,  at  its  right-hand  end  ; 
thus  we  may  write  d>«^»  %»,  or,  for  abbreviation,  j  =  m~hk  ;  and  for  every 
substitution  k,  the  substitution  j  has  all  the  forms  derivable  by  giving  to  h 
all  positive  and  negative  integral  values  including  zero,  except  that,  when  k 

*  Barriers  being  drawn  to  connect  the  infinities  of  the  function. 


232]  OF  THE  THIRD  AND   FIRST   KINDS.  357 

is  the  identical  substitution,  if  m  =  n,  h  can  only  have  the  one  value  zero  ; 
then  applying  S/1  to  every  quantity  of  the  cross  ratio  under  the  logarithm 
sign,  we  have 

JL    V  locr  (Zj-im  —  Bn  I  £j-im-^?A 
'  n.  in  —  o      •    •*-•  iu>i  \     i*  n          ~it  ~A 

2-rri   j      6  V  ?j-i  -  Bn  I    £,-_!  -  An  j 

=  —    2  IQ 


and  therefore,  if  m  be  not  equal  to  n, 


r  . 


V*)  -  Bj  **\Am)  -  Aj  ' 

while  when  m  =  •/?.,  separating  away  the  term  for  which  k  is  the  identical 
substitution, 

1 


—  2'  log 

*         * 


where  2'  denotes  that  the  identical  substitution,  ^  =  1,  is  not  included  ; 
thus 


where  s  denotes  every  substitution  of  the  group  other  than  the  identical 
substitution,  not  beginning  or  ending  with  a  power  of  X,  and  excluding 
every  substitution  of  which  the  inverse  has  already  occurred. 

These  formulae,  like  that  for  wj  a,  are  not  definite  unless  the  barriers  (§  227) 
are  drawn. 

232.     Ex.  i.     If  v,,'    =  un  +  iwn  ,  un,  iion  being  the  real  and  imaginary  parts  of  v%  a,  prove, 
as  in  the  case  of  a  Riemann  surface,  by  taking  the  integral  fu  dw  round  the  p  closed 

curves  each  formed  by  the  circumferences  of  a  pair  of  circles  and  the  two  sides  of  the 
barrier  joining  them,  that  the  imaginary  part  of  N*TU  +  ......  +  2A\Nzrl2  +  ......  is  positive, 

Ni  ,  .  .  .  ,  Nv  being  any  real  quantities,  and  u  +  iw  =  Nl  v*'  a  +  ......  +  N  /'  a.     Prove  also  the 

result  r,m  p=Tn,m  by  contour  integration. 

Ex.  ii.     Prove  that  the  function  of  f  expressed  by 


has  analogous  properties  to  Riemann's  normal  elementary  integral  of  the  second  kind. 
Ex.  iii.     Prove  that 

where  a,  =  («,a 


358  FURTHER   COMPARISON    WITH    A    RIEMANN   SURFACE. 

Ex.  iv.     With  the  notation 


prove  that 


[232 


*  (*,  t«)  -  *  (Z,  f )  =  2*1  ^  /'  "  =  *(*,  £„)  -  *  (Z,  5), 


where  £  is  an  arbitrary  point,  and  hence  prove  that  if  z,  clt  ...,  cp,  £  be  any  arbitrary 
points,  and  £1  =  ^  (£),  ...,  £P  =  SP  (£),  the  function  of  f  expressed  by 

*(*,  <T),     *(*,  I),     *(*,    &),  .-.,     *(*,  &) 


(cp>  0,     *  (cp,  '£),     *  (ep,  £),  .  .  .  ,     *  (cp,  |p) 
1      ,  1      ,  1       ,  .-.,  1 

is  unchanged  by  the  substitutions  of  the  group,  and  has  simple  poles  at  z,  c1?  ...  ,  cp,  and 
their  analogues,  and  a  simple  zero  at  £,  and  its  analogues.  Thus  the  function  is  similar  to 
the  function  ty(x,  a;  2,  cl  ,  ...,  cp)  of  §  122,  and  every  function  which  is  unchanged  by  the 
substitutions  of  the  group  can  be  expressed  by  means  of  it. 

As  a  function  of  z,  the  function  is  infinite  at  z=£,  z=£,  beside  being  infinite  at  z=oo  , 
and  its  analogues;  when  (aiz  +  pi)/(yiZ  +  8i')  is  put  for  z,  the  function  becomes  multiplied 
by  (yi2  +  $i)2-  This  last  circumstance  clearly  corresponds  with  the  fact  (§  123)  that 
\lr(x,a;  z,  clt  ...,  cp)  is  not  a  rational  function  of  z,  but  a  rational  function  multiplied  by 


Ex.  v.     Prove  that 


JEr.  vi.     In  case  p  =  l,  we  have 


where 


(a,  -  £)/(ar-  J)  =  (Mei'c)r  (a  -  J5)/(a  -  J  ). 
Putting,  for  abbreviation,  q  =  el7rr  =  v  pe1*,  and 


prove,  by  applying  the  fundamental  transformation  once,  that 


and  shew  that  0  (f)  is  a  multiple  of  the  Jacobian  theta  function  0  (/'  a,q;  £,  £). 

/-(D    /    ^"^? 

jEr.  vii.     Taking  two  circles  as  in  figure  6  (§  223),  let  C'BfAC'  =  ir  and  I7i    -r-^,  =  ^  ; 


take  an  arbitrary  real  quantity  a>,  and  a  pure  imaginary  quantity  a>'  =  ~  log  p,  and  let 

ITT 


233]  SOLUTION   OF  A   PROBLEM   OF   HYDRODYNAMICS.  359 

$>(u)  denote  Weierstrass's  elliptic  function  of  u  with  2o>,  2<a'  as  periods.  Then  prove, 
if  a,  c  denote  points  outside  both  the  circles,  a'  denote  the  inverse  point  of  a  in  regard  to 
either  one  of  the  circles,  and  P,  Q  be  arbitrary  real  quantities, 

(a)     that  the  function 

*      a-B  lc- 


is  unaltered  by  the  substitution  (£'  —  B)/(('  —  A)  =  n(£-B)/(£—A),  and  has  poles  of  the 
first  order,  outside  both  the  circles,  only  at  the  points  f  =a,  f  =c. 

O)    that  the  function, 
__  P+iQ  P-iQ 

\    1 


r3 j     *- 7?~| r3 T     ^ 7?~!  T^ 1     /•        /J~|  r*  \     a' K~\ 

&      'r-  log  —  |jp      — •  log  -  (f)     -r-  log  -      -  .         I  —  0  I   -^  \Q°  -    -7 

[_Z7T        (T  £—  A_]        \_iir        a  a  —  A_j         [_in        &  f — A_\        \_iir       a  ci'—A_\ 

is  real  on  the  circumference  of  each  circle,  and,  outside  both  the  circles,  has  a  pole  of  the 
first  order  only  at  the  point  f=«.  The  arbitraries  P,  Q  can  be  used  to  prescribe  the 
residue  at  this  pole. 

Ex.  viii.  Prove  that  any  two  uniform  functions  of  f  having  no  discontinuities  except 
poles,  which  are  unaltered  by  the  substitutions  of  the  group,  are  connected  by  an  algebraic 
relation  (cf.  §  235)  ;  and  that,  if  these  two  be  properly  chosen,  any  other  uniform  function 
of  £  having  no  discontinuities  except  poles,  which  is  unaltered  by  the  substitutions  of  the 
group,  can  be  expressed  rationally  in  terms  of  them.  The  development  of  the  theory  on 
these  lines  is  identical  with  the  theory  of  rational  functions  on  a  Eiemann  surface,  but 
is  simpler  on  account  of  the  absence  of  branch  places.  Thus  for  instance  we  have  a 
theory  of  fundamental  integral  functions,  an  integral  function  being  one  which  is  only 
infinite  in  the  poles  of  an  arbitrarily  chosen  function  x.  And  we  can  form  a  function  such 
as  E  (x,  z}  (§  124,  Chap.  VII.)  ;  but  the  essential  part  of  that  function  is  much  more 
simply  provided  by  the  function,  w  (f,  y),  investigated  in  the  following  article. 

233.  The  preceding  investigations  are  sufficient  to  explain  the  analogy 
between  the  present  theory  and  that  of  a  Riemann  surface.  We  come  now 
to  the  result  which  is  the  main  purpose  of  this  chapter.  In  the  equation 


where  {£,  y/Zi,  Ci]  denotes  a  cross  ratio,  let  the  point  z  approach  indefinitely 
near  to  £  and  the  point  c  approach  indefinitely  near  to  7;  then  separating 
away  the  term  belonging  to  the  identical  substitution,  and  associating  with 
the  term  belonging  to  any  other  substitution  that  belonging  to  the  inverse 
substitution,  we  have,  after  applying  a  linear  transformation  to  every  element 
of  the  cross  ratio  arising  from  the  inverse  substitution 

n*.  <  =  ion-  <*  -  P  <c  ~  ?>  +  vloo.  (*  -  0  (c<  -  7)  (*  -Jt)  (c  -  7.-) 

fcr  --'  0--- 


where  S'  denotes  that,  in  the  summation,  of  terms  arising  by  a  substitution 


360  INTRODUCTION   OF  THE   FUNDAMENTAL   FUNCTION  [233 

and  its  inverse,  only  one  is  to  be  taken,  and  the  identical  substitution  is 
excluded.     Thus  we  have* 


s=f,e=y 


where  IT  has  a  similar  signification  to  S'  and  {£,  7/7^,  £*}  denotes  a  cross 

i  i 

ratio.     Consider  now  the  expression 

«r(&7),    =  (C-  7)  IT  {£  7/71.  6}  5 

t 

it  has  clearly  the  following  properties  —  it  represents  a  perfectly  definite 
function  of  £  and  7,  single-valued  on  the  whole  £-plane  ;  it  depends  only  on 
two  variables,  and  vr  (£,  7)  =  —  '57(7,  £)  ;  as  a  function  of  £  it  is  infinite,  save 
for  the  singular  points  of  the  group,  only  at  £=00,  and  not  at  the  analogues 
of  £=  oo  ;  it  vanishes  only  at  £  =  7  and  the  analogues  of  this  point,  and 
limitf=y  ts  (£,  7)/(£—  7)  =  1.  Thus  the  function  may  be  expected  to  generalise 
the  irreducible  factor  of  the  form  x  —  a,  in  the  case  of  rational  functions,  and 
the  factor  <r  (u  —  a)  in  the  case  of  elliptic  functions,  and  to  serve  as  a  prime 
function  for  the  functions  of  £  now  under  consideration  (cf.  also  Chap.  VII. 
§  129  and  Chaps.  XIII.  and  XIV.).  It  should  be  noticed  that  the  value  of 
VT  (£,  7)  does  not  depend  upon  the  choice  we  make  in  the  product  between 
any  substitution  and  its  inverse  ;  this  follows  by  applying  the  substitution 
S  r1  to  every  element  of  any  factor. 

234.     We  enquire  now  as  to  the  behaviour  of  the  function  CT  (£,  7)  under 
the  substitutions  of  the  group.     It  will  be  proved  that 

«!?»,  7)  +h  g-^Y+K..) 


, 

where  (—  l^,  (—  !)*»  are  certain  +  signs  to  be  explained. 

This  result  can  be  obtained,  save  for  a  sign,  from  the  definition  of  CT  (£,  7), 

as  a  limit,  from  the  function  II  z]  \  ;  but  since,  for  our  purpose,  it  is  essential 
to  avoid  any  such  ambiguity,  and  because  we  wish  to  regard  the  function 
CT  (£,  7)  as  fundamental,  we  adopt  the  longer  method  of  dealing  directly  with 
the  product  (f—  7)  11'  {£,  7/7$,  &}.  We  imagine  the  barriers,  each  connecting 

i 

a  pair  of  circles,  which  are  necessary  to  render  the  functions  v\a,  ...,  wp'a 

*  This  function  occurs  in  Schottky,  Crelle,  ci.  (1887),  p.  242  (at  the  top  of  the  page).  See 
also  p.  253,  at  the  top.  The  function  is  modified,  for  a  Eiemann  surface,  by  Klein,  Math.  Annul. 
xxxvi.  (1890),  p.  13.  The  modified  function  occurs  also,  in  particular  cases,  in  a  paper  by 
Pick,  Math.  Annal.  xxix.,  and  in  Klein,  Math.  Annal.  xxxn.  (1888),  p.  367.  For  p  =  l,  the 
theta  function  was  of  course  expressed  in  factors  by  Jacobi.  The  function  employed  by  Bitter, 
Math.  Annal.  XT,IV.  (p.  291),  has  a  somewhat  different  character. 


234]  OF   THE   THEORY   OF   THIS    CHAPTER.  361 

uniform,  to  be  drawn;   then  the  quantities  rn>m,  rn,n  given  in  §  231,  and 

defined  by  vnm>  ,  vnn-    are  definite;  so  therefore  is  also  evlvny  and  the  quan 
tity  ewiTn'n,  which  is  equal  to 


IT 


A  n  — 


where  s  denotes  a  substitution,  other  than  the  identical  substitution,  not 
beginning  or  ending  with  a  power  of  *bn,  and  excluding  the  inverse  of  a 
substitution  which  has  already  occurred.  This  formula  raises  the  question 
whether  Kn,  which  we  take  positive,  is  to  be  regarded  as  less  than  2?r  or  not, 
since  otherwise  the  sign  of  e*l'"»  is  not  definite.  But  in  fact,  as  it  arises  in 

this  formula,  from  vfa' f,  log  /*n  +  iKn  is  the  value  of  log  [  |j -£  I  \,  --5M  when 

\S    ~  •»»/  t,—-"-nl 

f '  has  reached  £n  from  f  by  a  path  which  does  not  cross  the  barriers.  Thus  tcn 
is  perfectly  definite  when  the  barriers  are  drawn,  and  the  sign  of  the 
quantity 


is  perfectly  definite  and  independent  of  the  barriers.  We  denote  it  by 
(-  l)^"1.  The  annexed  figure  illustrates  two  ways  of  drawing  a  barrier 
PP.  In  the  first  case  /cn  is  less  than  2?r.  In  the  second  case  £'  must  pass 


once  round  the  point  B,  and  KH  is  greater  than  2?r.  When  Kn  is  thus 
determined,  the  expression  by  means  of  Kn  of  the  p£  which  occurs  in 
the  formulae  connecting  an>  /3n,  yn,  8n  and  An,  Bn,  pn,  for  instance  in  the 
formula  pn  =  (I  +  pn) / (an  +  Sn),  is  also  definite;  it  may  be  /4=/4»eii<tn  or 
Pn  =  -pn  e**n-  We  shall  put  p*  =  (-  1)^ g*  ei^n  If  the  whole  investigation 
had  been  commenced  with  a  different  sign  for  each  of  a.n,  /?„,  yn,  8n,  hn  would 
have  become  hn  —  l,  but  gn,  depending  only  on  the  circles  and  the  barrier, 
would  have  the  same  value. 

We  have 

CT  (£n,  7)  =  ?n  -  7  n/  (Tin  ~  7    7»"  ~  ?n      ?j-  ^ 

'' 


362  BEHAVIOUR   OF  THIS   FUNCTION  [234 

where  i  denotes  in  turn  all  substitutions  which  with  their  inverses  give  the 
whole  group,  except  the  identical  substitution  ;  thus  i  denotes  all  substitutions 
?ix  for  \=  1,  2,  3,  ...,  oo,  as  well  as  all  substitutions  nhsnk,  where  s  has  the 
significance  just  explained  and  h,  k  take  all  positive  and  negative  integer 
values  including  zero.  Therefore 

-  7    7«*  -  £M         £>-  £ 


jj      n*«i*_+  1_^  7 
A,  *,  A    £n>«im*  —  7 

£n  -  7  jj  £nA+l  -7  jj      £IA-£    jj  7nA  ~  £» 

(T-  7   A     £«A  -  7     A  £»A+I  -  f  A   7«x  -  f  ' 

-       (^n)n^—  7      (^.71X^8  —  £ 


^,  *     (^H)HA*  —  7       (Bn)nhs  —  £  h>  s<  k  ynhmk  —  £     ^nhsnk+l  —  £n  ' 

the  transformation  of  the  second  part  of  the  product  being  precisely  as  in  the 
first  part, 


-  7        Tn  -  7         n~       A     7  -  £«- 


7      ^MMftg  —          „    7  —  ^M-ta-i 


h,  s         nnhs  —  7    (n)nhs  ~       h,s,k     7  ~  £n-*sn-ft          n  ~ 
7?n-_g'    _7_~(T       (Tn  ~  ^n         (^n)n»»  ~  7    (.^!^! 


-  7    7  ~ 


since  &  and  —  k  have  the  same  range  of  signification  we  may  replace  —  k  by  h, 
in  the  last  form,  and  obtain,  by  a  rearrangement  of  the  second  product, 


.,  _ 

7)  -5«  -  ?'  7  -  ^n  A,  s      ~  7  -        n 

7  ~  (^n) 


*,  ^  7 

but,  from  the  formula 


^r=y,         Z  7_-») 

»    27r.  g-'~-' 


where  j  can    have  the  forms  ?IAS,  nhs-1,  or  be   the   identical  substitution, 
we  have 

**£  y=  {-Bn  7  -^l,  n  C-(JgnU  y-(An)nhg  n  ^-(^U-!  7-(^n))tA8-1  1 

{—A*    J  -  Bn  h,^-(An)nhs  '  7  -  (Bn)nhg  s,  h  ^-(A^nhs-i  '  7  -  (Bn)nk,-i  ' 


235]  UNDER   A   LINEAR   SUBSTITUTION   OF   THE   GROUP. 

therefore 


363 


7) 


—  An  s,h%n  —  (Bn)nha-\  '  £—  (An)nh 

-"-n 


TT 

S       -"n  s,  & 


*n  ~       n 


TT 


n-ft  —  An 
?t)s  ~  An 


and  hence 


(Bn)s-Bn-(An\-An' 


CT 


now  from   the   formula   (^  -  5B)/(C»  -  An)  =  Pn  (S  -  Bn)/(?-  An),    and    the 
values  of  an>  0n,  7n,  8n  given  in  §  226,  we  immediately  find 

or-  ^» 


thus,  as  pj  =  (-  1)^,4  e**"B,  we  have 


hence,  finally 


7-n  J 


where  (—  \)°*e  mrn.ne--lKn  js  independent  of  how  the  barriers  are  drawn,  and 
(-1)A"7«.  (~  lA^i  are  independent  of  the  signs  attached  to  yn  and  Sn. 

235.  The  function  w(f,  7),  whose  properties  have  thus  been  deduced 
immediately  from  its  expression  as  an  infinite  product,  supposed  to  be 
convergent,  may  be  regarded  as  fundamental.  Thus,  as  can  be  imme 
diately  verified,  the  integral  II£y  is  expressible  by  -07(^,7),  in  the  form 


y  , 

»*(**)*<&  tf)' 

and  thence  the  integrals  v^y  arise,  by  the  definition  v^y  = 
thence,  also,  integrals  with  algebraic  infinities,  by  the  definition 


,  and 


~dxLi*'a 

(cf.  Ex.  ii,  §  232).  Further,  if  F  (£)  denote  any  uniform  function  of  %  whose 
value  is  unaltered  by  the  substitutions  of  the  group,  which  has  no  discontinui 
ties  except  poles,  it  is  easy  to  prove,  by  contour  integration,  as  in  the  case  of 


364  EXAMPLES   OF   THIS    FUNCTION.  [235 

a  Riemann  surface,  (i)  That  F(£)  must  be  somewhere  infinite  in  the  region  S, 
(ii)  That  F(£)  takes  any  assigned  value  as  many  times  within  S  as  the  sum 
of  its  orders  of  infinity  within  8,  (iii)  That  if  a1}  ...,  ak  be  the  poles  and 
&,  ...,  fa  the  zeros  of  F  (£)  within  S,  and  the  barriers  be  supposed  drawn, 


where  m1}  ...,  mp,  m/,  ...,  mp'  are  definite  integers.     Thence  it  is  easy  to 
shew  that  the  ratio 


is  a  constant  for  all  values  of  £.     And  replacing  some  of  /3lf  ...,  ctk  in  this 
expression  by  suitable  analogues,  the  exponential  factor  may  be  absorbed. 

Ex.  In  the  elliptic  case  where  there  is  one  fundamental  substitution  (£  —  B)I(£'  —  A)  = 
p  (f  -  B)I(£-A\  we  have  (&  -  5)/(Cf  -  -4)  =  pi  (f-  ^)/(f-  -4),  and  thence  putting  ?«,  v,  respec 
tively  for  the  integrals  /,  ^,  so  that  e27rj'"=  (f-  ff)/((-A),  cl™=(y-  B)l(y-  A],  we 
immediately  find 


~  Ct  __  !  ~  2Pi  cos  2n"  (M  ~  y)  +P2i       >_.  _ 
—  -    *2 


7  ~~  y»    y~  d  (i  ~ p*)2  2i     s^n  ""^  sin  ""^ 

and  hence 

^?-^l     sii 


OT  (C'  y)  ~     2i     sin  TT«  sin  ^  ,2  (1  -  p*)2 

which*,  putting  enlT=p^,  is  equal  to 


where  w  is  an  arbitrary  quantity,  and 


236.  The  further  development  of  the  theory  of  functions  in  the  £  plane 
may  be  carried  out  on  the  lines  already  followed  in  the  case  of  the  Riemann 
surface.  We  limit  ourselves  to  some  indications  in  regard  to  matters  bearing 
on  the  main  object  of  this  chapter. 

The  excess  of  the  number  of  zeros  over  the  number  of  poles,  in  any 
region,  of  a  function  of  £,  /(£),  which  is  uniform  and  without  essential 
singularities  within  that  region,  is  of  course  equal  to  the  integral 


See,  for  instance,  Halphen,  Fonct.  Ellipt.  (Paris,  1886),  vol.  i.  p.  400. 


230]  INTRODUCTION   OF   THE   THETA   FUNCTIONS.  365 

taken  round  the  boundary  of  the  region.  If  we  consider,  for  example,  the 
function  £ln(£),  =  dvn  y/d£,  which  is  nowhere  infinite,  in  the  region  S,  the 
number  of  its  zeros  within  the  region  8  is 

-'^n^pi 
,(£r)    a»(pja 

where  the  dash  denotes  a  differentiation  in  regard  to  f,  and  the  sign  of 
summation  means  that  the  integral  is  taken  round  the  circles  C\'  ,  ...,  Cpf,  in 
a  counter-clockwise  direction.  Since  fln  (fr)  =  (7r£  +  8r)z  fln  (£),  the  value  is 


or  2p;  thus  as  Hn  (f)  vanishes  to  the  second  order  at  f=  GO  in  virtue  of  the 
denominator  d£  we  may  say  that  <foj  y  has  2p  -  2  zeros  in  the  region  £,  in 
general  distinct  from  £  =  x  .  The  function  flB  (f)  vanishes  in  every  analogue 
of  these  2p  -  2  places,  but  does  not  vanish  in  the  analogues  of  £=  co  . 

The  theory  of  the  theta  functions,  constructed  from  the  integrals  Vn  y,  and 
their  periods  rn>m,  will  subsist,  and,  as  in  the  case  of  the  Riemann  surface 
there  will,   corresponding  to  an   arbitrary  point   m,  which  we   take   in   the 
region  S,  be  points  ml}  ...,  mp  in  the  region  S,  such  that  the  zeros  of  the 
function    ©  (i£  m  -  «?•  .  ».  -  ......  -  ^,™,.)    are    the    places    ^  ^      ^  ^      Anf} 

corresponding  to  any  odd  half  period,  £OS),,,  there  will  be  places  nli...inp_l, 
in  the  region  S,  which,  repeated,  constitute  the  zero  of  a  differential  dtf>  *,  and 
satisfy  the  equations  typified  by 


The  values  of  the  quantities  e«T»,«  and  the  positions  of  m1}  ...,mp  may 
vary  when  the  barriers  which  are  necessary  to  define  the  periods  rn>m  are 
changed. 

But  it  is  one  of  the  main  results  of  the  representation  now  under 
consideration  that  a  particular  theta  function  is  derivable  immediately  from 
the  function  *r  (f,  7)  ;  and  hence,  as  is  shewn  in  chapter  XIV.,  that 
any  theta  function  can  be  so  derived.  Let  v  denote  the  integral  whose 
differential  vanishes  to  the  second  order  in  each  of  the  places  n1}  ....Wp.,. 
Consider  the  expression  */dv/d£  in  the  region  S.  It  has  no  infinities  and  it  is 
single-valued  in  the  neighbourhood  of  its  zeros,  as  follows  from  the  fact  that 
the  p  zeros  of  dv/d£  are  all  of  the  second  order.  Hence  if  the  region  S  be 
made  simply  connected  by  drawing  the  p  barriers,  and  joining  the  p  pairs  of 
circles  byp-l  further  barriers  (Cl),  ...  ,  (Cp_,),  of  which  (cr)  joins  the  circumfer 
ence  Cr'  to  the  circumference  Cr+l,  ^/dvjd^  will  be  uniform  in  the  region  8  so 
long  as  £  does  not  cross  any  of  the  barriers.  For  the  change  in  the  value  of 
when  f  is  taken  round  any  closed  circuit  may  then  be  obtained  by 


366  EXPRESSION   OF   w  (£,  7)   BY   THETA   FUNCTIONS.  [236 

considering  the  equivalent  circuits  enclosing  the  zeros.  But  in  fact  the 
barriers  (d),  ...,  (c^)  are  unnecessary;  to  see  this  it  is  sufficient  to  see  that 
any  circuit  in  the  region  8  which  entirely  surrounds  a  pair  of  circles,  such 
as  GI,  Clt  encloses  an  even  number  of  the  infinities  of  dv/d£  which  are  at  the 
singular  points  of  the  group.  Since  these  infinities  are  among  the  logarithmic 
zeros  and  poles  of  v{'  v,  ...,  vpy,  whereof  v  is  a  linear  function,  the  proof 
required  is  included  in  the  proof  that  any  one  of  the  functions  vf  Y,  ...,  v%y  is 
unaltered  when  taken  round  a  circuit  entirely  surrounding  a  pair  of  the 
circles,  such  as  d',  Q.  Thus  when  the  barriers  which  render  the  functions 

V\  ,  ...,vf  uniform  are  drawn,  the  function  *Jdv/d£  is  entirely  definite  within 
the  region  S,  save  for  an  arbitrary  constant  multiplier,  provided  the  sign  of 
the  function  be  given  for  some  one  point  in  the  region  S.  And,  this  being 

done,  if  7  be  any  point,  the  function  y^y  /  is  independent  of  this  sign. 

This  function,  with  a  certain  constant  multiplier,  which  will  be  afterwards 
assigned,  may  be  denoted  by  -^  (£). 

237.     We  proceed  now  to  prove  the  equation 

;:: 

where  s'v  '  y  =  sfa  '  y  +  ......  +  sp'vf}  y,  and  A  is  constant,  independent  of  f  and 

7.  It  is  clear  first  of  all  that  the  two  sides  of  this  equation  have  the  same 
poles  and  zeros  in  the  region  S.  For  ®  (v*'y  +  £fls,S')  vanishes  to  the  first 
order  at  the  places  7,  nlt  ...,  np_l}  and  ^(£)  vanishes  to  the  first  order  at 
n1}  ...,  np_1}  oo,  while  m  (£,  7)  vanishes  to  the  first  order  at  £=7,  and  is 
infinite  to  the  first  order  at  £=  QO  *.  Thus  the  quotient  of  the  two  sides  of  the 
equation  has  no  infinities  within  the  region  S.  Further  the  square  of  this 
quotient  is  uniform  within  the  region  S,  independently  of  the  barriers;  for 
this  statement  holds  of  each  of  the  factors 

«r(C,7),     ^(0,      6(^  +  ^11.,,),     <Pr*^\ 

And,  if  f  be  replaced  by  £n,  the  square  of  the  quotient  of  the  two  sides  of  the 
equation  becomes  (cf.  §  175,  Chap.  X.)  multiplied  by  the  factor 


'    7»?  +  «»         ' 

which  is  equal  to  unity.     Nowf  a  function  of  £  which  is  unaltered  by  the 
substitutions  of  the  group,  and  is  uniform  within  the  region  8,  and  has  no 

*  At  the  analogues  of  f  =  oo  neither  w  (f,  7)  nor  I/  \j/  (f  )  becomes  infinite. 

t  If  U+iV  be  the  function,  the  integral  \UdV,  taken  round  the  2p  fundamental  circles  is 
expressible  as  a  surface  integral  over  S  whose  elements  are  positive  or  zero.  In  the  case 
considered  the  former  integral  vanishes. 


238]  INTRODUCTION    OF   AN    ASSOCIATED    FUNCTION    X  (f,  7).  367 

infinities,  must,  like  a  rational  function  on  a  Riemann  surface,  bo  a  constant. 
Since  the  square  root  of  a  constant  is  also  a  constant  the  proof  of  the  equation 
is  complete. 

From  it  we  infer  (i)  that 

*  (£»)/*  (0  -  (-  1>""+A'1  (7H?+  «»)  (-  l)*», 

and  (ii)  that  the  values  of  \fr  (£)  on  the  two  sides  of  a  barrier  have  a  quotient 
of  the  form  (-!/».  The  constant  factor  to  be  attached  to  i/r(£)  may  be 
chosen  so  that  .4  =  1.  P'or  this  it  is  sufficient  to  take  for  the  integral  v  the 
expression 


where  ®i  (u)  =  d®  (u)/dUi.  Then  (cf.  §  188,  p.  281)  the  right-hand  side, 
when  f  is  near  to  7,  is  equal  to  A  (£-  7)  +  ...,  while  the  left-hand  side  has 
the  value  (£  —  7)  -f  ____ 

238.  The  developments  of  an  equation  analogous  to  that  just  obtained, 
which  will  be  given  in  Chap.  XIV.  in  connection  with  the  functions  there 
discussed,  render  it  unnecessary  for  us  to  pursue  the  matter  further  here. 
The  following  forms  an  interesting  example  of  theta  functions,  of  another  kind. 

Suppose  that  the  quantities  ^,  .  .  .  ,  pp  are  small  enough  to  ensure  (cf.  §  226) 
the  convergence  of  the  series 


wherein  p,  denotes  an  arbitrary  place  within  the  region  S,  and  i  denotes  a 
summation  extending  to  every  substitution  of  the  group.  It  will  appear  that 
this  function  is  definite  in  all  cases  in  which  the  function  «r  (£,  /*)  is  definite. 
The  function  is  immediately  seen  to  verify  the  equations 


and 


where  r  denotes  the  substitution  inverse  to  that  denoted  by  i.     Thus 

X  (£  M)  =  -  X  fa,  f ). 

The   function    has   one  pole  in  the  region  S,  namely  at  p,  and  no  other 
infinities,  and  if  the  series  be  uniformly  convergent  near  f  =  oo  ,  as  we  assume, 


368  PROPERTIES   OF   THE    FUNCTION    X  (£  7).  [238 

the  function  vanishes  to  the  first  order  at  £  =  oc  .     The  excess  of  the  number 
of  its  zeros  over  the  number  of  its  poles  in  8,  which  is  given  by 

i     »  ftx' (£»,/*)    *•'(£, 


where  the  dash  denotes  a  differentiation  in  regard  to  f ,  and  the  integrals  are 
taken  counter-clockwise  round  the  circles  C\r ,  ...,  Cp',  namely  by 


— .  2  I 


is  equal  to  p.  Thus  the  function  has  p  zeros  in  $  other  than  £  =  oo  ;  denote 
these  by  fa,  ...,  JJ,P.  Within  any  region  S-n$  the  function  has  the  analogue  of 
fj,  for  a  pole,  and  the  analogues  of  fa,  ...,  JJ,P  for  zeros;  it  does  not  vanish  at 
the  analogue  of  £  =  oc  .  This  result  may  be  verified  also  by  investigating 
similarly  the  excess  of  the  number  of  zeros  over  the  number  of  poles  in  any 
such  region  ;  the  result  is  found  to  be  p  —  1. 

Consider  the  ratio 


where  v  is  any  linear  function  of  th  ,  ...,.tiu  ;  let  £\,  ...,  ^2p_2  denote  the 
zeros  of  dv.  Then  /(£)  is  uniform  within  the  region  8,  and  is  unaltered  by 
the  substitutions  of  the  group.  It  has  poles  fj?,  £,  ...,  £2p-2,  and  no  other 
infinities  in  S,  and  has  zeros  fa2,  ...,  fip2,  the  square  of  a  symbol  being  written 
to  denote  a  zero  or  pole  of  the  second  order.  Thus  we  have,  precisely  as  for 
the  case  of  rational  functions  on  a  Riemann  surface, 


or  (§179,  p.  256), 

(p2,  £i,  •••>  (V-a)=  (y"a2>  •••,  /V)> 

and  therefore,  if  mlt  ...,  mp  denote  the  points  in  S,  derivable  from  //,  (§  236), 
such  that  ®  (/'  M  -  /"  '"'  -  ......  -  /"  '  mp)  vanishes  in   f  =  x,  ,  .  .  .  ,  £  =  xp,  we 

have  (§  182,  p.  265). 

(fa2,  ...,  ftp*)  =  (mi2,  ...,  mp2). 

When  the  barriers  are  drawn,  let 

v»"'"'+  ......  •\-vymp  =  ^(ki  +  klfT2i  !  +  ......  +  kpTi>p),  (i=l,  2,  ...,p), 

klt  ...,  kp,  ki,  ...,  kp  being  integers. 

Now  consider  the  product  X(£,  jj,)  •&  (£,  p,}.  It  has  no  poles,  in  8,  and  its 
zeros  are  fa,  ...,  fj,p.  It  is  an  uniform  function  of  £  and,  subjected  to  one  of 
the  fundamental  substitutions  of  the  group  it  takes  the  factor 


238]  EXPRESSION   BY  THETA   FUNCTIONS.  369 

Hence  the  function 


wherein  &'/'M  denotes  Ar/t^H-  ......  +  V4'*  and  n  denotes  the  j9  quantities 

&i  +  &/T";,  j  +  ......  +kpTiip,  has,  within  S,  no  zeros  or  poles,  and  is  such  that, 

for  a  fundamental  substitution, 


(cf.  §  175,  Chap.  X.);  thus,  as  in  the  previous  article,  F(%)  is  a  constant 
thus,  also,  gn  +  hn  —  kn  is  an  even  integer,  =  2Hn,  say,  and  we  have 


where  P  denotes  the  p  quantities  #  +  ^  +  k^Ti>  ,  +  ......  +  kp'ri>pt  and  A  is 

independent  of  $  But,  if  f  describe  the  circumference  Cn,  the  left-hand  side 
is  unchanged,  and  the  right-hand  side  obtains  the  factor  «-"•'*'»  Thus  the 
integers  &/,  ...,kp  are  all  even  ;  put  kr'  =  2Hr';  then,  as 


where  the  notation  is  that  of  §  175,  Chap.  X.,  we  have 


wherein  5  is  independent  of  £  and  therefore,  since  the  interchange  of  £  /* 
leaves  both  sides  unaltered,  B  is  also  independent  of  /j,.  The  value  of  5  may 
be  expressed  by  putting  £=/*;  thence  we  obtain,  finally, 


This  equation  may  be  regarded  as  equivalent  to  2^  equations.  For  if  in 
one  of  the  p  fundamental  substitutions  $>£=(«,-£  +  &)/(7r£+  S,),  we  consider 
the  signs  of  o^,  &.,  7r,  gr  all  reversed,  the  function  X(£  /A),  which  involves  the 
first  powers  of  these  quantities,  will  take  a  different  value.  The  function 
•a  (f,  /*),  the  p  fundamental  circles,  and  the  integrals  /'  M  and  their  periods 
rn,m,  and  therefore  the  integers  g1}  ...,  gp,  will  remain  unchanged,  if  the 
barriers  remain  unaltered.  But  the  integer  hr  will  be  increased  by  unity. 

If,  on  the  other  hand,  the  coefficients  a,  /3,  7,  B  remaining  unaltered, 
one  of  the  barriers  be  drawn  differently,  the  left-hand  side  of  the  equation 
remains  unaltered;  on  the  right-hand  one  of  hlt  ...,  hp  will  be  increased  by 
an  integer,  say,  for  example,  hr  increased  by  unity,  and  therefore  each  of 
Ti.r,  •••>  fp,r  also  increased  by  unity.  Putting  u  for  v^^-^g-^h,  and 
B-  24 


370  APPLICATION   TO   THE   ELLIPTIC   CASE.  [238 

neglecting  integral  increments  of  w,  the  exponent  of  the  general  term  of  the 
theta  series  is  increased,  save  for  integral  multiples  of  ZTTI,  by 

27Ti  (—  ^)  nr  +  t7rar2, 

which  is  an  even  multiple  of  iri,  so  that  the  general  term  is  unchanged. 
Ex.  i.     Prove  that  the  function  X  (f,  p.)  can  be  written  in  the  form 

where  the  sign  of  summation  refers  to  all  the  substitutions  of  the  group,  other  than 
the  identical  substitution,  with  the  condition  that  when  any  substitution  occurs  its  inverse 

must  not  occur,  and  {f ,  &  \  p,  /z,-}  denotes  — —  /    *       . 

o         r^t  '      ot         f^l 

Ex.  ii.     In  case  />  =  !,  where  the  fundamental  substitution  is 

(£'-  B)/(£-A)  =  p(£-B)/(£-A), 
putting  e2™* = (f  -  B)  /  (f  -  A ),  e2™  =  (fJ.-B)/(fji-A),  prove  that 


4  (  -  l)Ai 
(f,  M)  - 


and  hence 


When  A  =  0  this  becomes* 

4i'&)  sin  TTM  sin  irv  <r3  [2<o  (M  -  y)] 
o-  [2o>  (n  -  »)]  ' 


f)  sin2  TT  (u-v}~\ 
(it-^)  +  p2<      J' 


where  the  sigma  functions  are  formed  with  2w,  2ar  as  periods,  o>  being  an  arbitrary 
quantity.     Thus  (§  235,  Ex.) 


where  the  symbol  50  is  as  in  Halphen,  Fonct.  Ellip.  (Paris,  1886),  Vol.  I.  pp.  260,  252. 
This  agrees  with  the  general  result  ;  in  piitting  p^=eir'T  we  have  taken  g  —  \  ;  and,  as 
stated,  h  is  here  taken  zero. 

When  h  =  1  we  similarly  find 

...      .      4i'o)  sin  iru  sin  irv  <r3  [2o>  (u  —  v  +  £)]    -  2i)w  (?t  -  ti) 

*(»>  A1)111 '  /~T>     j\ ?~r      T^O    zr;    ^\i~  e  » 

(Jj  —  A)  ircr3  (<t>)        cr  \z,a)  (u  —  V) J 
and  hence 


also  in  agreement  with  the  general  formula.     In  these  formulae  Q(u]  denotes  the  series 

2e2iri«n+tirT»»  =  1  +  2?  COS  (2JTM)  -f-  2 J4  COS  (47Ttt)  +  2j9  COS  (67TM)  + , 

where  q  =  el7TT. 

*  Cf.  Halphen,  Fonct.  Ellip.  (Paris,  1886),  Vol.  i.  p.  422. 


238]  THE   PROBLEM   OF  THE   CONFORMAL  REPRESENTATION.  371 

Ex.  iii.     Denoting 


where  the  summations  include  all  substitutions  of  the  group  except  the  identical  sub 
stitution,  respectively  by  um>n,  v^n,  prove  that,  when  f  is  near  to  /*, 


Ex.  iv.  If  z,  s  be  two  single-valued  functions  of  £,  without  essential  singularities, 
which  are  unaltered  by  the  substitutions  of  the  group,  the  algebraic  *  relation  connecting 
z  and  s  may  be  associated  with  a  Eiemann  surface,  whereon  £  is  an  infinitely  valued 
function  ;  and  if  2,  s  be  properly  chosen,  any  single-valued  function  of  f  without  essential 
singularities,  which  is  unaltered  by  the  substitutions  of  the  group,  is  a  rational  function  on 
the  Riemann  surface.  But  if 


where  £'=  -~  ,  etc.,  we  immediately  find  that  the  value  Z=(af  +  #)/(yf  +8)  gives 

{Z,  *}  =  {£,  2}; 

//cfe\2 
therefore,  as  {£,  2},   =  -  {z,  £}  I  (  ^-  I   ,  is  a  single-  valued  function  of  f  without  essential 

/  V*i/ 
singularities,  and  is  unaltered  by  the  substitutions  of  the  group,  we  have 

{<T,  4  =  27(2,  s), 

where  /  denotes  a  rational  function.     Therefore,  if  Y  denote  an  arbitrary  function,  and 
P—  -  j^  log  (  F2  ^  J  ,  Y  and  £Y  are  the  solutions  of  the  equation 


and  if  Ir  be  chosen  so  that  F2  /^  is  a  rational  function  on  the  Riemann  surface,  the 
coefficients  in  this  equation  will  also  be  rational  functions.  Thus  for  instance  we  may 
take  for  Y  the  function  /y  ^,  in  which  case  P=0,  or  we  may  take  for  Y  the  function 
^  (0>  =  \/  j*  j-  »  considered  in  §  236,  which  is  uniform  on  the  f  plane  when  the  barriers 


are  drawn,  in  which  case  P=  -  -^  log  ~  ,  and  the  equation  takes  the  form  ^f  +  R.Y=0, 

where  R  is  a  rational  function,  or  again  we  may  take  for   Y  the  uniform  function  of 
C>  *  (f>  /*).  considered  in  §  238  f. 

*  Ex.  viii.  §  232. 

t  Cf.  Riemann,  Get.  Werke  (Leipzig,  1876),  p.  416,  p.  415;  Schottky,  Crelle,  LXXXIII.  (1877) 
p.  336  ff. 

24—2 


372  THE   HYPERELLIPTIC   CASE.  [238 

Ex.  v.  If,  as  in  Ex.  iv.,  we  suppose  a  Riemann  surface  constructed  such  that  to 
every  point  £  of  the  f  plane  there  corresponds  a  place  (z,  *)  of  the  Riemann  surface,  and 
in  particular  to  the  point  f  =£  there  corresponds  the  place  (x,  y\  and  if  R,  S  be  functions 
of  £  denned  by  the  expansions 


prove  that 


and  that  R,  8  are  rational  functions  of  x  and  y. 

Ex.  vi.  The  last  two  examples  suggest  a  problem  of  capital  importance  —  given  any 
Riemann  surface,  to  find  a  function  f,  which  will  effect  a  conformal  representation  of  the 
surface  to  such  a  f-region  as  that  here  discussed.  This  problem  may  be  regarded  as  that 
of  finding  a  suitable  form  for  the  rational  function  I  (z,  a).  The  reader  may  consult 
Schottky,  Crelle,  LXXXIII.  (1877),  p.  336,  and  Crelle,  ci.  (1887),  p.  268,  and  Poincare', 
A  eta  Mathem.atica,  iv.  (1884),  p.  224,  and  Bulletin  de  la  Soc.  Math,  de  France,  t.  XI.  (18  May, 
1883),  p.  112.  In  the  elliptic  case,  taking 


where  $>  denotes  Weierstrass's  function  with  1  and  T  as  periods,  it  is  easy  to  prove  that 
-jr.  and  f  */  -jj.  are  the  solutions  of  the  equation 


239.  There  is  one  case  of  the  theory  which  may  be  referred  to  in 
conclusion.  Take  p  circles  Cf1,  ...,  Cp,  exterior  to  one  another,  which  are  all 
cut  at  right  angles  by  another  circle  0  ;  take  a  further  circle  G  cutting  this 
orthogonal  circle  0  at  right  angles;  invert  the  circles  C1}  C.2}  ...  in  regard  to 
C.  We  shall  obtain  p  circles  <7/,  C2',  ...,  Cp'  also  cutting  the  orthogonal 
circle  0  at  right  angles.  The  case  referred  to  is  that  in  which  the  circles 
C1}  O/,  ...,  Cp,  Cp  are  the  fundamental  circles  and  the  angles  Klt  ...,  KP  are 
all  zero,  so  that,  if  ^n  denote  one  of  the  p  fundamental  substitutions,  the 
corresponding  points  £,  S-n£  lie  on  a  circle  through  An  and  Bn.  We  may 
suppose  that  the  circles  (7a  ,  .  .  .  ,  Cp  are  all  interior  to  the  circle  C.  It  can  be 
shewn  by  elementary  geometry  that  An,  Bn  are  inverse  points  in  regard  to 
the  circle  C  as  well  as  in  regard  to  the  circle  Cn,  and  further  that  if  &>  denote 
the  process  of  inversion  in  regard  to  the  circle  C  and  wn  that  of  inversion  in 

regard  to  Cn,  the  fundamental  substitution  S-n  is  a>nw,  so  that  ufen<a  =  ST»  ,  or 
&)^7V  =  ^1&).  Hence  if  the  points  of  intersection  of  the  circles  0,  Cn  be 
called  an',  bn',  the  points  of  intersection  of  0,  Cn'  be  called  an,  bn,  and  the 
points  of  intersection  of  0,  C  be  called  a,  b,  it  may  be  shewn  without  much 
difficulty  that 


_     _ 

vr      = 


a,,  .  b..        ,          .^          a,  b        ,          T-,        ,  -,     c\  i      \ 

nn'  "  =  $  +  Qn,  vn'    =$  +  R,     (n,  r  =  l,2,...,p  ;  n+r), 


239]  THE    HYPERELLIPfIC   CASE.  373 

where  Pn>  r,  Qn,  R  are  integers,  and  the  integrations  are  along  the  perimeters 
of  the  several  circles.  Hence  it  follows  that  the  uniform  functions  of  £ 

2jj£  c       2n^'  c 
expressed  by  e    «•••  *>r>  e     «-  *  are  unaltered  by  the  substitutions  of  the  group. 

Denote  them,  respectively,  by  xr  (f)  and  x  (£).  Each  of  them  has  a  single 
pole  of  the  second  order,  and  a  single  zero  of  the  second  order,  and  therefore, 
as  in  the  case  of  rational  functions  on  a  hyperelliptic  Riemann  surface,  we 
have,  absorbing  a  constant  factor  in  xr  (£),  an  equation  of  the  form 

x  m-^O-^K) 
•~*(0-*(&rj' 

But  it  follows  also  that  the  function 


is  unaltered  by  the  substitutions  of  the  group.     Hence  we  have*,  writing 
y,  x  for  y  (£),  as  (£),  etc., 


if  -xx 


Thus  the  special  case  under  consideration  corresponds  to  a  hyperelliptic 
Riemann  surface;  and,  for  example,  the  equations  t£"'  6"=  1  +  Qn,  etc.,  cor 
respond  to  part  of  the  results  obtained  in  §  200,  Chap.  XI.  It  is  manifest 
that  the  theory  is  capable  of  great  development.  The  reader  may  consult 
Weber,  Gottinger  Nachrichten,  1886,  "Ein  Beitrag  zu  Poincare's  Theorie, 
u.  s.  w.  ,"  also,  Burnside,  Proc.  London  Math.  Soc.  xxm.  (1892),  p.  283,  and 
Poincare,  Acta  Math.  m.  p.  80  and  Acta  Math.  iv.  p.  294  (1884);  also 
Schottky,  Crelle,  cvi.  (1890),  p.  199.  For  the  general  theory  of  automorphic 
functions  references  are  given  by  Forsyth,  Theory  of  Functions  (1893), 
p.  619.  The  particular  case  considered  in  this  chapter  is  intended  only 
to  illustrate  general  ideas.  From  the  point  of  view  of  the  theory  of  this 
volume,  Chapter  XIV.  may  be  regarded  as  an  introduction  to  the  theory 
of  automorphic  functions  (cf.  Klein,  Math.  Annalen,  xxi.  (1883),  p.  141,  and 
Ritter,  Math.  Annalen,  XLIV.  (1894),  p.  261). 

*  The  function  x  here  employed  is  not  identical  in  case^  =  l  with  the  z  of  Ex.  vi.  §  238. 


[240 


CHAPTER    XIII. 
ON  RADICAL   FUNCTIONS. 

240.  THE  reader  is  already  familiar  with  the  fact  that  if  sn  u  represent 
the  ordinary  Jacobian  elliptic  function,  the  square  root  of  1  —  sn2  u  may  be 
treated  as  a  single-valued  function  of  u.  Such  a  property  is  possessed  by 
other  square  roots.  Thus  for  instance  we  have* 


v(l  —  sn  u)  (1  —  k  sn  u) 

l  -  2om  sin  ~  +  f*      l  -  2qm~*  sin        4-  g2"1-1 

Tir    -  tjr         \-rr  *** 

=  M  Sin  -.       (K  -  U)  II 


where  M  is  a  certain  constant,'  and,  as  usual,  q  =  e~wR'IK.  The  single- 
valuedness  of  the  function  V(l  —  sn  u)  (]  —  k  sn  u)  can  be  immediately  seen 
to  follow  from  the  fact  that  each  of  the  zeros  and  poles  of  the  function 
(1  —  sn  u)  (1  —  ksnu)  is  of  the  second  order.  It  is  manifest  that  we  can 
easily  construct  other  functions  having  the  same  property.  If  now  we  write 
u  =  ux>  a  and  consider  the  square  root  on  the  dissected  elliptic  Riemann 
surface,  we  shall  thereby  obtain  a  single-valued  function  of  the  place  x, 
whose  values  on  the  two  sides  of  either  period  loop  will  have  a  ratio, 
constant  along  that  loop,  which  is  equal  to  +  1. 

Ex.     Prove  that  the  function 


is  a  single-valued  function  of  it. 

Further  we  have,  in  Chapter  XI.,  in  dealing  with  the  hyperelliptic  case 
associated  with  an  equation  of  the  form 

y"-  =  (a;  -  Oj)  .  .  .  (x  -  a2p)  (x  -  c), 

*  Cf.  Cayley,  Elliptic  Functions  (1876),  Chap.  XI.  The  function  may  be  regarded  as  a 
doubly  periodic  function,  with  8K,  2iK'  as  its  fundamental  periods.  It  is  of  the  fourth  order, 
with  K,  5K,  K  +  iK',  5K+iK'  as  zeros,  and  iK',  2K  +  IK',  iK+iK',  6K+iK'  as  poles. 


242]  EXPRESSION    BY    RIEMANN    INTEGRALS.  375 


been  led  to  the  consideration  of  functions  of  the  form  V(c  —  x^)  ...  (c  —  xp), 
which  are  expressible  by  theta  functions  with  arguments  u,  =uxi>ai+  ...... 

+  U*P<  aP.  These  functions  are  not  only  single-  valued  functions  of  the 
arguments  u,  but,  when  the  Riemann  surface  is  dissected  in  the  ordinary 
way,  also  of  every  one  of  the  places  tK1}  ...  ,  scp.  In  fact  the  square  root  vc  —  x 
is  a  single-valued  function  of  the  place  x  because,  c  being  a  branch  place, 
x  —  c  vanishes  to  the  second  order  at  the  place,  and  the  point  at  infinity 
being  a  branch  place,  x  —  c  is  there  infinite  to  the  second  order.  The  values 
of  the  square  root  \/c  —  x  on  the  two  sides  of  any  period  loop  will  have  a 
ratio,  constant  along  that  loop,  which  is  equal  to  +  1. 

241.  More  generally  it  may  be  proved,  for  any  Riemann  surface,  that  if 
Z  be  a  rational  function  such  that  each  of  its  zeros  and  poles  is  of  the  mih 
order,  the  mth  root,  \/Z,  is  a  single-valued  function  of  position  on  the 
dissected  surface,  with  factors  at  the  period  loops  which  are  wth  roots  of 
unity.  And  it  is  easy  to  prove  this  in  another  way  by  obtaining  an  ex 
pression  for  such  a  function.  For  let  alt  ...,  ar  be  the  distinct  poles  of  Z,  and 

fii,  ...,  @r  its  distinct  zeros,  so  that  the  function  is  of  order  mr.     Let  Hz\  *  be 

the  normal  elementary  integral  of  the  third  kind  and  Vi'a,  ...,  Vf  the  normal 
integrals  of  the  first  kind.  Then  when  the  paths  are  restricted  not  to  cross 
the  period  loops  we  have*  equations 


kpfri>p, 


wherein  klt  ...,  kp,  &/,  . . . ,  kp'  are  certain  integers  independent  of  i.     Hence 
the  expression 

m  [Hx>  a    A-          4-  nx>  a    1-2    'I- '  x>  a  -  -2    -i-  '  x>  a 

e  0u«l  Pr>  ar  P    P       , 

wherein  a  is  an  arbitrary  fixed  place,  represents  the  rational  function  Z,  save 
for  an  arbitrary  constant ;  and  we  have 


,x,a 


,  ,.x,  a 

+  ......  +H  ~— 


'=Ae 

where  A  is  a  certain  constant.  This  expression  defines  \/Z  on  the  dissected 
surface  as  a  single-valued  function  of  position.  More  accurately  it  defines 
one  branch  of  \/Z,  the  other  m-  1  branches  being  obtained  by  multiplying 
A  by  wth  roots  of  unity.  So  defined,  the  function  V Z  is  affected,  at  the 

-—  K 

period  loop  «,-,  with  a  factor  e  m  ',  and,  at  the  period  loop  «/,  with  the 
factor  em  '. 

242.     We  have,  in  chapters  X.,  XL,  been  concerned  with  other  functions, 
namely  the  theta  functions  which  also  have  the  property  of  being  single- 

*  Chap.  VIII.  §  155. 


376  EXPRESSION    BY   THETA    FUNCTIONS.  [242 

valued  on  the  dissected  Riemann  surface,  but  affected  with  a  factor  for  each 
period  loop.  They  are  also  simpler  than  rational  functions,  in  that  they  do 
not  possess  poles.  It  is  therefore  of  interest  to  express  such  functions  as 
\/ Z  by  means  of  theta  functions ;  and  the  expression  has  an  importance 
arising  from  the  fact  that  the  theory  of  the  theta  functions  may  be  established 
independently  of  the  theory  of  the  algebraic  integrals.  To  explain  this 
mode  of  representation  consider  the  quotient 

-/;  0 


U1 .      D\  ' 

-  * ;  ft) 

where  the  numerator  and  denominator  contain  the  same  number  of  factors, 
^  (a,  q)  denotes  the  function  (Chap.  X.  §  189)  given  by 

(n+g')2 


q,  r,  ...,  Q,  R,  ...  denote  any  characteristics,  and  e,f....,E,F,...  denote  any 
arguments. 

Then  by  the  formula  (§  190) 

£  (u  +  flj,  ;  q)  =  &M  <«>+2*W-J/'<?)  ^  (M  ;  q)t 
where  M,  M'  denote  integers,  we  have  ty  (u,  +  H  „)  fty  (u)  =  e'\  where  L  is 

\M(u-e)  +  \Jl(u-f)  +  ......  -\M(u-E)-\JI(u-F)-  ...... 

+  2iriM(q'  +  r'+  ......  -  Q'  -  R'  -...)-  2iriMf(q  +  r+  ......  -Q-R-...}, 

namely,  is 

......  -Q'-R'-  ...) 

q  +  r  +  ......  -Q-R-...). 

Thus  if 

ei+fi+  ......  =Et  +  Fi+  ......  , 

and 

ff*  +rt  +  ......  -(Qi  +Ri+...)  =  ~Ki,     (i  =  l,2,  ...,p), 

I  IV 

qi+r^+  ......  -(Q/  +  JR/+...)  =  -^/, 

772* 

where  Kiy  Kl  are  integers  and  m  is  an  integer,  it  follows,  for  integral  values 
of  M,  M',  that 


If  now  we  take  b  =  iirr,  as  in  §  192,  and  put  ux<a  for  u,  *$(u—e;  q) 
becomes  a  single-  valued  function  of  x  whose  zeros  are  (§§  190  (L),  179)  the 
places  #j,  .  ..,  xp,  given  by 


244]  COMPARISON   WITH   RATIONAL   FUNCTIONS.  377 

where  alt  ...,  ap  are  p  places  determined  from  the  place  a,  just  as  in  §  179 
the  places  m1  ,  ...,  mp  were  determined  from  the  place  m  ;  hence,  in  this  case, 
i/r  (w)  is  the  wth  root  of  a  rational  function,  having  for  zeros  places 


each  m  times  repeated,  and  for  poles  places 

Y  Y      7  7 

.AH  ...,  -Ap,  oif  ...,  &p,  ..., 

each  m  times  repeated,  these  places  being  subject  only  to  the  conditions 
expressed  by  the  equations 

A",      (A). 


II  v 


In  this  representation  we  have  obtained  a  function  of  which  the  number 
of  m  times  repeated  zeros  is  a  multiple  of  p,  and  also  the  number  of  m  times 
repeated  poles  is  a  multiple  of  p.  It  is  easy  however  to  remove  this  restric 
tion  by  supposing  a  certain  number  of  the  places  x1}  ...,  xp,  zlt  ...,  zp  to 
coincide  with  places  of  the  set  X1}  ...,  Xp,  Z1}  ...,  Zp, 

243.  A  rational  function  on  the  Riemann  surface  is  characterised  by  the 
facts  that  it  is  a  single-valued  function  of  position,  such  that  itself  and  its 
inverse   have  no  infinities  but  poles,  which  has,  moreover,  the  same  value 
at  the  two  sides  of  any  period  loop.     The  functions  we  have  described  may 
clearly  be  regarded  as  generalisations  of  the  rational  functions,  the  one  new 
property  being  that  the  values  of  the  function  at  the  two  sides  of  any  period 
loop  have  a  ratio,  constant  along  that  loop,  which  is  a  root  of  unity.     For 
these  functions  there  holds  a  theorem,  expressed  by  the  equations  (A)  above, 
which  may  be  regarded  as  a  generalisation  of  Abel's  theorem  for  integrals 
of  the  first  kind ;    and,  when  the  poles  of  such  a  function  are  given,  the 
number  of  zeros  that  can  be  arbitrarily  assigned  is  the  same  as  for  a  rational 
function  having  the  same  poles,  being  in  general  all  but  p  of  them;    this 
follows   from   the   theory   of    the    solution    of    Jacobi's    inversion   problem 
(Chap.  IX. ;  cf.  also  §§  37,  93).     It  will  be  seen  in  the  course  of  the  following 
chapter  that  we  can  also  consider  functions  of  a  still  more  general  kind, 
having  constant  factors  at  the  period  loops  which  are  not  roots  of  unity,  and 
possessing,  beside  poles,  also  essential  singularities;  such  functions  may  be 
called  factorial  functions.     The  particular  functions  so  far  considered  may  be 
called  radical  functions ;  it  is  proper  to  consider  them  first,  in  some  detail,  on 
account   of  their   geometrical    interpretation   and   because   they   furnish   a 
convenient  method  of  expressing  the  solution  of  several  problems  connected 
with  Jacobi's  inversion  problem. 

244.  The  most  important  of  the  radical  functions  are  those  which  are 
square  roots  of  rational  functions,  and  in  view  of  the  general  theory  developed 
in  the  next  chapter  it  will  be  sufficient  to  confine  ourselves  to  these  functions. 

s 


378  ASSOCIATION   OF   A   RADICAL   FUNCTION  [244 

In  dealing  with  these  we  shall  adopt  the  invariant  representation  by  means 
of  (^-polynomials,  which  has  already  been  described*.  An  integral  polynomial 
of  the  rth  degree  in  the  p  fundamental  (^-polynomials,  <f>1}  ...,  <j>p,  will  be 
denoted  by  3>{n  ,  or  "SP"'*,  when  its  2r(p  —  1)  zeros  are  subject  to  no  condition. 
When  all  the  zeros  are  of  the  second  order,  and  fall  therefore,  in  general,  at 
r(p—  1)  distinct  places,  the  polynomial  will  be  denoted  by  X(r>  or  Y(r)  ;  we 
havef  already  been  concerned  with  such  polynomials,  Xw  ,  of  the  first  degree 
in  </>!,  ...,  <j>p. 

It  is  to  be  shewn  now  that  the  square  root  VJT(r)  can  properly  be  associated 
with  a  certain  characteristic  of  2p  half-integers;  and  for  this  purpose  it  is 
convenient  to  utilise  the  places  m1}  ...,  mp,  arising  from  an  arbitrary  place  m, 
which  have  already  |  occurred  in  the  theory  of  the  theta  functions.  These 
places  are§  such  that  if  a  non-adjoint  polynomial,  A,  of  grade  p,  be  taken  to 
vanish  to  the  second  order  at  m,  there  is  an  adjoint  polynomial,  ty,  of  grade 
(11  —  l)cr+  n  —  3  +  fi,  vanishing  in  the  remaining  n/j,  —  2  zeros  of  A,  whose 
other  zeros  consist  of  the  places  ml}  ...,mp,  each  repeated.  Take  now  any 
(^-polynomial,  <f>0>  vanishing  to  the  first  order  at  m,  and  let  its  other  zeros  be 
Al}  ...,  A^p-s",  and  take  a  polynomial  <&(3)  vanishing  to  the  second  order  in 
each  of  A1}  ...,  A2p_2;  then  <E>(3>  will||  contain  5(^-1)  -  2(2p  -  3),  =  p+l, 
linearly  independent  terms,  and  will  have  6  (p  —  1)  —  2  (2p  —  3),  =  2p,  further 
zeros.  Let  X(l)  be  any  ^-polynomial  of  which  all  the  zeros  are  of  the  second 
order.  Consider  the  most  general  rational  function,  of  order  2p,  whose  poles 
consist  of  the  place  m,  this  being  a  pole  of  the  second  order,  and  of  the  zeros 
of  Xw.  This  function  will  contain  2p—p  +  1,  =p  +  1,  linearly  independent 
terms  and  can  be  expressed  in  either  of  the  forms  <!>(3'/</>02.X(1),  -v|r/A^(1),  where 
•»Jr  is  any  polynomial  of  grade  (n  —  1)  cr  +  n  —  3  +  p  which  vanishes  in  the 
up  —  2  zeros  of  A  other  than  m.  Since  now  11  -v/r  can  be  chosen,  =  i|r,  so  that 
the  zeros  of  this  function  are  the  places  m1}  ...,mp,  each  repeated,  it  follows 
that  <E>(3)  can  be  equally  chosen  so  that  this  is  the  case.  So  chosen  it  may  be 
denoted  by  X(s>.  Thus  the  places  m^,  ...,mp  arise  as  the  remaining  zeros  of  a 
form  X{S}  (with  3(p  —  1),  =p  +2p  —  3,  zeros,  each  of  the  second  order),  whose 
other  2p  —  3  separate  zeros  are  zeros  of  an  arbitrary  (^-polynomial,  <)>0,  which 
vanishes  once  at  the  place  m. 

If  now  ?i:,  ...,  ?z_p_i  be  the  places  which,  repeated,  are  the  zeros  of  Xw,  it 
follows,  since  m,  nl}  ...,  ?ip_i,  each  repeated,  are  the  poles,  and  m1}  ...,mp, 
each  repeated,  are  the  zeros  of  a  rational  function,  X{3}/<f>02Xw  ,  that,  upon  the 
dissected  surface,  we  have 


*  Chap.  VI.  §  110  ff.,  and  the  references  there  given,  and  Klein,  Math.  Annal.  xxxvi.  p.  38. 

t  Chap.  X.  §  188,  p.  281.  I  Chap.  X.  §  179. 

§  Chap.  X.  §  183,  Chap.  VI.  §  92,  Ex.  ix. 

||  Chap.  VI.  §  111.  H  Chap.  X.  §  183. 


245]  WITH   A   HALF-INTEGER   CHARACTERISTIC.  379 

where  ki,  ...,  kp,  &/,  ...,  kp'  are  certain  integers.  Hence,  as  in  §  241,  it 
immediately  follows  that  the  rational  function  Xi3)/(f)Q-X{11,  save  for  a  constant 
factor,  is  the  square  of  the  function 


and  therefore  that  the  expression  ^X(3>/<f)0*/X(v  may  be  regarded  as  a  single- 
valued  function  on  the  dissected  Riemann  surface,  whose  values  on  the  two 
sides  of  any  period  loop  have  a  ratio  constant  along  that  loop.  These  constant 
ratios  are  equal  to  enik>-'  and  e~n!kr  for  the  rth  loop  of  the  first  and  second  kind 
respectively.  When  the  places  ml}  ...,  mp  are  regarded  as  given,  these 
equations  associate  with  the  form  VZ  (1)  a  definite  characteristic 


T  «V>  •  •  •  j  T"j»  9*1  t  •  •  •  >  2  "'P  ' 

Also,  if  F|3>  be  any  polynomial  which,  beside  vanishing  to  the  second 
order  in  Alt  ...,  A^p_3,  vanishes  to  the  second  order  in  places  m/,  ...,  mp  , 
Y(3]jX(3]  is  a  rational  function,  and  we  have  equations  of  the  form 


where  \lt  ...,  \p  are  integers,  A  is  a  constant,  and  the  paths  of  integration 
are  limited  to  the  dissected  Riemann  surface.  These  equations  associate 
VF(3)  with  the  characteristic  \1}  ...,  \,  X/,  ., 


And,  as  in  §  184,  Chap.  X.,  we  infer  that  every  odd  characteristic  is 
associated  with  a  polynomial*  Xw,  and  every  even  characteristic  with  a 
polynomial  F(3),  which  has  Aly  ...,  A^^  for  zeros  of  the  second  order;  and  it 
may  happen  that  the  polynomial  F(3)  corresponding  to  an  even  characteristic 
has  the  form  </>02F(1),  in  which  case  the  places  w/,  ...,  mp  consist  of  the  place 
m  and  the  zeros  of  a  form  F(1)  . 

245.  Let  now  X(*v+1)  be  any  polynomial  whose  zeros  consist  of 
(2i>  +  1)  (p  —  1)  places,  zlt^,  ...,  each  repeated  ;  let  </>„  be  as  before,  vanishing 
in  m,  Alt  ...,  ^4.2p_3)  and  X(3}  be  as  before,  vanishing  to  the  second  order  in 
Al}  ...,  Azp-3,  Wj,  ...,  wp.  Then  if  4>(I>)  be  any  ^-polynomial  whose  zeros 
are  CL,  C2)  ...,  the  function 


*  Or  in   particular  cases  with  a  lot  of  such  polynomials,  giving  rise  to  coresidual   sets  of 
places. 


380  GENERAL  THEORY  OF  THE  EXPRESSION  [245 

is  a  rational  function  of  order  2  (2z/  -f  1)  (p  —  1)  +  2,  whose  zeros  are  m,  z1 ,  z.2,  . . . , 
and  whose  poles  consist  of  the  places  7?^,  ...,  mp,  and  the  zeros  of  <£'"),  each 
repeated.  Hence  as  before  <f>0*/X(Zv+v/<&w  V5^>  is  a  single-valued  function  on 
the  dissected  surface,  and  the  form  \/X(Zv+l)  is  associated  with  a  characteristic 
^ql} ...,  ^qp,  \q{ ,  ...,  ^qp ,  such  that,  on  the  dissected  surface, 


ZP, 


(i  =  l,  2,  .....p); 

and  if,  instead  of  4>(v),  we  had  used  any  other  polynomial  ^{v>,  the  character 
istic  could,  by  Abel's  theorem,  only  be  affected  by  the  addition  of  integers. 
Suppose  now  that  Y(^+l}  is  another  polynomial,  and  take  a  polynomial 


then  if  the  characteristic  of  the  function     0V7<^+1>^w\/X^  differ  from  that 


of  (/>0v  X^+v  !<&(")  \/  X(z)  only  by  integers,  we  have  when  xl}  #2,  •  ••  denote  the 


zeros  of  *Y^+l\  and  d1}  d2,  ...  denote  the  zeros  of  M^),  the  equation 

xi  i  m\  Xp,m,t         Xn+i.d,  ,  ,  , 

P  P         ' 


MP'TPI 


where  Mlt  ...,  Mp>  M^  ,  ...,  Mp'  denote  integers;  by  adding  this  to  the  last 
equation  we  infer*  that  ^^X^^T^^I^^  V(ti)  X®  is  a  rational  function. 
Hence  "f1,  since  there  exists  a  rational  function  of  the  form  (f)^X^/X^3),  we 
infer,  when  *JX(2v+1\  ^Y^+1]  have  characteristics  differing  only  by  integers, 
there  exists  a  form  <J><'X+|/+1>  whose  zeros  are  the  separate  zeros  of  \l  X  (2"+1)  and 
),  and  we  have 


Hence,  all  possible  forms  F'2^*1',  with  the  same  value  of  /i,  whose 
characteristics,  save  for  integers,  are  the  same,  are  expressible  in  the  form 
<j>  (,*+„+!)  /VZ(2"+1>,  where  <E><>*+*+1>  is  a  polynomial  of  the  degree  indicated, 
which  vanishes  once  in  the  zeros  of  */X(2v+1}.  All  such  forms  -v/F^+D  are 
therefore  expressible  by  such  equations  as 


where  V  F](2'x+1),  ...,  v  F"^^^  are  special  polynomials,  and  X,,  ...,  X2M(p_1)  are 
constants.  The  assignation  of  2/j,  (p  —  1)  —  1,  =  (2/i  +  1)  (p  —  1)  —  p,  zeros  of 
will  determine  the  constants  X1;  ...,  X^^-D,  and  therefore  determine 


the  remaining  p  zeros.    When  p  =  0  there  may  be  a  reduction  in  the  number 
of  zeros  determined  by  the  others. 

It  follows  also  that  the  zeros  of  any  form  VF(2'A+1)  are  the  remaining  zeros 
of  a  polynomial  ^>^+2)  which  vanishes  in  the  zeros  of  a  form  x/Z13'  having 


Chap.  VIII.  §  158.  t  Chap.  VI.  §  112. 


246]  OF   RADICAL   FUNCTIONS.  381 

the  same  characteristic  as  \/F(2'1+1),  or  a  characteristic  differing  from  that  of 
integers.     When  the  characteristic  of  ^/X®   is  odd,  and 
,  we  may  take  <J><"+2>  to  be  of  the  form 


It  can  be  similarly  shewn  that  if  Xw  be  a  polynomial  of  even  degree,  2/j,, 
in  the  fundamental  0-polynomials,  of  which  all  the  zeros  are  of  the  second 
order,  and  <f>w  be  any  polynomial  of  degree  /*,  the  quotient  \/Xw/<&w  may 
be  interpreted  as  a  single-valued  function  on  the  dissected  surface,  and  the 


form  vX(w  may  be  associated  with  a  certain  characteristic  of  half-integers. 


Further  the  zeros  of  ^Xw  are  the  remaining  zeros  of  a  form  c£<>*+1)  which 
vanishes  in  the  zeros  of  a  form  VjT<->  of  the  same*  characteristic  as  VZ"  <*'*>. 


Also  if  */Xm,  \/F(1)   be  two  forms  whose  (odd)  characteristics  have  a  sum 


differing  from  the  characteristic  of  VZ*2'  by  integers,  the  ratio 
is  a  rational  function  ;  and  if  we  determine  (p  —  1)  pairs  of  odd  characteristics, 
such  that  the  sum  of  each  pair  is,  save  for  integers,  equal  to  the  character 
istic  of  \/Z<2',  and  V5V1',  VF^,  VZ^,  VTy1"',  ...,  represent  the  corresponding 
forms,  there  exists  an  equation  of  the  form 


As  a  matter  of  fact  every  characteristic,  except  the  zero  characteristic,  can, 
save  for  integers,  be  written  as  the  sum  of  two  odd  characteristics  in 
2p_2  (2p-i_  1)  ways. 

246.  In  illustration  of  these  principles  we  consider  briefly  the  geometrical 
theory  of  a  general  plane  quartic  curve  for  which  p  =  3.  We  may  suppose 
the  equation  expressed  homogeneously  by  the  coordinates  xl,  x.2,  x3  and  take 
the  fundamental  0-polynomials  to  be  cf>l  =  x1,  (f>.2=x2,  <f>s  =  cc3.  There  are 
then  2^-1(2^-l)  =  28  double  tangents,  X^,  of  fixed  position.  There  are 
2^,  =  64,  systems  of  cubic  curves,  X(3),  each  touching  in  six  points.  Of  these 
six  points  of  contact  of  a  cubic,  X(3},  of  prescribed  characteristic,  three  may  be 
arbitrarily  taken  ;  and  we  have  in  fact 


=  x,   J^)  +  x,  Vz/>  +  A,  VIv5*  + 


where  \lt  A,,,  A3,  A4  are  constants,  and  ^/X^,  VJt2<3>,  ...,  are  special  forms  of 
the  assigned  characteristic.  The  points  of  contact  of  all  cubics  X(3}  of  given 
odd  characteristic  are  obtainable  by  drawing  variable  conies  through  the 
points  of  contact  of  the  double  tangent,  D,  associated  with  that  odd 
characteristic.  Let  no  be  a  certain  one  of  these  conies  and  let  X0  denote  the 
corresponding  contact-cubic  ;  then  the  rational  function  X0D/fl02  has,  clearly, 
no  poles,  and  must  be  a  constant,  and  therefore,  absorbing  the  constant,  we 
infer  that  the  equation  of  the  fundamental  quartic  can  be  written 


Or  a  characteristic  differing  from  that  of  vjP     by  integers. 


382  THE   CASE   OF   THE   BITANGENTS  [246 

Three  of  the  conies  through  the  points  of  contact  of  D  are  xj)  =  0,  x2D  =  0, 
x3D=Q;  the  corresponding  forms  of  JT(3)  are  x^D,  x.22D,  xjD.  Hence  all 
contact  cubics  of  the  same  characteristic  as  VZ)  are  included  in  the  formula 


v  z0, 


or 


where  P  =  X,^  +  \^cz  +  X3#3,  X1;  Xa,  X3  being  constants  ;  the  conic  through  the 
points  of  contact  of  D  which  passes  through  the  points  of  contact  of  X®  is 
given  by  H  =  2  \/J9X<3',  or  H  =  2PD  +  H0  ;  and  the  fundamental  quartic  can 
equally  be  written 

4,x®D  -  n2  =  4  (XQ  +  n0p  +  DP*)  £  -  (n0  +  ZPD?  =  o. 

If  then  we  introduce  space  coordinates  X,  Y,  Z,  T  given  by 
X=x1,  Y=x     Z=x     T= 


so  that  the  general  form  of  VJT(3)  with  the  same  characteristic  as  VZ)  is  given 

by 

VZ<3>  =  Vi)  (X1Z  +  X27  +  X3^-  T), 
we  have 

4Z0  (Z,  F,  Z)  D  (Z,  F,  £)  =  W  (X,  7,  Z), 

2TD  (X,  Y,  Z)  +  A,  (X,  Y,  Z)  =  0, 

where  X0  (X,  Y,  Z)  is  the  result  of  substituting  in  X0,  for  aclt  oc2,  x3, 
respectively  X,  Y,  Z,  etc.  ;  by  these  equations  the  fundamental  quartic  is 
related  to  a  curve  of  the  sixth  order  in  space  of  three  dimensions,  given 
by  the  intersection  of  the  quadric  surface 


and  the  quartic  cone 

4Z0  (X,  Y,  Z)  D  (X,  F,  Z)  =  Cl*  (X,  Y,  Z)  • 
the  curve  lies  also  on  the  cubic  surface 

T*D  (X,  Y,  Z)  +  mo  (X,  Y,  Z)  +  X0  (X,  Y,  Z)  =  0, 
which  can  also  be  written 

(T-P)*D(X,  7,Z)  +  (T-P)Q(X,  Y,Z)  +  X®(X,  Y,  Z)  =  0, 


where  P  denotes  \,X  +  X2F+  \3Z,  n  =  2PD  +  flc,  and  X®  =  DP2  +  H0P  +  X0, 
as  above. 

It  can  be  immediately  shewn  (i)  that  the  enveloping  cone  of  the  cubic 
surface  just  obtained,  whose  vertex  is  the  point  X  =  0  =  F=  Z,  is  the  quartic 
cone  whose  intersection  with  the  plane  T  =  0  gives  the  fundamental  quartic 
curve,  (ii)  that  the  tangent  plane  of  the  cubic  surface  at  the  point 


247]  OF   A    PLANE   QUARTIC    CURVE.  383 

X  =  0  =  Y  =  Z  is  the  plane  D  (X,  Y,  Z)  =  0,  (iii)  that  the  planes  joining 
the  point  X  =  0  =  F  =  Z  to  the  27  straight  lines  of  the  cubic  surface 
intersect  the  plane  T=0  in  the  27  double  tangents  of  the  fundamental 
quartic  other  than  Dt  (iv)  that  the  fundamental  quartic  curve  may  be 
considered  as  arising  by  the  intersection  of  an  arbitrary  plane  with  the 
quartic  cone  of  contact  which  can  be  drawn  to  an  arbitrary  cubic  surface 
from  an  arbitrary  point  of  the  surface. 

Thus  the  theory  of  the  bitangents  is  reducible  to  the  theory  of  the  right 
lines  lying  on  a  cubic  surface.  Further  development  must  be  sought  in  geo 
metrical  treatises.  Cf.  Geiser,  Math.  Annal.  Bd.  I.  p.  129,  Crelle  LXXII.  (1870); 
also  Frahm,  Math.  Annal.  vn.  and  Toeplitz,  Math.  Annal.  XL;  Salmon,  Higher 
Plane  Curves  (1879),  p.  231,  note  ;  Klein,  Math.  Annal.  xxxvi.  p.  51. 

247.  We  have  shewn  that  there  are  28  double  tangents  each  associated 
with  one  of  the  odd  characteristics  ;  the  association  depends  upon  the  mode 
of  dissection  of  the  fundamental  Riemann  surface.  We  have  stated  moreover 
(§  205,  Chap.  XL),  in  anticipation  of  a  result  which  is  to  be  proved  later,  that 
there  are  8  .  36  =  288  ways  in  which  all  possible  characteristics  can  be  repre 
sented  by  combinations  of  one,  two,  or  three  of  seven  fundamental  odd 
characteristics.  These  fundamental  characteristics  can  be  denoted  by  the 
numbers  1,  2,  3,  4,  5,  6,  7,  and  in  what  follows  we  shall,  for  the  sake  of 
definiteness,  suppose  them  to  be  either  the  characteristics  so  denoted  in  the 
table  given  §  205,  or  one  of  the  seven  sets  whose  letter  notation  is  given  at 
the  conclusion  of  §  205.  Thus  the  sum  of  these  seven  characteristics  is  the 
characteristic,  which,  save  for  integers,  has  all  its  elements  zero  ;  or,  as  we 
may  say,  the  sum  of  these  characteristics  is  zero. 

A  double  tangent  whose  characteristic  is  denoted  by  the  number  i  will  be 
represented  by  the  equation  m  =  0.  A  combination  of  two  numbers  also 
represents  an  odd  characteristic  (§  205,  Chap.  XL),  so  that  there  will  also  be 
21  double  tangents  whose  equations  are  of  such  forms  as  uitj  =  0.  The  three 
products  Vi^ttj,,  4/t%»,7,  *Ju3ul2  will  be  radical  forms,  such  as  have  been  denoted 
by  V3>,  each  with  the  characteristic  123.  Hence  if  suitable  numerical 
multipliers  be  absorbed  in  ul}  u3,  we  have  (§  245)  an  identity  of  the  forms 

vVw^  +  Vi*2w31  +  V-M.WU  =  0,     (u,u3l  +  u3u12  -  ulU23)2  =  4,u2u3u3^2  ; 

this  must  then  be  a  form  into  which  the  equation  of  the  fundamental  quartic 
curve  can  be  put.     Further,  each  of  the  six  forms 


has  the  same  characteristic,  denoted  by  the  symbol  1.  Thus,  if  suitable 
numerical  multipliers  be  absorbed  in  u2,  u4,  the  equation  of  the  quartic  can 
also  be  given  in  the  form 


384  THE    CASE    OF   THE   BITANGENTS  [247 

If  therefore 

/=  UaUsi  +  U3U12  —  WiW23>       <j)  -  U2u12  +  U^uu  —  U3U13, 

we  have 

(/-  0)  (/+  <#>)  =  4u2u12  (wsM,,  -  w,4w14). 

Now  if/-<£  were  divisible  by  u2,  and/+</>  divisible  by  ul2,  the  common 
point  of  the  tangents  u2  =  0,  u12  =  0  would  make  /=  0,  and  therefore  be  upon 
the  fundamental  quartic,  /2  =  4w2w3w31w12  ;  this  is  impossible  when  the  quartic 
is  perfectly  general.  Hence,  without  loss  of  generality,  we  may  take 

f—<f>  = 
2 


X  being  a  certain  constant,  and  therefore 

*u2u12,  =  u3uls  -  X  (u.2u3l  +  usu12  -  u-^ 


Therefore,  when  the  six  tangents  uly  u2,  u3,  u^,  uzl,  ulz  are  given,  the  tangents 
ut,  w]4  can  be  found  by  expressing  the  condition  that  the  right-hand  side 
should  be  a  product  of  linear  factors  ;  as  the  right-hand  is  a  quadric  function 
of  the  coordinates  this  will  lead  to  a  sextic  equation  in  X,  having  the  roots 
X  =  0,  X  =  oo  ;  if  the  other  roots  be  substituted  in  turn  on  the  right-hand,  we 
shall  obtain  in  turn  four  pairs  of  double  tangents  ;  these  are  in  fact  (u4,  Uu), 
(us,  u15),  (ue,  ULG),  (UT,  ul7).  We  use  the  equation  obtained  however  in  a 
different  way  ;  by  a  similar  proof  we  clearly  obtain  the  three  equations 

W4W14  =  U3U13  —  Xj  (U2U31  +  U3U12  —  l^U^}  +  X^WgWjj, 

u^u^  =  UiUn  -  X2  (u3u12  +  u^i^  -  u2u31)  +  X22M3W23,  (B) 

\s  (U^zs  +  U2U31  —  U3U12)  +  X32^  U31, 


and  hence 


from  this  we  infer  that  the  common  point  of  the  tangents  wlT  u4  either  lies  on 

11 

w23  or  on   X2u3  +  -2  =  Q;  as  the  fundamental  quartic  may  be  written  in  the 

A-3 


form  ^AU^UM  +  \/Bu2u^  +  VC^t^  =  0,  it  follows  that  if  ^,  M4,  u.23  intersect, 
they  intersect  on  the  quartic,  which  is  impossible.  Hence  w4  must  pass 

through  the  intersection  of  ^and  X2w3  +  -^  =  0  ;   now  we  may  assume  that 

X3 

the  tangents  uly  u2,  u3  are  not  concurrent,  since  else,  as  follows  from  the 
equation  Vw^  +  Vw2w31  +  *Ju3u12  =  0,  they  would  intersect  upon  the  quartic  ; 
thus  w4  may  be  expressed  linearly  by  u1}  u2,  u3,  and  we  may  put 


+  a2u2  +  asu3  =  a^  +    -x^Us  +~) 

X3X 


247]  OF   A   PLANE   QUARTIC   CURVE.  385 

and  so  obtain  X2=Aia3,  X3  =  1/^a.j,  hi  being  a  certain  constant;   then  the 
equation  under  consideration  becomes 


or 


/M24         7/34          ,  \  /^, 

U*  V7u      X~  ~    lW23J  =  Ml  I  XT  +  ^Wsi  "     /2 
so  that,  if  &!  denote  a  proper  constant, 


,     ^34  _   7  &1 

I       -v          -   Wl  "^S  7        Wl» 

A.3  fli 


ci3      &% 
We  can  similarly  obtain  the  equations 

-  k2u,  =  ^  +  ^-  h,u3i  (2  +  a 


where  /i2)  /<3,  Ar2,  A?3  are  proper  constants;  therefore,  as  u.a,  u3l,  ua  are  not 
concurrent  tangents,  since  else  they  would  intersect  on  the  fundamental 
quartic,  we  infer,  by  comparing  the  right-hand  sides  in  these  three  equations, 


and    hence,   k1  =  k.2  =  ks,   =  k,   say,   and    1  +  2^  +  a,2/*,2  =  0  or  hi  =  -  i 

a, 

7  1       I  1 

//,,  =  --   ,    *,-  --  . 

tt2  a:i 

Thus 

-fa«l=2»  +  ^!  +  ^> 

ttj       a.,      as 
or 

w.,8      ««31      7^], 

—  +-+—"  +  ^  («!  Wj  +  «2  u2  +  a3u3)  =  0.  (C) 

u-i        a2        t'3 

Further  we  obtained  the  equation 

"24^34  A?j 

_  +  _  =  /,1^__Wi; 

thus  we  have 


25 


386  THE   CASE   OF  THE   BITANGENTS  [247 

and  therefore,  as  Xj  =  --  -,  X3  =  --  -,  and  similarly  Xj  =  —  -,  we  have,  by 

ft]  (12  d3 

the  equation  (C), 

--  -uu  =  —  +  k  (a2u2  +  a3u3), 
ct/%          (LI 

Cvj  ^31  7     /  \ 

--  M24  =  --  1-  fc  (a3u3  +  aiWj), 

CL3  CL2 

2  12          7    /  \ 

^34  ^~  -     I    iG  \  ^1  ^1     I     ^2  ^2/' 

tti  CL3 

But  if  we  put 

u5=  b1u1  +  b2u2  +  b3it3,     ^£e  =  c1'M1  +  c2M2  +  c3w3,     U7=dlul+d2u2  +  d3u3, 

we  have  also  three  other  equations  such  as  (C),  differing  from  (C)  in  the 
substitution  respectively  of  the  coefficients  b1}  b.2)  b3  clf  c2,  C3  and  dlt  d2,  ds  in 
place  of  alt  a2,  a3,  and  of  three  constants,  say  I,  m,  n,  in  place  of  k.  As  the 
tangents  u5,  u6,  u7  are  not  concurrent  (for  the  fundamental  quartic  can  be 
written  in  a  form  v  usul5  +  *Ju6uls  +  ^u7u17  =  0)  we  may  use  these  three  last 
equations  to  determine  u23,  u3l,  u12  in  terms  of  w1}  w2,  us;  the  expressions 
obtained  must  satisfy  the  equation  (C).  Thus  there  exist,  with  suitable 
values  of  the  multipliers  A,  B,  C,  D,  the  six  equations 

A     B     C     D 


Dndl  =  0, 

/i        Ui          ]        C/i 

A     B     C     D 


+  Dnd2  =  0, 
ct%     02     c2     d2 

A     B     C     D 

-  +  j-  +  --  +  -j  =  0,  Aka3  +  Blb3  +  Cmc3  +  Dnd3  =  0. 

C13        03        C3        Cl3 

From  these  equations  the  ratios  of  the  constants  k,  I,  m,  n  are  determinable; 
suppose  the  values  obtained  to  be  written  pk',  pi',  pm',  pn',  where  p  is  undeter 
mined,  and  k',  I',  m,  n'  are  definite  ;  then,  if  we  put  a;  for  af  VK,  &  for 
biVl',  <yt  for  C;Vm',  Si  for  di^ln,  v^  for  u^/p,  vsl  for  ti3l/p,  and  v12  for  u12/p,  the 
equations  obtained  consist  of 

(i)     four  of  the  form 

Vos        VS1        V,o  //^(,, 

-+~  +  --+alul  +  a2u2  +  a3u3  =  0  (C  ) 

ai  a2  a3 

in  which  there  occur  in  turn  the  sets  of  coefficients  (alt  «2,  a3),  (y81}  ^2,  /93), 
(71.  72,  7s)>  (^i,  S2,  S3)  ;  from  any  three  of  these  v^,  v3l,  vl2  may  be  expressed  in 
terms  of  u1}  u2,  us; 

(ii)     four  sets  of  the  form 


where  v,4  =  uujp  ^k',  v^  =  u^/p  VF,  VM  =  u^/p  VF. 


247]  OF  A  PLANE  QUARTIC  CURVE.  387 

It  will  be  recalled  that  in  the  course  of  the  analysis  the  absolute  values, 
and  not  merely  the  ratios  of  the  coefficients  in  u^,  u2,  u3,  u4,  u^,  u6,  u?,  have 
been  definitely  fixed.     Thus  when   these   seven  bitangents   are   given   the 
values  of  alt  a,,  a3,  blt  b,,  ba,  etc.  are  definite  ;  therefore  the  equations  of  the 
15  bitangents  v.a,  v3l,  vn,  vu>  v»,  VM,  ......  are  now  determined  from  the  seven 

given  ones  in  an  unique  manner,  and   there   is  an    unique   quartic   curve 

expressed  by 

12  =  0, 


which  has  the  seven  given  lines  as  bitangents. 

It  remains  now  to  determine  the  remaining  six  double  tangents  whose 
characteristics  are  denoted  by 

45,  46,  47,  56,  57,  67. 

If  the  characteristics  1,  2,  3,  4,  5,  6,  7  be  taken  in  the  order  1,  4,  5,  2,  3,  6,  7 
it  is  clear  that  as  we  have  determined  the  double  tangents  u^,  u3l,  ul2  in 
terms  of  ul}  u»,  u3,  so  we  can  determine  the  tangents  u^,  usl,  uu  in  terms 
of  ul}  ut,  u5.  Thus  the  tangent  ««  can  be  found  by  substitutions  in  the 
foregoing  work.  For  the  actual  deduction  the  reader  is  referred*  to  the 
original  memoir,  Riemann,  Ges.  Werke  (Leipzig,  1876),  p.  471,  or  Weber, 
Theorie  der  Abel'schen  Functionen  vom  Geschlecht  3  (Berlin,  1876),  pp.  98—100. 
Putting  ctlul  =  x,  o2-M2  =  y,  a3u3  =  z,  i^fa  =  £,  %/«,  =  ??,  v12/a3=^,  /3i/<xi  =  Ai, 
yi/di  =  Bi,  Bifai  =  Gi  (i=  1,  2,  3),  the  quartic  has  the  form 


=  0, 

and  the  28  double  tangents  are  given  by  the  following  scheme,  where  the 
number  representing  the  characteristic  is  prefixed  to  each 

(1)  *=0,      (2)  y  =  0,       (3)  *=0,       (23)  |  =  0,       (31)  7;  =  0,       (12)  £=0, 
(4)    x  +  y+z  =  0,        (5)    A1x  +  A<,y+A3z  =  0,        (6)    B^x  +  B^y  +  B3z=  0, 

(7)     (7^  +  0^  +  6^  =  0, 
(14)     %  +  y  +  z  =  0,  (24)     ^+z  +  x  =  0,  (34)     £  +  x  +  y  =  0, 


(15)  -  +  A,y  +  A3z  =  Q,     (25)  -£•  +  A3z  +  AlX=0,     (35) 

AI  A-i  -- 

(16)  L  +  B.2y  +  B3z  =  0,    (26)  £  +  B3z  +  B1x=Q,    (36)  -^  +  B&  +  B,y  =  0, 

Jji  E*i  **> 

(17)  |  +  C,y  +  G3z  =  0,     (27)  ^-  +  G3z  +  C,x  =  0,     (37)  £  +  C,x  +  C,y  =  0, 

GI  G2  ^3 

*  For  the  theory  of  the  plane  quartic  curve  reference  may  be  made  to  geometrical  treatises  ; 
developments  in  connection  with  the  theta  functions  are  given  by  Schottky,  Crelle,  cv.  (1889), 
Frobenius,  Crelle,  xcix.  (1885)  and  ibid.  cm.  (1887)  ;  see  also  Cayley,  Crelle,  xciv.  and  Kohn, 
Crelle,  cvn.  (1890),  where  references  to  the  geometrical  literature  will  be  found. 

25—2 


388  THE   CASE   OF  THE   BITANGENTS  [247 

*  * 


(67) 


(75) 


-      _  _ 

J-   —  ^In-Aft  A    —  -/la^li  J.   — 

___ 


(d,(i\ 


__ 

51  (1  -  B,BZ}     B,  (1  - 


1  -  Ca  C3     1  -  (73  ^     1  -  0, 


(47} 


__  __  __  __ 

,  (1  -  G2G3)     C,  (1  -  ^00     C,  (1  -  C 

Here  the  six  quantities  x,  y,  z,  g,  i),  £  are  connected  by  the  equations 


=  0, 


rr  +  7T  +  rr  +  CiX+C,y+C3z  =  0. 

U,         l/j         O3 

Conversely,  if  we  take  arbitrary  constants  ^.,,  ^2,  A3,  5,,  52,  £3,  whose 
number,  6,  is,  when  ^  =  3,  equal  to  Sp  —  3,  namely  equal  to  the  number 
of  absolute  constants  upon  which  a  Riemann  surface  depends  when  p  =  3, 
and,  by  the  first  three  of  the  equations  (D)  determine  £,  77,  f  in  terms  of  the 
arbitrary  lines  x,  y,  z,  the  last  of  the  equations  (D)  will  determine  Clt  C.,,  C3 
save  for  a  sign  which  is  the  same  for  all  ;  then  it  can  be  directly  verified 
algebraically  that  the  28  lines  here  given  are  double  tangents  of  the  quartic 
curve  V#£  +  \/yt]  +  \/z%=  0. 


248.  Before  leaving  this  matter  we  desire  to  point  out  further  the 
connection  between  the  two  representations  of  the  tangents  which  have  been 
given.  Comparing  the  two  equations  of  the  fundamental  quartic  curve 
expressed  by  the  equations  (§§  246,  247) 


and  putting,  in  accordance  therewith, 

D  (xl  ,  x2  ,  x3}  =  £     H0  (xl  ,  x.,  ,  as,)  =  z£-  x%  -  yq,     X0  (xl  ,  x2  ,  a?,)  =  xyq 
and    (cf.    p.    382)    replacing    the    fourth    coordinate    T   by    T  +  u,    where 


249]  OF  A    PLANE   QUARTIC   CURVE.  389 

u  is  an  arbitrary  linear  function  of  x,  y,  z  or  xlt  x2,  x3)  the  equation  of  the 
cubic  surface 

(T+  ™)2  D  +  (T+  u)  00  +  X0  =  0, 
becomes 

T*£  +  T  (z%-  x%  -  y-n  +  2i*f  )  +  u*%  +  u  (z%  -  y<n  -  x%}  +  xyrj  =  0, 
or 


which  will  be  found  to  be  the  same  as 


Write  now 

v  =  u  —  x  —  z,     w  =  u  —  x  —  %  ,     u  =  u  —  x,     v'  =  u+y,     iv'  =  u+  rj; 

then  we  obtain  the  result,  easy  to  verify,  that  if  u,  v,  w,  u',  v',  w'  be  arbitrary 
linear  functions  of  the  homogeneous  space  coordinates  X,  Y,  Z,  and  T  be 
the  fourth  coordinate,  the  tangent  cone  to  the  cubic  surface* 

(T  +  u)(T+v)(T+w)-(T+u')(T  +  J)(T+v/)  =  Q  (i) 

from  the  vertex  X  =  0  =  Y=  Z  can  be  written  in  the  form 

V(P  -  P)  (u-  u'}  +  \/(u  -  v')  (u  -  w')  +  V(M'  -  v)  (u'  -  w)  =  0, 
where  P  —  P'  =  u  +  v  +  w  —  u'  —  v'  —  w'  ;  we  have  in  fact 

x  =  u  —  u',     y  =v'  —  u,     z  =  u'  —  v,     77  =  w'  —  u,     %=u'  —  w, 


Now  the  27  lines  on  the  cubic  surface  (i)  can  be  easily  obtainedf;  and 
thence  the  forms  obtained  in  §  247,  for  the  bitangents  of  the  quartic,  can  be 
otherwise  established. 

249.  Ex.  i.  Prove  that  when  the  sum  of  the  characteristics  of  three  bitangents  of  the 
quartic  is  an  even  characteristic,  their  points  of  contact  do  not  lie  upon  a  conic. 

By  enumerating  the  constants  we  infer  that  it  is  possible  to  describe  a  plane  quartic 
curve  having  seven  arbitrary  lines  as  double  tangents.  By  the  investigation  of  §  247 
it  follows  that  only  one  such  quartic  can  be  described  when  the  condition  is  introduced 
that  no  three  of  the  tangents  shall  have  their  points  of  contact  upon  a  conic.  By  the 
theory  here  developed  it  follows  that  for  a  given  quartic  such  a  set  of  seven  bitangents  can 
be  selected  in  8  .  36  =  288  ways. 

Ex.  ii.  We  have  given  an  expression  for  the  general  radical  form  \/A'(3>  of  any  given 
odd  characteristic.  Prove  that  a  radical  form  \/XM  whose  characteristic  is  even,  denoted, 
suppose,  by  the  index  123,  can  be  written  in  the  form 


*  Any  cubic  surface  can  be  brought  into  this  form,  Salmon,  Solid  Geometry  (1882),  §  533. 

t  See  Frost,  Solid  Geometry  (188(5),  §  537.  The  three  last  equations  (D)  of  §  247  are  deducible 
from  the  equations  occurring  in  Frost.  The  three  equations  correspond  to  the  three  roots  of  the 
cubic  equation  used  by  Frost. 


390  NOETHER'S  GENERAL  SOLUTION  [249 

where  X,  A1?  X2,  X3  are  constants,  and  MJ,  M^-  denote  double  tangents  of  the  characteristics 
denoted  by  the  suffixes,  as  in  §  247. 


Ex.  iii.     If  (^q,  £<?')>  (ir?  iO   denote  any  two  odd  characteristics  of  half-integers, 
express  the  quotient 


algebraically,  when  p  =  3. 

Ex.  iv.     Obtain  an  expression  of  the  quotient  of  any  two  radical  forms  \/  X$\ 
of  assigned  characteristics  and  known  zeros,  by  means  of  theta  functions,/*  being  equal  to  3. 

250.  Noether  has  given*  an  expression  for  the  solution  of  the  inversion 
problem  in  the  general  case  in  terms  of  radical  forms,  which  is  of  importance 
as  being  capable  of  great  generalization. 

Using  the  places  m1}  ...,  mp,  associated  as  in  Chap.  X.  with  an  arbitrary 
place  m,  and  supposing  them,  each  repeated,  to  be  the  remaining  zeros  of  a 
form  X  (3),  which  vanishes  to  the  second  order  in  each  of  the  places  Alt  ...,  A.2p_3 
in  which  an  arbitrary  ^-polynomial,  <£0,  which  vanishes  in  m,  further  vanishes, 
as  in  §  244,  let  VF(3)  be  any  radical  form,  and  <I>(1)  any  (^-polynomial  whose 
zeros  are  a1}  ...  ,  0^-2-  Then  (§  241)  the  consideration  of  the  rational  function 
</>02F<3)/[<E>(1)]2^(3)  leads  to  the  equations 


wherein  the  places 

X}  ,    .  .  .  ,   &-2p—  3  ,   C'i  ,    .  .  .  ,   Cp 

are  the  zeros  of  \/F(3),  all  of  o-u  ...,  crp,  a/,  ...,  arp'  are  integers,  and  z  is  an 
arbitrary  place;  and,  as  follows  from  these  equations,  the  places  xlt  .•.,x2p-3 
may  be  arbitrarily  assigned,  the  places  c1;  ...,  cp  and  the  form  \/F(3>  being 
determinate,  respectively,  from  these  equations  and  the  equation 


,  0  ^..  -f-..  rt'  •n' 

g5^W]P>  =C  1>a'        ......  '"*"  -'+       '"'"'  +  ......  +       e"'m 

•  r         /     •'  '  ^  /    -^j  ^n 

+  Tn[<rlvl     +  ......  +  <rp  vp    J, 

wherein  the  place  a  is  arbitrary.     Hence  if  we  speak  of 


as  the  characteristic  of  VF(3),  it  follows,  if  \IZ(®  be  another  radical  form  with 
the  characteristic 


and  the  zeros 

Xl,    .  .  .  ,   ^2p_3  ,   ttj  ,    .  .  .  ,   Clp  , 

*  Math.  Annal.  xxvm.  (1887),  p.  354,  "Zum  Umkehrproblem  in  der  Theorie  der  Abel'schen 
Functionen." 


250]  OF   THE   INVERSION    PROBLEM 

that  the  quotient  */Y®/*/Z(3),  which  is  equal  to 


391 


wherein  A  is  a  quantity  independent  of  x,  is  (§  187,  Chap.  X.)  also  equal  to 

_:  r/ _  /  _  -  /\  ~j%t  ^4-  -|-  ((T  '  —  fi  f\  v^'  ^1  (—\  /    %>  m  GI  j  "^1  <i/^*  *  "*P\ 

(7e  d  ~d   m    ' 

where  (7  is  a  quantity  independent  of  x ;  but  by  the  equations  here  given 
this  is  the  same  as 

.  {l    ,        M    *, «  ,  ,  /     ;        >\  „,#,  a-, 

vi[(ffl-pl)vl       + +  (*!,  -P,,)vp'    ] 

Ce 

where  £ H^  denotes  p  such  quantities  as  J(<7{ +  CT/T,:,  j  + +  o-p'ritp);  thus, 

if  we  put 

and  recall  the  formula  (§  175) 
we  infer  that 

where  E  is  a  quantity  independent  of  x. 

Now  in  fact  (§  245)  the  general  radical  form  \/F(3),  of  assigned  charac 
teristic  (^cr,  ^<r')>  is  given  by 

/      (3)  /      (3) 

where  ^  F!  ,...,*«'  F2p_  2  are  special  forms  of  this  characteristic,  and  Xj , . . . ,  X2^2 
are  constants.  If  we  introduce  the  condition  that  VF(3)  vanishes  at  the 
places  x1,  ...,#.,p_3  we  infer  that  VF(3)  is  equal  to  F^  (x,  xly  ...,  #2p_3),  where 

/Q\ 

F  is  independent  of  x  and  Aa  (x,  xlt  ...,  #21>_3)  denotes  the  determinant 


in  which  t  is  to  be  taken  in  turn  equal  to  1,  2,  ...,  2p  —  3.     Hence  we  have 

(3) 

,   _ 

~~ 


392  BY    MEANS   OF   RADICAL    FUNCTIONS.  [250 

where,  from  the  symmetry  in  regard  to  the  places  x,  xly  ...,  x.,p_3,  G  is 
independent*  of  the  position  of  any  of  these  places,  and  v  is  given  by 

y  =  lf>  «2p-  2-j-fl*!.  «i  +   ......   _|_^2p-3.  «2j>-3. 

To  apply  this  equation  to  the  solution  of  the  inversion  problem  expressed 
by  p  such  equations  as 

Vx>  '  *>  +  ......  +  Vxi"  ^P  —  U, 

where  pl,  ...,  ^p  denote  p  arbitrary  given  places,  we  suppose  the  positions  of 
the  places  xp+l,  ...,  x2p_3  to  be  given  ;  then  instead  of  &„(%,  xly  ...,  #2p_3)  we 
have  an  expression  of  the  form 


where  v  }  7[  (a),  ...,  v  Yp+i(x)  denote  forms  \/F(3)  (x)  vanishing  in  the  given 
places  asp+1,  ...,  xw_z,  and  A1}  ...,  Ap+1  are  unknown  constants.  Since  the 
arguments  u  are  given,  the  arguments  v  are  of  the  form  if'  a%>-2  +  w,  where  w 
is  known.  If  then  in  the  equation 


we  determine  the  unknown  ratios  A  1  :  A2  :  ......   :  Ap+1  :  B±  :  ......   :  Bp+\ 

by  the  substitution  of  2p  +  1  different  positions  for  the  place  x,  this  equation 
itself  will  determine  the  places  xlt  ...,  xp.  They  are,  in  fact,  the  zeros  of 
either  of  the  forms 


other  than  the  given  zeros  xp+l)  ...,  ^2p_3.  If  the  first  of  these  forms  be 
multiplied  by  an  arbitrary  form  \/F(3)  (x),  of  characteristic  (Jo-,  ^cr'),  the 
places  #a,  ...,  xp  are  given  as  the  zeros  of  a  rational  function  of  the  form 


of  which  4>p  —  6  zeros  are  known,  consisting,  namely,  of  the  places  xp+1,  ...,  Xy,-* 
and  the  zeros  of  ViT(3)  (x). 

In  regard  to  this  result  the  reader  may  consult  Weber,  Theorie  der  A  bePschen  Functio- 
nen  vom  Geschlecht  3  (Berlin,  1876),  p.  157,  the  paper  of  Noether  (Math.  Annal.  xxvm.) 
already  referred  to,  and,  for  a  solution  in  which  the  radical  forms  are  with  roots  of  rational 
functions,  Stahl,  Crelle,  LXXXIX.  (1880),  p.  179,  and  Crette,  cxi.  (1893),  p.  104.  It  will  be 
seen  in  the  following  chapter  that  the  results  may  be  deduced  from  another  result  of 
a  simpler  character  (§  274). 

251.  The  theory  of  radical  functions  has  far-reaching  geometrical  applications  to 
problems  of  the  contact  of  curves.  See,  for  instance,  Clebsch,  Crelle,  LXIII.  (1864),  p.  189. 
For  the  theory  of  the  solution  of  the  final  algebraic  equations  see  Clebsch  and  Gordan, 
Abel'sche  Functnen.  (Leipzig,  1866),  Chap.  X.  Die  Theilung;  Jordan,  Traite  des  Sub 
stitutions  (Paris,  1870),  p.  354,  etc.;  and  now  (Aug.  1896),  for  the  bitangents  in  case  p  =  3, 
Weber,  Lehrbuch  der  Algebra  (Braunschweig,  1896),  II.  p.  380. 

*  For  the  determination  of  G  see  Noether,  Math.  Annal.  xxvm.  (1887),  p.  368,  and  Klein, 
Math.  Annal.  xxxvi.  (1890),  pp.  73,  74. 


252] 


CHAPTER    XIV. 

FACTORIAL  FUNCTIONS. 

252.  THE  present  chapter  is  concerned*  with  a  generalisation  of  the 
theory  of  rational  functions  and  their  integrals.  As  in  that  case,  it  is  conve 
nient  to  consider  the  integrals  and  the  functions  together  from  the  first.  In 
order,  therefore,  that  the  reader  may  be  better  able  to  follow  the  course  of 
the  argument,  it  is  desirable  to  explain,  briefly,  at  starting,  the  results 
obtained.  All  the  functions  and  integrals  considered  have  certain  fixed 
singularities,  at  placesf  denoted  by  clf  ...,  ck.  A  function  or  integral  which 
has  no  infinities  except  at  these  fixed  singularities  is  described  as  everywhere 
finite.  The  functions  of  this  theory  which  replace  the  rational  functions  of 
the  simpler  theory  have,  beside  the  fixed  singularities,  no  infinities  except 
poles.  But  the  functions  differ  from  rational  functions  in  that  their  values 
are  not  the  same  at  the  two  sides  of  any  period  loop ;  these  values  have  a 
ratio,  described  as  the  factor,  which  i^  constant  along  the  loop  ;  and  a  system 
of  functions  is  characterised  by  the  values  of  its  factors.  We  consider  two 
sets  of  factors,  and,  correspondingly,  two  sets  of  factorial  functions,  those  of 
the  primary  system  and  those  of  the  associated  system;  their  relations  are 
quite  reciprocal.  We  have  then  a  circumstance  to  which  the  theory  of 
rational  functions  offers  no  parallel ;  there  may  be  everywhere  finite  factorial 
functions^..  The  number  of  such  functions  of  the  primary  system  which  are 
linearly  independent  is  denoted  by  cr'  +  1 ;  the  number  of  the  associated 
system  by  a-  +  1.  As  in  the  case  of  algebraical  integrals,  we  may  have  every 
where  finite  factorial  integrals.  The  number  of  such  integrals  of  the  primary 
system  which  are  linearly  independent  is  denoted  by  CT,  that  of  the  associated 
system  by  CT'.  The  factorial  integrals  of  the  primary  system  are  not  integrals 
of  factorial  functions  of  that  system ;  they  are  chosen  so  that  the  values  u,  u' 

*  The  subject  of  the  present  chapter  has  been  considered  by  Prym,  Crelle,  LXX.  (1869),  p.  354; 
Appell,  Acta  Mathematica,  xm.  (1890);  Hitter,  Math.  Annal.  XLIV.  (1894),  pp.  261—374.  In 
these  papers  other  references  will  be  found.  See  also  Hurwitz,  Math.  Annal.  XLI.  (1893),  p.  434, 
and,  for  a  related  theory,  not  considered  in  the  present  chapter,  Hurwitz,  Math.  Annal.  xxxix. 
(1891),  p.  1.  For  the  latter  part  of  the  chapter  see  the  references  given  in  §§  273,  274,  279. 

t  In  particular  the  theory  includes  the  case  when  &  =  0,  and  no  such  places  enter. 

£  This  statement  is  made  in  view  of  the  comparison  instituted  between  the  development  of 
the  theory  of  rational  functions  and  that  of  factorial  functions.  The  factorial  functions  have 
(unless  k  =  Q)  fixed  infinities. 


394  SUMMARY  OF   RESULTS.  [252 

of  such  an  integral  on  the  two  sides  of  a  period  loop  are  connected  by  an 
equation  of  the  form  u'  =  Mu  +  p,,  where  p,  is  a  constant  and  M  is  the  factor  of 
the  primary  system  of  factorial  functions  which  is  associated  with  that  period 
loop.  The  primary  and  associated  systems  are  so  related  that  if  F  be  a 
factorial  function,  of  either  system,  and  G'  a  factorial  integral  of  the  other 
system,  FdG'jdx  is  a  rational  function  without  assigned  singularities.  In  the 
case  of  the  rational  functions,  the  smallest  number  of  arbitrary  assigned  poles 
for  which  a  function  can  always  be  constructed  is  p  +  1.  In  the  present 
theory,  as  has  been  said,  it  may  be  possible  to  construct  factorial  functions  of 
the  primary  system  Avithout  poles ;  but  when  that  is  impossible,  or  <r'  +  1  =  0, 
the  smallest  number  of  arbitrary  poles  for  which  a  factorial  function  of  the 
primary  system  can  always  be  constructed  is  or'  +  1.  Similarly  when 
a-  +  1  =  0,  the  smallest  number  of  arbitrary  poles  for  which  a  factorial  func 
tion  of  the  associated  system  can  always  be  constructed  is  OT  + 1.  Of  the 
two  numbers  cr  +  1,  cr'+l,  at  least  one  is  always  zero,  except  in  one  case, 
when  they  are  both  unity.  When  o-'  +  l  is  >  0,  the  everywhere  finite  fac 
torial  functions  of  the  primary  system  can  be  expressed  linearly  in  terms  of 
the  everywhere  finite  factorial  integrals  of  the  same  system.  We  can  also 
construct  factorial  integrals  of  the  primary  system,  which,  beside  the  fixed 
singularities,  have  assigned  poles ;  the  least  number  of  poles  of  arbitrary 
position  for  which  this  can  be  done  is  a-  +  2.  And  we  can  construct  factorial 
integrals  of  the  primary  system  which  have  arbitrary  logarithmic  infinities ; 
the  least  number  of  such  infinities  of  arbitrary  position  is  cr  +  2.  For  the 
associated  system  of  factors  the  corresponding  numbers  are  cr'  +  2. 

It  will  be  found  that  all  the  formulae  of  the  general  theory  are  not  imme 
diately  applicable  to  the  ordinary  theory  of  rational  functions  and  their 
integrals.  The  exceptions,  and  the  reasons  for  them,  are  pointed  out  in 
footnotes. 

The  deduction  of  these  results  occupies  §§  253 — 267  of  this  chapter.  The 
section  of  the  chapter  which  occupies  §§  271 — 278,  deals,  by  examples,  with 
the  connection  of  the  present  theory  with  the  theory  of  the  Biemann  theta 
functions.  With  a  more  detailed  theory  of  factorial  functions  this  section 
would  be  capable  of  very  great  development.  The  concluding  section  of  the 
chapter  deals  very  briefly  with  the  identification  of  the  present  theory  with 
the  theory  of  automorphic  functions. 

253.  Let  G!,  ...,  Ck  be  arbitrary  fixed  places  of  the  Riemann  surface, 
which  we  suppose  to  be  finite  places  and  not  branch  places.  In  all  the 
investigations  of  this  chapter  these  places  are  to  be  the  same.  They  may  be 
called  the  essential  singularities  of  the  systems  of  factorial  functions.  We 
require  the  surface  to  be  dissected  so  that  the  places  c1}  ...,  ck  are  excluded 
and  the  surface  becomes  simply  connected.  This  may  be  effected  in  a  manner 
analogous  to  that  adopted  in  §  180,  the  places  c1}  ...,  Ck  occurring  instead  of 


253] 


DISSECTION    OF   THE   SURFACE. 


395 


zlt  ...,zk.  But  it  is  more  convenient,  in  view  of  one  development  of  the 
theory,  to  suppose  the  loops  of  §  180  to  be  deformed  until  the  cuts*  between 
the  pairs  of  period  loops  become  of  infinitesimal  length.  Then  the  dissection 
will  be  such  as  that  represented  in  figure  9 ;  and  this  dissection  is  sufficiently 

Fig.  9. 


well  represented  by  figure  10.  We  call  the  sides  of  the  loops  (ar),  (br),  upon 
which  the  letters  ar,  br  are  placed,  the  left-hand  sides  of  these  loops,  and  by 
the  left-hand  sides  of  the  cuts  (7^,  ...,  (7^),  to  the  places  clt  ...,  c&,  we  mean 


the  sides  which  are  on  the  left  when  we  pass  from  A  to  d,  ...,  c^  respec 
tively.  The  consideration  of  the  effect  of  an  alteration  in  these  conventions 
is  postponed  till  the  theory  of  the  transformation  of  the  theta  functions 
has  been  considered. 

*  These  cuts  are  those  generally  denoted  by  clt  ...,cp_,.     Cf.  Forsyth,  Theory  of  Functions, 
§181. 


396  FUNDAMENTAL   EXPRESSION   OF    FACTORIAL   FUNCTIONS.  [254 

254.     In  connection  with  the  surface  thus  dissected  we  take  now  a  series 
of  2p  +  k  quantities 

Xj,  ...,\k,     hl}  ...,  hp,     gi,...,gp, 

which  we  call  the  fundamental  constants;  we  suppose  no  one  of  \1}  ...,  \k  to 
be  a  positive  or  negative  integer,  or  zero ;  but  we  suppose  X,  +  . . .  +  \t  to  be 
an  integer,  or  zero ;  and  we  consider  functions 

(1)  which  are  uniform  on  the  surface  thus  dissected,  and  have,  thereon, 
no  infinities  except  poles, 

(2)  whose    value    on    the    left-hand   side   of  the    period    loop   (a,f)   is 
g-STriAj  times  the  value  on  the  right-hand  side ;  whose  value  on  the  left-hand 
side  of  the  period  loop  (h)  is  e27"^  times  the  value  on  the  right-hand  side, 

(3)  which*,  in  the  neighbourhood  of  the  place  c;,  are  expressible  in  the 
form  t~^fa,  where  t  is  the  infinitesimal  at  c;  and  fa  is  uniform,  finite,  and  not 
zero  in  the  neighbourhood  of  the  place  c;, 

(4)  which,  therefore,  have  a  value  on  the  left-hand  side  of  the  cut  7; 
which  is  e~-ni*i  times  the  value  on  the  right-hand  side. 

Let  «1(  ...,  OM,  &,  ...,  f3N  be  any  places;  consider  the  expression 

x,a  x,  a  x,  a  x,a  x,a  x,akx,a 

f=  ^e11/?,,  m+---  +  lip,,,  m  -  nai)  m  -  ...  -  naj/>  m  -  2«  [(A  +  ffJ  vi     +...  +  (hp  +  Hp)  rp    ]  -  S  XjIIc.,  ,„ 

«/  t=l 

wherein  A  is  independent  of  the  place  x, 

N-M=2\,  (i), 

*=i 

SX  being  an  integer  (or  zero),  m  is  an  arbitrary  place,  and  Hl ,  ...,  Hp  are 
integers.  It  is  clear  that  this  expression  represents  a  function  which  is 
uniform  on  the  dissected  surface,  which  has  poles  at  the  places  al}  ...,  aM>  and 
zeros  at  the  places  /3j,  ...,  /3N,  and  that  in  the  neighbourhood  of  the  place  c; 
this  function  has  the  character  required.  For  the  period  loop  (a^)  the 
function  has  the  factor  e~Zvt^hi+a^  =  e~Zwihi,  as  desired;  for  the  period  loop 
(bi)  the  function  has  the  factor  eZwtK,  where 


r=l  r=l 

and  this  factor  is  equal  to  e2niyi  if  only 

k 

r=l 

r=p 

r=l 

Gi  being  an  integer. 

*  It  is  intended,  as  already  stated,  that  the  places  cl,  ...,  c*  should  be  in  the  finite  part  of  the 
surface  and  should  not  be  branch  places. 


255]  THE  TWO   SYSTEMS   OF   FACTORS.  397 

It  follows  therefore  that,  subject  to  the  conditions  (i)  and  (ii),  such  a 
function  as  has  been  described  certainly  exists. 

Conversely  it  can  be  immediately  proved  that  any  such  function  must  be 
capable  of  being  expressed  in  the  form  here  given,  and  that  the  conditions 
(i),  (ii)  are  necessary. 

Unless  the  contrary  be  expressly  stated,  we  suppose  the  quantities 
X^.-.jXjfc,  hly...,hp,  g1,...,gp  always  the  same,  and  express  this  fact  by 
calling  the  functions  under  consideration  factorial  functions  of  the  primary 
system.  The  quantities  e~2iri^,  ...,  e~-ni*k,  e"2™'1*,  ...,  e~Zwihp,  e27™^',  ...,  e27™^>  are 
called  the  factors.  It  will  be  convenient  to  consider  with  these  functions 
other  functions  of  the  same  general  character  but  with  a  different  system  of 
fundamental  constants, 

Xt ,  . . . ,  Xj/,  /*/, . . . ,  hp',  g-t,  ...,  gpi 
connected  with  the  original  constants  by  the  equations 

X;  +  X/  +1=0,    hi  +  hi  =  0,   g{  +  g-  =  0  ; 

these  functions  will  be  said  to  be  functions  of  the  associated  system.  The  fac 
tors  associated  therewith  are  the  inverses  of  the  factors  of  the  primary  system. 

255.  As  has  been  remarked,  the  rational  functions  on  the  Riemann 
surface  are  a  particular  case  of  the  factorial  functions,  arising  when  the 
factors  are  unity  and  no  such  places  as  cl5  ...,  ck  are  introduced.  From  this 
point  of  view  the  condition  (i),  which  can  be  obtained  as  the  condition  that 

Id  log/,  taken  round  the  complete  boundary  of  the  dissected  surface,  is  zero, 

is  a  generalisation  of  the  fact  that  the  number  of  zeros  and  poles  of  a  rational 
function  is  the  same,  and  the  condition  (ii)  expresses  a  theorem  generalising 
Abel's  theorem  for  integrals  of  the  first  kind. 

Now  Riemann's  theory  of  rational  functions  is  subsequent  to  the  theory 
of  the  integrals ;  these  arise  as  functions  which  are  uniform  on  the  dissected 
Riemann  surface,  but  differ  on  the  sides  of  a  period  loop  by  additive 
constants.  In  what  follows  we  consider  the  theory  in  the  same  order,  and 
enquire  first  of  all  as  to  the  existence  of  functions  whose  differential  coefficients 
are  factorial  functions.  For  the  sake  of  clearness  such  functions  will  be 
called  factorial  integrals;  and  it  will  appear  that  just  as  rational  functions 
are  expressible  by  Riemann  integrals  of  the  second  kind,  so  factorial  functions 
are  expressible  by  certain  factorial  integrals,  provided  the  fundamental  con 
stants  of  these  latter  are  suitably  chosen.  We  define  then  a  factorial  integral 
of  the  primary  system,  H,  as  a  function  such  that  dH/dx  is  a  factorial 
function  with  the  fundamental  constants 


398  FACTORIAL   INTEGRALS.  [255 

thus  dH/dx  has  the  same  factors  as  the  factorial  functions  of  the  primary 
system,  but  near  the  place  d,  dH/dx  is  of  the  form  t~(*i+l}  fa,  where  fa  is 
uniform,  finite  and  not  zero  in  the  neighbourhood  of  d-  Similarly  we  define 
a  factorial  integral  of  the  associated  system,  H',  to  be  such  that  dH'/dx 
is  a  factorial  function  with  the  fundamental  constants 

V  +  1,  .  .  .  ,  V  +  1,   A/,  .  .  .  ,  V,  ffi,  ...,  ffp, 
or 

—  A]  ,  .  .  .  ,        A.£  ,          III,   ...  ,        lip,          (/i  ,   .  .  .  ,         ffp  5 

thus,  if/  be  any  factorial  function  of  the  primary  system,  fdH'/dx  is  a 
rational  function  on  the  Riemann  surface,  for  which  the  places  c1}  ....  Ck 
are  not  in  any  way  special.  And  similarly,  if/'  be  any  factorial  function 
of  the  associated  system,  and  H  any  factorial  integral  of  the  primary 
system,  /'  dH/dx  is  a  rational  function. 

The  values  of  a  factorial  integral  of  the  primary  system,  H,  at  the  two 
sides  of  any  period  loop  are  connected  by  an  equation  of  the  form 


where  p  is  one  of  the  factors  e~-irihr,  e^'UJr,  and  fl  is  a  quantity  which  is 
constant  along  the  particular  period  loop.     Near  d,  H  is  of  the  form 


where  At  is  a  constant,  fa  is  uniform,  finite,  and,  in  general,  not  zero  in  the 
neighbourhood  of  C;,  and  (7f  is  a  constant,  which  is  zero  unless  Xt-  -f-  1  be  a 
positive  integer  (other  than  zero),  and  may  be  zero  even  when  X;  +  1  is  a 
positive  integer.  After  a  circuit  round  d,  H  will  be  changed  into 


H  =  Ai  +  e~z^  rA*  fa  +  Z-jriCi  +  Gi  log  t  ; 

thus,  when  Gt  =  0, 

H=  He-zvi^  +  Ai(l-  er****), 

and  when  d  is  not  zero,  and,  therefore,  \  +  1  is  a  positive  integer, 

H=H 
in  either  case  we  have 


where  7  =  e~2iriki,  and  F  is  constant  along  the  cut  (7;). 

Thus,  in  addition  to  the  fundamental  factors  of  the  system,  there  arise, 
for  every  factorial  integral,  2p  +  k  new  constants,  *2p  of  them  such  as  that 
here  denoted  by  ft  and  k  of  them  such  as  that  denoted  by  F.  It  will  be 
seen  subsequently  that  these  are  not  all  independent. 


256]  FACTORIAL   INTEGRALS   WITHOUT   INFINITIES.  399 

As  has  been  stated  we  exclude  from  consideration  the  case  in  which  any 
one  of  \i,  ...,  At  is  an  integer,  or  zero.  Thus  the  constants  Ci  will  not  enter; 
neither  will  the  corresponding  constants  for  the  associated  system. 

256.  Consider  now  the  problem  of  finding  factorial  integrals  of  the 
primary  system  which  shall  be  everywhere  finite.  Here,  as  elsewhere,  when 
we  speak  of  the  infinities  or  zeros  of  a  function,  we  mean  those  which  are  not 
at  the  places  d,  ...,  ck,  or  which  fall  at  these  places  in  addition  to  the  poles 
or  zeros  which  are  prescribed  to  fall  there. 

If  V  be  such  a  factorial  integral,  dVjdx  is  only  infinite  when  dx  is  zero 
of  the  second  order,  namely  2p  —  2  +  2n  times,  at  the  branch  places  of  the 
surface.  And  d  V/dx  is  zero  at  x  =  oo  ,  2n  times*.  Thus,  if  N denote  the  num 
ber  of  zeros  of  dVjdx  which  are  not  due  to  the  denominator  dx,  or,  as  we  may 
say  (cf.  §  21)  the  number  of  zeros  of  dV,  we  have  by  the  condition  (i)  §  254, 

N  +  2n  =  2p  -  2  +  2/i  +  2  (X*  +  1), 
1=1 

so  that  the  number  of  zeros  of  dV  is  2p  -  2  +  2  (X;  +  1). 

Now  let  f0  denote  a  factorial  function  with  the  primary  system  of 
factors,  but  with  behaviour  at  a  like  J-to+D  fa,  where  fa  is  uniform,  finite, 
and  not  zero  at  a.  Then,  if  an  everywhere  finite  factorial  integral  V 
exists  at  all,  Z,  =f0-ldV/dx,  will  be  a  rational  function  on  the  Riemann 
surface,  infinite  at  the  (say  N0)  zeros  of  /0,  and  2w  +  2p-2  times  at  the 
branch  places  of  the  surface,  and  zero  at  the  (say  M0)  poles  of /0,  and  In 

times  at  x  =  oo  (beside  being  zero  at  the  zeros  of  dV).     Conversely  a  rational 

f 
function  Z  satisfying  these  conditions  will  be  such  that  \ZfQdx  is  a  function  V. 


Thus  the  number  of  existent  functions  V  ivhich  are  linearly  independent  is  at 
least 


provided  this  be  positive.  We  are  therefore  sure,  when  this  is  the  case,  that 
functions  V  do  exist.  To  find  the  exact  number,  let  F0  be  one  such ;  then 
if  F  be  any  other,  dV/dV0  is  a  rational  function  with  poles  in  the 

2p  -  2  +S(X+  1)  zeros  of  dV0;  and  conversely  if  R  be  a  rational  function 

e 
whose  poles  are  the  zeros  of  dVQ,  the  integral  IRdV0  is  a  function  F.    Thusf 

the  number  of  functions  V,  when  any  exist,  is  (§  37,  Chap.  III.) 
*r,  =  p-l  +  2(X  +  l)  +  <r+l, 

*  These  numbers  may  be  modified  by  the  existence  of  a  branch  place  at  infinity.  But  their 
difference  remains  the  same. 

t  For  the  ordinary  case  of  rational  functions  er  +  1,  as  here  defined,  is  equal  to  unity,  and, 
therefore,  omitting  the  term  S  (\  +  l),  we  have  -a -p. 


400  EXISTENCE    OF    FACTORIAL    FUNCTIONS.  [256 

where  <r  +  1  is  the  number  of  linearly  independent  differentials  dv,  of  ordinary 
integrals  of  the  first  kind,  which  vanish  in  the  2p  —  2  +  2  (X+l)  zeros  of  the 
differential  dV0  of  any  such  function  V0.  Since  dV/dV0  is  a  rational 
function,  the  number  of  differentials  dv  vanishing  in  the  zeros  of  dV0  is  the 
same  as  the  number  vanishing  in  the  zeros  of  dV.  Since  dv  has  2p  —  2  zeros, 
a  +  1  vanishes  when  2  (A  +  1)  >  0. 

Ex.     For  the  hyperelliptic  surface 


the  factorial  integrals,  V,  having  the  same  factors  at  the  period  loops  as  the  root  function 
•J(x  —  a}  (x  —  b),  and  no  other  factors,  are  given  by 

_  dx 

*l(x-a)(x-V)  (x,  l)p_2  — 

and  -u3=p  —  1.     Here  £=0  ;  there  are  no  places  clt  ...  ,  ck. 

257.  The  number  <r  +  1  is  of  great  importance  ;  when  it  is  greater 
than  zero,  which  requires  2  (X  +  1)  to  be  negative  or  zero,  there  are  cr  +  1 
factorial  functions  of  the  associated  system  which  are  nowhere  infinite. 

For  if  V  be  an  everywhere  finite  factorial  integral  of  the  primary  system, 
and  dv1}  ...,  dvv+1  represent  the  linearly  independent  differentials  of  integrals 
of  the  first  kind  which  vanish  in  the  zeros  of  dV,  the  functions 


dV"  '"' 

whose  behaviour  at  a  place  Ci  is  like  that  of  TT^+T,  &>  where  fa  is  uniform, 

finite  and  not  zero  in  the  neighbourhood  of  a,  namely  of  t^'fy,  are  clearly 
factorial  functions  of  the  associated  system,  without  poles.  Conversely  if  K' 
denote  an  everywhere-finite  factorial  function  of  the  associated  system,  the 

integral  \K'dV  is  the  integral  of  a  rational  function,  and  does  not  anywhere 
become  infinite.  Denoting  it  by  v,  dv  vanishes  at  the  2p  —  2  +  2(A.  +  l) 

k 

zeros  of  dV  as  well  as  at  the  0+2  A,/,  =  —  2  (A.  +  1),  zeros  of  K  '  (cf.  the 

t=i 

condition  (i),  §  254).  Thus,  to  every  factorial  integral  V  we  obtain  <r  +  1 
functions  K'  ;  and  since,  when  <r  +  1  >  0,  the  quotient  of  two  differentials 
dV,  dV0  can*  be  expressed  by  the  quotient  of  two  differentials  dv,  dv0,  we 
cannot  thus  obtain  more  than  <r  +  1  functions  K'  ;  while,  conversely,  to  every 
function  K'  we  obtain  a  differential  dv  which  vanishes  in  the  zeros  of  any 
assigned  function  V;  and,  as  before,  we  cannot  obtain  any  others  by  taking, 
instead  of  V,  another  factorial  integral  V0. 

*  Cf.  Chap.  VI.  §  98. 


258]  WHICH    DO   NOT   BECOME   INFINITE.  401 

258.  The  existence  of  these  everywhere  finite  factorial  functions,  K',  of 
the  associated  system  can  also  be  investigated  a  priori  from  the  fundamental 
equations  (i)  and  (ii)  (§  254).  These  give,  in  this  case, 


-  TI,  p  (hp  +  Hp),         (iii) 
and  N=-  2  (Xr+l), 

r=l 

where  Glt  ...,  Gp,  Hl,  ...,  Hp  are  integers. 

Hence  no  functions  K'  exist  unless  2  (A,  +  1)  be  a  negative  integer  or  be 
zero  ;  we  consider  these  possibilities  separately. 

When  2(X+1)  =  0,  it  is  necessary,  for  the  existence  of  such  functions, 
that  the  fundamental  constants  satisfy  the  conditions 


conversely,    when   these   conditions    are    fulfilled,   taking   suitable   integers 
Hl}  ...,  Hp,  it  is  clear  that  the  function 


wherein  A  is  an  arbitrary  constant,  and  a,  m  are  arbitrary  places,  is  an 
everywhere  finite  factorial  function  of  the  associated  system,  and  it  can  be 
immediately  seen  that  every  such  function  is  a  constant  multiple  of  E0.  If 
then  we  denote  the  number  of  functions  K'  by  2  +  1  (to  be  immediately 
identified  with  a  +  1  ),  we  have,  in  this  case,  2  +  1  =  1;  and  there  are  p 

functions  V,  given  by  V=\E^dv,  where  dv  is  in  turn  the  differential  of 

every  one  of  the  linearly  independent  integrals  of  the  first  kind  ;  it  is  easy  to 
see  that  every  function  V  can  be  thus  expressed.  Thus,  in  the  zeros  of  a 
differential  dV  there  vanishes  one  differential  dv,  so  that  a  +1  =  1.  Hence 
o-  +  1  =  2  +  1,  and  the  formula  w  =p  —  l  +  2(\  +  l)  +  <r  +  l  is  verified. 

When  2(\  +  l)  is  negative  and  numerically  greater  than  zero,  and  the 
equations  (iii)  have  any  solutions,  let  t  denote  the  number  of  linearlv  in 
dependent  differentials  dv  which  vanish  in  the  places  of  one  and  therefore  of 
every  set,  &,  ...,  /9V,  which  satisfies  these  equations;  then*  the  number  of 
sets  which  satisfy  these  equations  is  oo  S-P+*}  where  s  =  —  2  (X  +  1)  ;  thus  the 
quotient  of  two  functions  K'  is  a  rational  function  with  2  +  1,  =s—p+t  +  l 
arbitrary  constants,  one  of  these  being  additive.  This  is  then  the  number  of 
linearly  independent  functions  K'.  If  K'  be  one  of  these  functions,  and 

'  Cf.  §  158,  Chap.  VIII.  ;  §  95,  Chap.  VI. 

B-  26 


402  EXPRESSION   OF   FINITE   FACTORIAL   FUNCTIONS  [258 

dVi,  ...,  dvt  denote  the  differentials  vanishing  in  the  zeros  of  K',  it  is  clear 

that  the  functions 

fdvl  rdvt 

JK"  ""  IK' 

are  finite  factorial  integrals  of  the  primary  system,  that  is,  are  functions  V ; 
conversely  if  Fbe  any  finite  factorial  integral  of  the  primary  system,  \K'dV 

is  an  integral,  v,  of  the  first  kind  such  that  dv  vanishes  in  the  zeros  of  K'. 
Hence  the  number  t,  which  expresses  the  number  of  differentials  dv  which 
vanish  in  the  zeros  of  K',  is  equal  to  the  number,  CT,  of  functions  V.  But  we 
have  proved  that  •&  =p  —  I  +  '2t(\+l)+<T+l,  and,  above,  that  t=p  -I—  s+2+1. 
Hence  o-  +  l  =2+  1.  .vl 

Thus  we  have  the  results*:  The  number,  cr  +  1,  of  everywhere  finite 
factorial  functions,  K' ,  of  the  associated  system  is  equal  to  the  number  of 
differentials  dv  which  vanish  in  the  2p  —  2  +  2  (X  +  1)  zeros  of  any  differential 
dV;  hence  (§  21,  Chap.  II.)  <7  +  1  is  less  than  p,  unless  2  (X  +  1)  =  -  (2^>  -  2). 

Also,  when  a  +  1  >  0,  the  number,  vr,  of  everywhere  finite  factorial  integrals, 
V,  of  the  primary  system,  is  equal  to  the  number  of  differentials  dv  which 
vanish  in  the  s,  =  -  2  (X  +  1),  zeros  of  any  function  K'.  The  argument  by 
which  this  last  result  is  obtained  does  not  hold  whenf  cr  +  1  =  0.  When 
o-  +  1  >  0,  it  follows  that  OT  is  not  greater  than  p. 

Similarly  when  s',  =  -  2  (X'  +  1),  =  Sx,  =  -  s  -  k,  is  >  0,  we  can  prove,  by 
considering  the  primary  system,  that  there  are  a'  + 1  everywhere  finite 
factorial  functions  K  of  the  primary  system,  where  cr'  +  1  is  the  number  of 
differentials  dv  vanishing  in  the  2p  -  2  -  2X,  =2p  —  2  +  s  +  k.  zeros  of  any 
differential  dV ";  and  that,  when  cr'+l>0,  the  number  &',  of  everywhere 
finite  factorial  integrals,  V ,  of  the  associated  system  is  equal  to  the  number 
of  differentials  dv  vanishing  in  the  s'  zeros  of  any  function  K.  Hence 
a'  +  1  =  0  when  s  >  0,  and,  then,  no  functions  K  exist.  When  s  =  0  we  have 
seen  that  there  may  or  may  not  be  functions  K' ;  but  there  cannot  be  func 
tions  K  unless  k  =  0,  since  otherwise  2p  —  2+s  +  k>2p—  2.  And  then  the 
existence  of  functions  K  depends  on  the  condition  whether  the  fundamental 
constants  be  such  that 


is  a  function  of  the  primary  system  or  not,  Hl}  ...,HP  being  suitable  integers, 
namely  whether  there  exist  relations  of  the  form 

9i.  +  Gi+fa  +  H,}  n,  l  + +  (hp  +  Hp)  ri>p  =  0,         (i  =  1,  2,  ...,  p), 

*  Which  hold  for  the  ordinary  case  of  rational  functions,  <r  +  l  being  then  unity. 

t  In  the  case  of  the  factorial  functions  which  are  square  roots  of  rational  functions  of  which 
all  the  poles  and  zeros  are  of  the  second  order,  so  that  the  places  cl ,  . . . ,  ck  are  not  present,  and 
the  numbers  g,  h  are  half  integers,  we  have  cr=p  -  1,  a  + 1  =  0. 


260]  BY   FINITE    FACTORIAL    INTEGRALS.  403 

where  Glt  ...,  Gp  are  integers.  In  such  case  E0  is  a  finite  factorial  function 
of  the  associated  system. 

On  the  whole  then  the  theory  breaks  up  into  four  cases  (i)  a  +  1  =  0, 
<r'  +  I  =  0,  (ii)  a-  +  1  >  0,  a-'  +  1  -  0,  (Hi)  o-  +  1  =  0,  a  +  1  >  0,  (iv)  a  +  1  =  1, 
<T'  +  1  =  1.  Of  these  the  cases  (ii)  and  (iii)  are  reciprocal. 

259.  One  remark  remains  to  be  made  in  this  connection.  When 
v  +  1  >  0  there  are  everywhere  finite  functions,  K',  of  the  associated  system, 
given  (§  257)  by 

dvi      cfag  dva+l 

dV"   dV"  '     "'  ~dV* 

these  have,  at  any  one  of  the  places  clt  ...,  Ck,  a  behaviour  represented  by 
that  of  t~*<f>  ;  hence  the  differential  coefficients  of  these  functions  satisfy  all 
the  conditions  whereby  the  differential  coefficients,  dV'/dx,  of  the  everywhere 
finite  factorial  integrals  of  the  associated  system,  are  defined.  Therefore*  the 
functions  K'  are  expressible  linearly  in  terms  of  the  functions  F/,  ...,  V'w> 
by  equations  of  the  form 


where  the  coefficients,  \j,  \  are  constants. 

Hence  also  the  difference  nr'  —  (a  +  1)  is  not  negative.  This  is  also 
obvious  otherwise.  For  when  <r  +  1  >  0,  —  2  (X  +  1),  =s,  is  zero  or  positive, 
and  cr  +  l>jp  (§  258),  and,  therefore,  v  -  a;  =p  -(a-  +  1)  +  er'  +  1  +  k  +  s, 
can  only  be  as  small  as  zero  when  k  =  0  =  s,  and  a  +  1  =  p  ;  these  are  in 
compatible. 

Similarly,  when  a'  +  1  >  0,  the  everywhere  finite  factorial  functions  of  the 
original  system  are  linear  functions  of  the  factorial  integrals  Vl}  ...,  Vw. 

It  follows  f  therefore  that  of  the  «•  periods  of  the  functions  F15  ...,  FOT, 
at  any  definite  period  loop,  only  -a  -  (a-'  +  1)  can  be  regarded  as  linearly 
independent;  in  fact,  a  +  1  of  the  functions  V1}  ...,  FOT  may  be  replaced 
by  linear  functions  of  the  remaining  w  -  (a-'  +  1),  and  of  the  functions 
Klt  ...,  KV'+I. 

260.  A  factorial  integral  is  such  that  its  values  at  the  two  sides  of  a  period  loop  of 
the  first  kind  are  connected  by  an  equation  of  the  form  u'  =  fiiU  +  Qiy  its  values  at  the  two 
sides  of  a  period  loop  of  the  second  kind  are  connected  by  an  equation  of  the  form 
w'=/*'«M  +  Q't>  and  its  values  at  the  two  sides  of  a  loop  (y{)  are  connected  by  an  equation 
of  the  form  u'^yiU  +  Ti,  where  J  1^  =  ^(1-^).  Of  the  2p+lk  periods  Qi}  Q'f,  I\  thus 


*  It  is  clearly  assumed  that  K'i  is  not  a  constant  ;  thus  the  reasoning  does  not  apply  to  the 
ordinary  case  of  rational  functions. 

t  In  the  ordinary  case  of  rational  functions  this  number  or  -  (<r  +  1)  must  be  replaced  by  p. 
See  the  preceding  note. 

J  §  255.     The  case  where  one  of  \j  ,  ...,  \k  is  zero  or  an  integer  is  excluded. 

26—2 


404  DELATIONS   AMONG   THE   PERIODS.  [260 

arising,  two  at  least  can  be  immediately  excluded.  For  it  is  possible,  by  subtracting  one 
of  the  constants  Alt  ...,  Ak  from  the  factorial  integral,  to  render  one  of  the  periods 
TU  ...,  Tk  zero;  and  by  following  the  values  of  the  factorial  integral,  which  is  single- 
valued  on  the  dissected  surface,  once  completely  round  the  sides  of  the  loops,  we  find,  in 
virtue  of  y1y2  •••  yt=lj  that 

2   [Oi(l-/ii')-ai/(l-f*i)]  =  ri  +  y1ra  +  y1y2r3  +  ...  +y1y2...yk-lTk. 
i=l 

Thus  there  are  certainly  not  more  than  2p  —  2+k  linearly  independent  periods  of  a 
factorial  integral. 

Suppose  now  that  V  is  any  everywhere  finite  factorial  integral  of  the  original  system, 
and  Vi  is  any  one  of  the  corresponding  integrals  of  the  associated  system.     The  integral 

I  Vd  F/,  taken  once  completely  round  the  boundary  of  the  surface  which  is  constituted  by 

the  sides  of  the  period  loops,  is  equal  to  zero.  By  expressing  this  fact  we  obtain  an 
equation  which  is  linear  in  the  periods  of  V  and  linear  in  the  periods  of  F/.  By  taking  i 
in  turn  equal  to  1,  2,  ...  ,  or',  we  thus  obtain  07'  linear  equations  for  the  periods  of  V, 
wherein  the  coefficients  are  the  periods  of  F1',  .  .  .  ,  V  w>.  As  remarked  above  these  coeffi 

cients  are  themselves  connected  by  <r  +  1  linear  equations  ;  so  that  we  thus  obtain  at  most 
or'  —  (<r  +  l)  linearly  independent  linear  equations  for  the  periods  of  F.  If  these  are  inde 
pendent  of  one  another  and  independent  of  the  two  reductions  mentioned  above,  it  follows 
that  the  2p  +  k  periods  of  V  are  linearly  expressible  by  only 

2p 
periods,  at  most.     Now  we  have 


and  therefore 
so  that 

Thus  or-(<r'-f  1)  is  the  number  of  periods  of  a  function  V  which  appear  to  be  linearly 
independent;  and,  taking  account  of  the  existence  of  the  functions  K^  ...,  Ka'+\,  this  is 
the  same  as  the  number  of  independent  linear  combinations  of  the  functions  Fn  ...  ,  FOT, 
which  are  periodic*.  But  the  conclusions  of  this  article  require  more  careful  considera 
tion  in  particular  cases  ;  it  is  not  shewn  that  the  linear  equations  obtained  are  always 
independent,  nor  that  they  are  the  only  equations  obtainable. 

Ex.  i.     Obtain  the  lineo-linear  relation  connecting  the  periods  of  the  everywhere  finite 
factorial  integrals   F,    V,  of  the  primary  and  associated  system,  which  is  obtained   by 

expressing  that  the  contour  integral  I  Vd  V  vanishes. 

Ex.  ii.     In  the  case  of  the  ordinary  Kiemann  integrals  of  the  first  kind,  the  relation 


is  identically  satisfied,  and  further  &=0.     Thus  the  reasoning  of  the  text  does  not  holdt. 

*  We  can  therefore  form  linear  combinations  of  the  periodic  functions  V,  for  which  the  inde 
pendent  periods  shall  be  1,  0,  .  .  .  ,  0  ;  0,  1,  .  .  .  ,  0  ;  etc.,  as  in  the  ordinary  case. 

t  In  that  case  the  numbers  -a'  —  (ff  +  1),  2p-2  +  k,  are  to  be  replaced  respectively  by  p  and  2p. 
See  the  note  t  of  §  259. 


262]  RIEMANN-ROCH   THEOREM    FOR    FACTORIAL   FUNCTIONS.  405 

261.  We  enquire  now  how  many  arbitrary  constants  enter  into  the 
expression  of  a  factorial  function  of  the  primary  system  which  has  M 
poles  of  assigned  position. 

Supposing  one  such  function  to  exist,  denote  it  by  FQ;  then  the  ratio  F/F0, 
of  any  other  such  function  to  F,  F0,  is  a  rational  function  with  poles  at  the 
zeros  of  F0 ;  conversely  if  R  be  any  rational  function  with  poles  at  the  zeros 
of  F0,  F0R  is  a  factorial  function  of  the  primary  system  with  poles  at  the 
assigned  poles  of  F0.  The  function  R  contains 

N-p+ 1+h+l 

arbitrary  constants,  one  of  them  additive,  where  N  is  the  number  of  zeros  of 

k 
F0>  so  that  N=M  +  2  \r,  and  h  +  l  is  the  number  of  differentials  dv  vanish- 

r=l 

ing  in  the  zeros  of  FQ. 

But  in  fact  the  number  of  differentials  dv  vanishing  in  the  zeros  of  F0  is 
the  same  as  the  number  of  differentials  dV  vanishing  in  the  poles  of  F0,  V 
being  any  everywhere  finite  factorial  integral  of  the  associated  system. 

For  if  dv  vanish  in  the  zeros  of  F0>  the  integral  ldv/FQ  is  clearly  a  factorial 

integral,  V,  of  the  associated  system  without  infinities,  and  such  that  dV 
vanishes  in  the  poles  of  F0 ;  conversely  if  V  be  any  factorial  integral  of  the 
associated  system  such  that  dV  vanishes  in  the  poles  of  FQ,  the  integral 

lF0dV  is  an  integral  of  the  first  kind,  v,  such  that  dv  vanishes  in  the  zeros 

QfJt 

Thus,  the  number  of  arbitrary  constants  in  a  factorial  function  of  the 
primary  system,  with  M  given  arbitrary  poles,  is 

k 

M+  2  \r-p+I+h  +  l,  =N-p  +  i+h+  1,  =M-*r'  +  h  +  I+<r'+l 

r=\ 

where  N  is  the  number  of  zeros  of  the  function,  and  h  +  l  the  number  of 
differentials  dV  vanishing  in  the  M  poles*. 

In  particular,  putting  M=0,  h .  +  1  =  *r'  (cf.  §  258),  we  have  the  formula, 

already  obtained, 

k 
o-'+l=  2  \r-p +  !+-&'. 

r=1 

We  can  of  course  also  obtain  these  results  by  considering  the  fundamental 
equations  (i)  and  (ii),  §  254. 

262.  Hence  we  can  determine  the  smallest  value  of  M  for  which  a 
factorial  function  of  the  primary  system  with  M  given  poles  always  exists. 

*  Counting  the  additive  constant  in  the  expression  of  a  rational  function,  the  last  formula 
holds  in  the  ordinary  case. 


406  FACTORIAL    FUNCTION    WITH    FEWEST    ARBITRARY   POLES.  [262 

When  M  =  •&'  +  1  it  is  not  possible  to  determine  a  function  V,  of  the 
form 


wherein  A1}  ...,  A^>  are  constants,  to  vanish  in  M  arbitrary  places;  and 
therefore  h  +  1  =  0.  Thus  a  factorial  function  of  the  primary  system  with 
-OT'  +  1  arbitrary  poles  will  contain,  in  accordance  with  the  formula  of  the 

last  Article, 

fc 

*r'  +  l  +    S    Xr-p  +  1,    =  <r'+2, 
r=l 

arbitrary  constants. 

When  a'  +  1=0,  this  number  is  1,  and  the  factorial  function  is  entirely 
determined  save  for  an  arbitrary  constant  multiplier.  Hence  we  infer  that 
when  a-'  +  1  =  0  the  smallest  value  of  M  is  CT'  +  1. 

We  consider  in  the  next  Article  how  to  form  the  factorial  function  in  ques 
tion  from  other  functions  of  the  system.  Of  the  existence  of  such  a  function 
we  can  be  sure  a  priori  by  the  formulae  (i)  (ii)  of  §  254.  Such  a  function 
will  have  N  =  •&'  +  1  +  Sx,  =p,  zeros.  They  can  be  determined  to  satisfy  the 
equations  (ii).  Then  an  expression  of  the  function  is  given  by  the  general 
formula  of  §  254. 

When  a'  +  I  >  0,  there  are  a  +  1  everywhere  finite  factorial  functions 
Kl}  ...,  KS+I,  of  the  primary  system,  and  the  general  factorial  function  with 
TV'  +  1  poles  is  of  the  form 


where  \  ,  ...,  X^+j  are  constants,  and  F  is  any  factorial  function  with  the 
assigned  poles.  In  this  case  also  there  exist  no  factorial  functions  with 
arbitrary  poles  less  than  is'  +  1  in  number  ;  the  attempt  to  obtain  such 
functions  leads*  always  to  a  linear  aggregate  of  Klt  ...,^T<r'+1. 

263.     Suppose   that    a'  +  1  =  0  ;    we   consider   the   construction   of    the 
factorial  function  of  the  primary  system  with  •&'  +  1  arbitrary  poles. 

Firstly  let  a  +  1  >  0,  so  that  there  are  cr  +  1  everywhere  finite  functions, 
K',   of    the   associated   system,   and   cr  +  1    differentials   dv   vanish   in   the 

k  k 

2p  —  2  +  2  (Xf  +  1)  zeros  of  any  differential  dV.     Hence  s,  =  —  2  (Xr+l), 

r=l  r=l 

is  greater  than  zero  or  equal  to  zero.     We  take  first  the  case  when  s  >  0. 

* 
Then  ^'=p  —  I—  2  \  =p  —  1  +  s  +  k,  and  it  is  possible  to  determine  a 

r=l 

rational  function  with  poles  at  -57'+  1  =p  +  s  +  k  arbitrary  places.  This 
function  contains  s  +  k  +  1  arbitrary  constants,  one  of  these  being  additive. 
It  can  therefore  be  chosen  to  vanish  at  the  places  clt  ...,  ck>  and  will  then 

*  For  J/  =  •or'  -  r,  we  shall  have  h  +  1  =  r,  and,  therefore,  M  -  &'  +  h  +  1  +  a'  +  1  =  <r'  +  1. 


264]  METHODS    FOR   CONSTRUCTING    THIS    FUNCTION.  407 

contain  at  least,  and  in  general,  s+I  arbitrary  constants.  Taking  now  any 
everywhere  finite  factorial  function  K'  of  the  associated  system,  let  the 
rational  function  be  further  chosen  to  vanish  in  the  s  zeros  of  K'  ;  then  the 
rational  function  is,  in  general,  entirely  determined  save  for  an  arbitrary 
constant  multiplier.  Denote  the  rational  function  thus  obtained  by  R. 
Then  RjK'  is  a  factorial  function  of  the  primary  system  with  the  -a'  4-  1 
assigned  poles,  and  is  the  function  we  desired  to  construct.  And  since  the 
ratio  of  two  functions  K'  is  a  rational  function,  it  is  immaterial  what  function 
K'  is  utilised  to  construct  the  function  required. 

This  reasoning  applies  also  to  the  case  in  which  <r  +  l  >0,  s  =  0,  unless 
also  k  =  0.  Consider  then  the  case  in  which  a  +  1  >  0,  s  =  0  and  k  =  0. 
There  is  (§  258)  only  one  function  K',  of  the  form 

-a+  ......  +  (hp  +  Hp)  vx;  "•] 

, 

or  or  -f  1  =  1  ;  and  E0~l  is  a  function  of  the  primary  system  without  poles. 
Thus  a'  +  1  =  1,  and  the  case  does  not  fall  under  that  now  being  considered, 
for  which  a  +  I  =  0.  The  value  of  w'  is  p,  and  the  factorial  function  with 
•BT'  +  1  arbitrary  poles  is  of  the  form  (F  +  C)  E0,  where  F+  C  is  the  general 
rational  function  with  the  given  poles. 

Nextly,  let  cr  +  1  =  0,  as  well  as  <r'  +  1  =  0.  Then  there  exist  no  functions 
K'  and  the  previous  argument  is  inapplicable.  But,  provided  OT'  +  1  <fc  2,  we 
can  apply  another  method,  which  could  equally  have  been  applied  when 
o-  +  1  >  0.  For  if  P  be  the  factorial  function  of  the  primary  system  with 
is'  +  1  assigned  poles,  and  V  be  one  of  the  CT'  factorial  integrals  of  the 

associated  system,  and  v  be  any  integral  of  the  first  kind,  P  —,     is  a  rational 

function  whose  poles  are  at  the  w'  +  1  poles  of  P  and  at  the  2p  —  2  zeros  of 
dv.  Conversely,  if  R  be  any  rational  function  with  poles  at  these  places 

(c£§37,  Ex.  ii.  Chap.  III.),  and  zeros  at  the  2p  -  2  -  2\  zeros  of  dV,  R\dJ 

I  civ 

is  the  factorial  function  required.     It  contains  at  least 


arbitrary  constant  multiplier. 

In  case  *r'  +  1  <  2,  so  that  «•'  =  0,  S\  =  p  -  1,  there  are  no  functions  V, 
and  we  may  fall  back  upon  the  fundamental  equations  of  §  254.  In  this  case 
the  least  number  of  poles  is  1. 

264.  Consider  now  the  possibility  of  forming  a  factorial  integral  of  the 
primary  system  whose  only  infinities  are  poles.  We  shew  that  it  is  possible 
to  form  such  an  integral  with  <r  +  2  arbitrary  poles,  and  with  no  smaller 
number. 


408  CONSTRUCTION    OF   THE    FACTORIAL    INTEGRAL  [264 

Suppose  G  to  be  such  a  factorial  integral,  with  <r  +  2  poles,  and,  under  the 
hypothesis  CT  >  0,  let  V  be  an  everywhere  finite  factorial  integral,  also  of  the 
primary  system.  Then  dG/dV  is  a  rational  function,  with  poles  at  the 
2p  -  2  +  2(A  +  1)  zeros  of  dV,  and  poles  at  the  poles  of  G]  near  a  pole 
of  G,  say  c,  the  form  of  dG/dV  is  given  by 


where  t  is  the  infinitesimal  for  the  neighbourhood  of  the  place  c,  the 
quantities  0,  A,  B  are  constants,  and  DCV  denotes  a  differentiation  in  regard 
to  the  infinitesimal  ;  this  is  the  same  as 


-r     —  E\—-  +  -     °      +  terms  which  are  finite  when  t 


=  0    , 


where  E  =  —  C/DCV.     Thus  dG/dV  is  infinite  at  a  pole  of  G  like  a  constant 
multiple  of 

.        nr«*>a     DC*V    x,a 

y  =  DCl-C         -    p~y    I  C        , 

a  being  an  arbitrary  place. 

Conversely  if  R  denote  a  rational  function  which  is  infinite  to  the  first 
order  at  the  zeros  of  d  V,  and  infinite  in  the  a-  +  2  assigned  poles  of  G  like 

functions  of  the  form  of  ty,  \RdV  will  be  such  a  factorial  integral  as  desired. 

J 

Now  R  is  of  the  form  (§  20,  Chap.  II.) 


e>  a   ,     ft    FT-)     -p*.  a        DXl  V     x,  a\ 
L  "*i  '         '    J 

|~  ,a         D*<r+2V     x,a  1 


wherein  a  is  an  arbitrary  place,  e1}  ...,  er  denote  the  zeros  of  dV,  x-^,  ...,  xy+n 
denote  the  assigned  poles  of  G,  and  A,  A1}  ...,  Ar,  Blt  ...,  Bv+.2  are  constants; 
the  period  of  R,  in  this  form,  at  a  general  period  loop  of  the  second  kind,  is 
given  by 

-O-iiij  \@i)  "T" T  -^-r^^i  \^r)    '    -^ 


where  ^(x),  ...,  Qp(x)  are  as  in  §  18,  Chap.  II.,  and  this  must  vanish  for 
i  =  l,  2,  ...,  p.  Now  (§  258)  in  the  places  el}  ...,  er  there  vanish  a  +  1  linear 
functions  of  f^  (x),  ...,  O^  (a;).  Thus,  from  the  conditions  expressing  that  the 
periods  of  R  are  zero,  we  infer  a  + 1  linear  equations  involving  only  the 
constants  Blt  ...,  Ba+2,  which,  since  the  places  oelt  ...,  ov+a  are  arbitrary,  may 
be  assumed  to  be  independent.  From  these  cr  +  1  equations  we  can  obtain 


265]  WITH    FEWEST    ARBITRARY   POLES.  409 

the   ratios   Bl:Bz:  ......  :  B^2.     There   remain   then,    of    the    p    equations 

expressing  that  the  periods  of  R  are  zero,  p  —  (cr  +  1)  independent  equations 
containing  effectively  r  +  1  unknown  constants.  Thus  the  number  of  the 
constants  Alt  ...,  Ari  Blt  ...,  B^  left  arbitrary  is  r+  1  -p  +  a-  +  I,  which  is 
equal  to  2p  -2  +  2  (X  +  !)  +  !—  p  +  a  +  1  or  tzr,  and  the  total  number  of 
arbitrary  constants  in  R  is  CT  +  1.  Thus  we  infer  that,  on  the  whole,  G  is  of 
the  form* 


where  [G]  is  a  special  function  with  the  cr  +  2  assigned  poles,  multiplied  by 
an  arbitrary  constant,  and  Glt  ...,  G^  ,  G  are  arbitrary  constants.  And  this 
result  shews  that  cr  -f  2  is  the  least  number  of  poles  that  can  be  assigned  for 
G.  The  argument  applies  to  the  case  when  cr  +  1  =  0  provided  that  w  >  0. 

The  proof  just  given  supposes  w  >  0  ;  but  this  is  not  indispensable. 
Let  f0  be  a  factorial  function  with  the  primary  system  of  multipliers  but 
with  a  behaviour  at  the  places  c;  like  t~(^+1)(j>ii  where  fa  is  uniform,  finite 

and  not  zero  in  the  neighbourhood  of  a.  Then  if,  instead  of  IRdV,  we 
consider  an  integral  IRfodv,  wherein  dv  is  the  differential  of  any  Riemann 


integral  of  the  first  kind,  and  R  is  a  rational  function  which  vanishes  in  the 
(say  M)  poles  of /0,  and  may  become  infinite  in  the  zeros  of  dv  and  the 
(say  N)  zeros  of  f0i  we  shall  obtain  the  same  results.  It  is  necessary  to 
take  N>  1  (cf.  §  37,  Ex.  ii.  Chap.  III.). 

265.  Another  method,  holding  whether  -sr  =  0  or  not,  provided  a  +  1  >  0, 
may  be  indicated.  Let  K'(x)  be  one  of  the  everywhere  finite  factorial  func 
tions  of  the  associated  system.  Consider  the  function  of  x, 


a,  c,  7  being  any  places  and  A  a  constant ;  when  x  is  in  the  neighbourhood 
of  the  place  c  it  is  of  the  form 


l_  \     X        _l     t_  — I 

where  t  is  the  infinitesimal  in  the  neighbourhood  of  the  place  c,  and  terms 
which  will  lead  only  to  positive  powers  of  t  under  the  integral  sign  are 
omitted ;  this  is  the  same  as 


*  In  the  ordinary  case  of  rational  functions,  where  V  is  replaced  by  a  Rieinann  normal  inte 
gral  v,  the  coefficients  of  #,,  ... ,  B<r+2,  in  the  expression  for  the  general  period  of  R,  vanish  for 
one  value  of  i,  namely  when  V=v(.  Thus  o-  +  l(  =  l)  pole  is  sufficient  to  enable  us  to  construct 
the  factorial  integral ;  it  is  the  ordinary  integral  of  the  second  kind. 


410  SIMPLIFICATION    OF   THE    INTEGRAL  [265 

hence  if  A  be  DK\c)/K'(c),  the  function  i/r  is  infinite  at  c  like  -  -  ™ 


-  ™  — 

t  K  (c) 

A 

At  the  place  7  the  function  ty  is  infinite  like  -  JJTT-^  log   ty,  where    ty    is 
the  infinitesimal  in  the  neighbourhood  of  the  place  7. 

Putting  now  M*]*  =  1^'  a  +         ^  IlJ  ",  consider  the  function 

K  (C) 


A          */ix>  a  ,     n    x>a  -n     x 

+  A*+*M*r+z,v  +  B^     +•••  +  BPVP 

where  a,  7  are  arbitrary  places  and  A^...,  Aa+t,  Bl}...,  Bp  are  constants, 
subject  to  the  conditions 

(i)     that 

AlDxMxx["y  +  ......  +  A9+iD,M2^ty  +  BA(x)+  ......  +  Bpflp(a>) 

vanishes  at  each  of  the  -  2  (X  +  1)  zeros  of  K'(x), 

(ii)  that 

DK'(*d  DK'(x<r+.) 

1  ZW'       A'+9  K'(a,.+t)  =  °' 

the  first  condition  ensures  that  G(x}  is  finite  at  the  zeros  of  K'(x),  the 
second  condition  ensures  that  G(x)  is  finite  at  the  place  7.  If  we  suppose* 

vi  ,-•>  v&a  to  be  those  integrals  of  the  first  kind  whose  differentials 
vanish  at  the  zeros  of  K'(x)  (§  258),  the  conditions  (i)  will  involve  only  the 
constants  A1}  ...,  Aa+z,  B^+l,  ...,  Bp>  and  if  these  conditions  be  independent 
these  a-  +  2  +  (p  —  w)  coefficients  will  thereby  be  reduced  to 

>sr  +  2(\  +  l),  =  2  ; 


thus,  if  the  condition  (ii)  be  independent  of  the  conditions  (i),  the  number 
of  constants  finally  remaining  isw  +  2  —  l=«r  +  l,  and  the  form  of  G(x}  is 

[G]  +  C1V1  +  ......  +  CWV^  +  C 

as  before. 

Ex.     Prove  that,  when  s,  =  -  2  (X  +  1  ),  is  positive,  we  have 


266.  The  factorial  integral  of  the  primary  system  with  o-  +  2  arbitrary 
poles  can  be  simplified.  If  a;1,  ...,  av+2  be  the  poles,  its  most  general  form 
may  be  represented  by 


*  This  is  to  simplify  the  explanation.  In  general  it  is  tzr  linear  combinations  of  the  normal 
integrals,  whose  differentials  vanish  in  the  zeros  of  K'(x).  The  reduction  corresponding  to  that  of 
the  text  is  then  obtained  by  taking  or  linear  combinations  of  the  conditions  (i). 


267]  IN    ANALOGY    WITH    THE    ORDINARY    CASE.  411 

where  E,  Elt  ...,  E^,  C  are  arbitrary  constants.     Near  a  place  clt  one  of  the 
singular   places    of   the    factorial   system,   the   integral    will   have   a   form 
represented   by  A^  +  £~A>  <f>  ;   we  may  simplify  the   integral  by  subtracting 
from    it    the    constant    A^,    the    consequence    is    that    the    additive    period 
belonging  to  the  loop  (7^  is  zero  ;  further  there  is  one  other  linear  relation 
connecting   the   additive   periods   of  the   integral,  which   is   obtainable  by 
following  the  value  of  the  integral  once  round  the  boundary  of  the  dissected 
surface  (cf.  §  260).      Thus   the  number  of  periods   of  the   integral   is   at 
most    2p  —  2  +  k.      We    suppose    the    additive    periods    of    the   functions 
G  (xl  ,  .  .  .  ,  av+2),  y\  ,  •••,  Vw  ,  at  the  loop  (71),  to  be  similarly  reduced  to  zero  ; 
then  the  constant  C  is  zero.     The  linear  aggregate  E1V1  +  ......  +  E^  V^ 

may  be  replaced  by  an  aggregate  of  the  non-periodic  functions  Klt  ...,  K^+i, 
and  Br-(<r'  +  l)  of  the  integrals  F,,...,  FOT,  so  that  the  integral  under 
consideration  takes  the  form 


EG  fa,  ...,  av+a)  +  CM  +  ...  4-  CW-((r<+1)  FOT_((r.+1) 

where  C1}  ...,  C^-^'+D,  Flt...,  F^+i  are  constants.  We  can  therefore,  pre 
sumably,  determine  the  constants  Cl}...,  C^_  („.•+!),  so  that  sr  —  (a-'  +  1)  of 
the  additive  periods  of  the  integral  vanish.  The  integral  will  then  have 
2p  —  2  +  k  —  (w  —  a-'  —  1),  =  CT'  —  (a-  +  1),  periods  remaining,  together  with  one 
period  which  is  a  linear  function  of  them.  A  particular  case*  is  that  of 
Riemann's  normal  integral  of  the  second  kind,  for  which  there  are  p  periods. 
As  in  that  case  we  suppose  here  that  the  period  loops  for  which  the  additive 
periods  of  the  factorial  integral  shall  be  reduced  to  zero  are  agreed  upon  before 
hand.  We  thus  obtain  a  function 


wherein  F,  Fly  ...  ,  F^+i  are  arbitrary  constants,  and  G^  (a-j.  ...,  xff+.i)  has 
additive  periods  only  at  CT'  —  (cr  +  1)  prescribed  period  loops,  beside  a  period 
which  is  a  linear  function  of  these.  We  may  therefore  further  assign  <r'  +  1 
zeros  of  the  integral  and  choose  F  so  that  the  integral  is  infinite  at  a\ 
like  the  negative  inverse  of  the  infinitesimal.  When  the  integral  is  so 
determined  we  shall  denote  it  by  F(a;1,  a;.,,  ...  ,  av+g).  The  assigned  zeros  are 
to  be  taken  once  for  all,  say  at  aly  ...,  <v+1. 

267.  The  factorial  function  of  the  primary  system  with  -or'  +  1  assigned 
arbitrary  poles  can  be  expressed  in  terms  of  the  factorial  integral  of  the 
primary  system  with  <r  +  2  assigned  poles.  Let  xly  ...,  xw>+l  be  the  assigned 
poles  of  the  factorial  function.  Then  we  may  choose  the  constants  C\  ,  ..., 
G-aj'-a,  so  that  the  •&'  —  (a-  +  1)  linearly  independent  periods  of  the  aggregate 


are.  all  zeros.     The  result  is  a  factorial  function  with  xl  ,  .  .  .  ,  av+1  as  poles, 

*  Of  the  result.     The  reasoning  must  be  amended  by  the  substitution  of  p,  2p  for  -as'  -  (a  +  1) 
and  2p  -  2  +  k  respectively.     Cf.  the  note  t  of  §  260. 


412  EXPRESSION    OF   THE   FUNDAMENTAL    FACTORIAL   FUNCTION  [267 

which  vanishes  in  the  places  a1}  ...,  cv+1.  Or,  taking  arbitrary  places 
d1  ,  ...,  da+l  we  may  choose  the  constants  El}  .  .  .  ,  EW>+1  so  that  the  w'  —  (a  +  1) 
linearly  independent  periods  of  the  aggregate 


ElY(xl,  dl}  ...,  d<T+1)  +  E2T(x2,d1,  ...,d.+l)  +  . 

are  all  zero,  and  at  the  same  time   the   aggregate   does   not   become   in 
finite  at  di,  ...,dv+1.     Then   the  addition,  to  the   result,  of  an  aggregate 
F1K1  +  ......  +  Fa'+1K0'+1,  wherein  Fl}  ...,  F^+l  are  arbitrary  constants,  leads 

to  the  most  general  form  of  the  factorial  function  with  xl}  ...,  xw'+l  as  poles. 
For  the  sake  of  defi  niteness  we  denote  by  ty  (x  ;  z,  tlt  .  .  .  ,  tw>}  the  factorial 
function  with  poles  of  the  first  order  at  z,  t1}  ...,  t&>,  which  is  chosen  so  that 
it  becomes  infinite  at  z  like  the  negative  inverse  of  the  infinitesimal,  and 
vanishes  at  the  places  a^,  ...,  aa>+1.  A  more  precise  notation  would  be* 
^r  (x,  alt  .  .  .  ,  <v+1  ;  z,  t1}  .  .  .  ,  t&>).  This  function  contains  no  arbitrary  constants. 
Denoting  this  function  now,  temporarily,  by  -fy,  and  any  everywhere 
finite  factorial  integral  of  the  inverse  system  by  V,  the  value  of  the  integral 
fydV,  taken  round  the  boundary  of  the  dissected  surface  formed  by  the 
sides  of  the  period  loops,  is  equal  to  the  sum  of  its  values  round  the  poles 
of  i|r.  Since  ^dV/dx  is  a  rational  function  the  value  of  the  integral  taken 
round  the  boundary  is  zero.  Near  a  pole  of  ^r,  at  which  t  is  the  infinitesimal, 
the  integral  will  have  the  form 


where  D  denotes  a  differentiation.  Thus  the  value  obtained  by  taking  the 
integral  round  this  pole  is  A  (DV).  If  then  the  values  of  A  at  the  poles 
Fn  ...,  FOT'  be  denoted  by  Alt  .  ..,  A^,  we  have,  remembering  that  the 
value  of  A  at  z  is  —  1,  the  -nr'  equations 


A, 

where  F/,  ...,  V'w'  are  the  •or'  everywhere  finite  factorial  integrals  of  the 
associated  system,  (DF/)r  denotes  the  differential  coefficient  of  F/  at  tr,  and 
(DVt\  denotes  the  differential  coefficient  at  z.  Thus,  if  wr(x)  denote,  here, 
the  linear  aggregate  of  the  form 


wherein  the  constants  Elt  ...,  E^>  are  chosen  so  that  wr(tr)  =  1  and  wr(ts)  =  0 
when  ts  is  any  one  of  the  places  ^,  ...,  t^>  other  than  tr,  we  have  Ar  =  o)r(z). 
Hence  we  infer  by  the  previous  article  (§  266)  that  ty(x\  z,t1}  ...,  tw<)  is 
equal  to 

T(z,dlt  ...,C?(T+])-WI(^)  F(^,  d1}  ...,  dc+1)-  ......  -a)w>(z)r(t^'ydl)  ...,d0+1), 

*  Cf.  §  122,  Chap.  VII.  etc. 


268]  BY   MEANS   OF   THE    FUNDAMENTAL    FACTORIAL   INTEGRAL.  413 

where  dl}  ...,  da+l  are  arbitrary  places.     For  these  two  functions  are  infinite 
at  the  places  z,tlt  ...,  tw>  in  the  same  way  and  both  vanish  at  the  places 

ttl,   ...,  &0'+\' 

As  in  the  case  of  the  rational  functions,  the  function  ty  (#;  z,  ti,  ...,  £OT') 
may  be  regarded  as  fundamental,  and  developments  analogous  to  those  given 
on  pages  181,  189  of  the  present  volume  may  be  investigated.  We  limit 
ourselves  to  the  expression  of  any  factorial  function  of  the  primary  system  by 
means  of  it.  The  most  general  factorial  function  with  poles  of  the  first 
order  at  the  places  ^  ,  .  .  .  ,  zm  may  be  expressed  in  the  form 


where  A1}  .  ..,  Au,  Blt  ...,  B^+l  are  constants.  The  condition  that  the 
function  represented  by  this  expression  may  not  be  infinite  at  tr  is 

A1a>r(z1)+  ......  +Ajrur(zM)=0; 

in  case  the  ta  equations  of  this  form,  for  r  =  1,  2,  ...,  CT',  be  linearly  indepen 
dent,  the  factorial  function  contains  M  +  a-'  +  1  —  m'  arbitrary  constants; 
but  if  there  be  h  +  1  linearly  independent  aggregates  of  differentials,  of  the 
form 

C1dVl'  +  ......  +  CW'dFV, 

which  vanish  in  the  M  assigned  poles,  then  the  equations  of  the  form 
A1a>r(z1)+ 


are  equivalent  to  only  vr'  —  (h  +  l)  equations,  and  the  number  of  arbitrary 
constants  in  the  expression  of  the  factorial  function  is  M  +  cr'  +  1  —  vrf  +  h  +  1, 
in  accordance  with  §  261. 

Ex.  i.     Prove  that  a  factorial  integral  of  the  primary  system  can  be  constructed  with 
logarithmic  infinities  only  in  o-  +  2  places,  but  with  no  smaller  number. 

Ex.  ii.     If  the  factorial  integral  Q  (x^  x%,  ...  ,  #<r  +  2)  become  infinite  of  the  place  xt  like 
j  ,  where  t  is  the  infinitesimal  at  x^  prove,  by  considering  the  contour  integral  \GdKr', 

where  A',.'  is  one  of  the  a-  +  1  everywhere  finite  factorial  functions  of  the  associated  system, 
and  0  denotes  G  (xlt  x2,  ...  ,  #<r  +  2)j  the  <r  +  1  equations 

^ 


D  denoting  a  differentiation.     From  these  equations  the  ratio  of  the  residues  R1,  R9,  ..., 
Ra  +  2  can  be  expressed. 

268.  The  theory  of  this  chapter  covers  so  many  cases  that  any  detailed 
exhibition  of  examples  of  its  application  would  occupy  a  great  space.  We 
limit  ourselves  to  examining  the  case  p  =  0,  for  which  explicit  expressions  can 
be  given,  and,  very  briefly,  two  other  cases  (§§  268  —  270). 


414  THE   GENERAL   THEORY   TESTED  [268 

Consider  the  case  p  =  0,  k  =  3,  there  being  three  singular  places  such  as 
have  so  far  in  this  chapter  been  denoted  by  clt  C2,  ...,  but  which  we  shall 
here  denote  by  a,  /3,  7,  the  associated  numbers*  being  \l  =  —  3/2,  X2  =  —  3/2, 
\2  =  —  2.  At  these  places  the  factorial  functions  of  the  associated  system 
behave,  respectively,  like  t~^(j)ly  t~^2,  t~l<f>z,  and  the  difference  between  the 
number  of  zeros  and  poles  of  such  a  function  is  N'  —  M'  =  —  2  (X  +  1)=  2. 
Thus  there  exist  factorial  functions  of  the  associated  system  with  no 
poles  and  two  zeros.  By  the  general  formula  of  §  254,  replacing  11*'"  by 

(CC  ~~  G  I  Ct  ~~  G\ 
-  I  -  1  ,  the  general  form  of  such  a  function  is  found  to  be 
as-yi  a  -  7/ 

+  Bx  +  C 


= 
(x-rix-ax- 

and  involves  three  arbitrary  constants,  so  that  a  +  1  =  3.  In  what  follows 
K'  '  (x)  will  be  used  to  denote  the  special  function  l/(x  —  y)(a;  —  OL^(X  —  /3)i 
The  difference  between  the  number  of  zeros  and  poles  of  factorial  functions 
of  the  primary  system  is  N  —  M  =  —  o  ;  hence  M=Q  is  not  possible,  and 
a-'  +  1  =  0.  Further 

OT  ,  =  p  _  1  +  £  (\  +  1)  +  <r  +  1,  =-1-2  +  3  =  0, 
or',  =p-l-2\  +  <r'  +  l  ,=-1  +  5         =4, 

and  the  factorial  function  of  the  primary  system  with  fewest  poles  has 
•BT'+  1  =  5  poles,  as  also  follows  from  the  formula  N—  M  =  —  5.  This  function 
is  clearly  given  by 

(x- 

(x  —  x-i)  (x  —  x2)  (x  —  x3)  (x  —  #4)  (x  —  xs)  ' 
Putting 

i/r  (x}  =  (x-a.)(x-  0)  (x  -  7),  f(x)  =  (x-  tfj)  (as  -  x2)  (x  -  x3)  (x  -  xt)  (x  -  #5), 
<£  O)  =  DK'  (x)IK'  (x}  =  -[(oc-  7)-1  +  i  (x  -  a)"1  +  £  (x  -  P)'1], 

and  putting  A,,-  =  ty  («»)/./"  O^f)*  where  i  is  in  turn  equal  to  1,  2,  3,  4,  5  and 
f'(x}  denotes  the  differential  coefficient  of  f(x),  it  is  immediately  clear  that 
P(x)  is  infinite  at  x^  like  Xj/(#  —  x-^  K'  (x^  It  can  be  verified  that 

2\!  =  0,  i^^^l,  i^1\1</>(a;1)  =  0,  ^scl-\l(j)(xl}=  -2,  SX10(^1)  =  0, 
111  i  i 

and  these  give 

1  X,  [1  +  x^  (x,)}  =  0,  i\,  [2^  +  xty  (x,)]  =  0. 
i  i 

The   factorial   integral  G,  of  the  primary  system,  with  <r  +  2  =  4  poles, 
T,  £,  77,  £,  is  (§  265)  given  by 


*  It  was  for  convenience  of  exposition  that,  in  the  general  theory,  the  case  in  which  anjr  of  the 
numbers  X,,  ...  ,  \k  are  integers,  was  excluded. 


268] 


BY   A   CASE    IN    WHICH   THE    DEFICIENCY    IS    ZERO. 


415 


where  the  sign  of  summation  refers  to  r,  %,  77,  £  and  the  constants  Al}  A2, 
A3,  AI  are  to  be  chosen  so  that  (i)  the  expression 

Arf  (r)  +  A2$  (f )  +  A3<j>  (77)  +  A<4>  (£) 

is  zero,  this  being  necessary  in  order  that   G(r,  f,  77,  £)  may  not  become 
infinite  at  the  place  c,  and  (ii)  the  expression 


vanishes  to  the  fourth  order  when  x  is  infinite ;  the  expression  always 
vanishes  to  the  second  order  when  x  is  infinite  ;  the  additional  conditions  are 
required  because  K'  (x)  is  zero  to  the  second  order  when  x  is  infinite. 

Taking  account  of  condition  (i),  we  find,  by  expanding  in  powers  of  - ,  that 

JO 

the  condition  (ii)  is  equivalent  to  the  two 

1  Al  [1  4-  T(f)  (T)]  =  0,     I  A,  [2r  +  T2<£  (T)]  =  0. 
i  i 

Thus,   introducing   the    values   of  A1}   ...,  A4   into    the   expression   for 
G  (T,  g,  77,  £),  we  find,  by  proper  choice  of  a  multiplicative  constant, 

1  $  (T)       /t\      t  \      ( 

±i    (£)>    (^X    ( 


(a;  -  r)2      x  -  r 


1  +  T  </>  (r), 


....ax 


in  which  the  second,  third  and  fourth  columns  differ  from  the  first  only  in 
the  substitution,  respectively,  of  £,  77,  £  in  place  of  T. 

The  factorial   integral   G(r,  g,  77,   £)   thus   determined  can   in   fact   be 
expressed  without  an  integral  sigo.     For  we  immediately  verify  that 


is  equal,  save  for  an  additive  constant,  to 

T-  +  1  +  r0  (r)  +  i  \x  -  7  -  i  (a  +  £)}  0  (T) 


(^a)-  ft) 


)  -  {7 


(T))  +    *7  (a 

x  log  \x  - 
I 


<#>  (T) 


T  —  a      T  — 


xlog 


a;  -  /8)  (r  -a)  +  V(a?  -  a)  (T  - 

Va;—  T 


416 


THE    GENERAL    THEORY    TESTED 


[268 


and,  by  the  definition  of  <f>  (#),  the  coefficient  of  the  logarithm  in  the  last  line 
of  this  expression  is  zero  ;  if  we  substitute  these  values  in  the  expression 
found  for  G  (r,  %,  rj,  £)  we  obviously  have 


7  —  T 


(j)  (T),      .   ,      .   ,      . 


-f  constant,...  (2), 


where  the  second,  third  and  fourth  columns  of  the  determinant  differ  from 
the  first  only  in  the  substitution,  in  place  of  r,  respectively  of  £  V,  £  We 
proceed  now  to  prove  that  this  determinant  is  a  certain  constant  multiple  of 
(x  -  a)  (x  -  ft)  (x  -  fi)/(x  -T)(X-  f  )  (x  -^(x-  £),  where  n  is  determined  by 


4- 

T 


If  we  introduce  constants,  A,  B,  C,  A',  B',  6",  depending  only  on  a,  ft,  7, 
defined  by  the  identities 

2 
Co?  +  Bx  +  A  = n(x 


4 


we  can  immediately  verify  that 

A(j>  (a-)  +  B  [1  +  x$  (x)]  +  C  [2a? 


x  —  a 


'  [1+ 


and  hence  that 


CC  —  T 


thus 


7  —  T 


'  (a  —  r)  (/3  —  T)  x  —  r  ' 
7~T  !        m    f, 


, w2f  -x-     -.  . 

(a  —  T)  (/3  —  T)  x  —  T 

<£(r),  .  ,     .  , 

1-f  T$  (T),  .   ,      .   , 


-f  constant, 
...(3) 


268]  BY   A   CASE   IN   WHICH   THE   DEFICIENCY   IS   ZERO.  417 


now  it  is  clear  from  the  equation  (2)  that  G  (T,  g,  i),  £)/V(#  —  a)  (x  —  /?)  is  of 
the  form  (x,  l\j(x  —  r)(x  —  £)  (x  —  rj)(x  —  £),  where  (x,  I),  denotes  an  integral 
cubic  polynomial;  and  since  l/K'(x)  vanishes  when  a;  =  y,  it  follows  from 
the  equation  (1)  that  the  differential  coefficient  of  G(T,%,V),  £)  vanishes 
when  a"  =  y.  Hence  we  have 


where  //.  is  such  that  the  differential  coefficient  of  this  expression  vanishes 
when  x  =  y,  and  has  therefore  the  value  already  specified,  L  is  a  constant 
whose  value  can  be  obtained  from  the  equation  (3)  by  calculation,  and  M 
is  a  constant  which  we  have  not  assigned.  In  the  neighbourhood  of  the 
place  a,  G  (r,  £,  77,  £)  has  the  form  M  +  L(x-  a)-  [\  +  p  (x  -  a)  +  v  (x-&f  +  ...}, 
and  similarly  in  the  neighbourhood  of  the  place  @.  In  the  neighbourhood 
of  the  place  y,  G  (r,  g,  77,  £)  has  the  form 

N  +  (x  -  7)-  [V  +  //  (a  -7)  +  v'(x-  7)2  +  ......  ]. 

where  N  is  a  constant,  generally  different  from  M. 

In  the  general  case  of  a  factorial  integral  for  p=0,  k=3,  the  behaviour  of  the  integral 
at  a,  /3,  y  is  that  of  three  expressions  of  the  form 


provided  no  one  ofX  +  l,/t  +  l,j/+l  be  a  positive  integer;  herein  one  of  the  constants 
A,  B,  C  may  be  taken  arbitrarily  and  the  others  are  thereby  determined.  The  factorial 
integral  becomes  a  factorial  function  only  in  the  case  when  all  of  A,  B,  C  are  zero. 

We  have  seen  that  the  factorial  function  of  the  primary  system  with 
fewest  poles  has  5  poles  ;  let  them  be  at  T,  rl}  %,  97,  £;  then,  taking  G  (r,  %,  rj,  £) 
in  the  form  just  found,  the  factorial  function  can  be  expressed  in  the  form 

P  (x}  =  CO  (r,  fc  rj,  ^  +  CtG  (TU  fc  77,  0  +  D, 
when  the  constants  C,  Gl}  D  are  suitably  chosen. 

For  clearly  D  can  be  chosen  so  that  the  function  P  (x)  divides  identically 
by  (x  —  af-(x  —  ftf-.  It  is  then  only  necessary  to  choose  the  ratio  G  :  Cl} 
if  possible,  so  that  the  function  P  (x)  divides  identically  by  (x  —  y)-.  This 
requires  only  that 


X-T  l  X  -  T,        ^  (X  -  T)  (X  -  Tj)  ' 

where  p  is  a  constant,  or  that  the  expression 


B.  27 


418  THE   GENERAL   THEORY   TESTED  [268 

divide  by  (x  -  7)-.     Thus  C  :  C,  =  -  (7  -  T)  (7  -  /*,)  :  (7  -  /*)  (7  -  TJ),  and 
27  -  /A  -  TI     _     27  -  /*!  -  r 

(7  -  fl)  (7  -  Tj)        (7  -  /ij)  (7  -  T)  ' 

or 


7  -  /*     7-r     7  -  /*i     7  —  Ti 

this  condition  is  satisfied ;  both  these  expressions  are  by  definition  equal  to 

J_       J_      _J__a'    J      •      J 

«•     I  t»          '2 


From  the  theoretical  point  of  view  it  is  however  better  to  proceed  as 
follows—  Let  the  poles  of  P  (x}  be  at  ar,  ,  .  .  .  ,  <r5.  Then  P  (a-)  can  be  expressed 
in  the  form 

Px  =  ClG(xl,  £  77,  0  +  0,0  (a?3>  £  77,  0+  ......  +CBG(ar0,  fc  17,  0  +  C, 


the  constants  C,  Glt  C.,,  ...,  Cs  being  suitably  chosen.     This  equation  requires, 
by  equation  (1), 


+ 


0,  #,  J7,  S 

r  [1  +  xr<f>  (#,)],        1  4-  ^  (|),        1  +  it  (*)),         1  +  ^  (D 


i 

5 


wherein  A  (£,  77,  £)  is  the  minor,  in  the  determinant  occurring  in  equation  (1), 
of  the  first  element  of  the  first  row,  and  E  =  (x  -  % )~2  +  </>  (£)  (x  -  I)-1, 
F=  (x  -  r})-"  +  <f>  (77)  (x  -  rj)~l,  G  =  (x-  ^)~2  +  <f>  (^)  (^  -  f)-1.  If  now  we  take 
C'j ,  ....  (75  so  that 

55  5 

^  /"'    *Jv  /  /v»  \  —  rt          ^?  t       r  1      l     /y    /"fk  /  *v*    i  I  —  C\       ^^  I  ,     \   s  nr       I     ^  *•  /T\  i  "T*    i  I   ~~*  1 1 
—  *      •  CD  \  w->*  I  —  V/j         .^^l^'i'  I  -L  "T"  vUf^r  \     T/  I  —  ^?       ^*\J '-p  \£t*Asf     i^  tAsj*    \L/  y**/'j*/J   ^^  ^j 

11  i 

this  leads  to 

/  /yi  /y»  /y»  /y>    \       I.     f]      7j  /Jt    /  //»  //»  /V»  0"      I 

l  w/j  j   tX/2  j  ^s  j   *^4/  T^  ^^5-*-^  ^*    V     1 )       2  ?       3  3       5/J 


77,  g 
and  the  solution  can  be  completed  as  before. 

There  are  TS'  =  4  everywhere  finite  factorial  integrals  of  the  associated 

dV  . 
system ;  if  V  be  one  of  these,  then  by  definition,  -^    is  a  factorial  function 


2(59]  BY   A   CASE   IN    WHICH    THE   DEFICIENCY   IS   ZERO.  419 

which  has  at  a  the  form  (x  —  a)~3<£,  and  similarly  at  ft,  and  has  at  7  the 
form  (x  —  y)-2<f>.  Further  dV'jdx  is  zero  to  the  second  order  at  x  =  x  . 
Hence  we  have 

(x,  1)3  cfa 


_    _ 
Jx- 


and  dV  has  2p  —  2  —  t\  =  —  2  +  5  =  3  zeros. 
Thus  V  can  be  written  in  the  form 

dx  La?  +  MX  + 


=  NK'  (x)  +  Mr/  O)  +  £#,'  (a?)  +  ^  F0', 

where  JV,  Jlf,  Z,  .R  are  constants,  K'  (x),  KJ  (x),  K2'  (x)  are  particular,  linearly 
independent,  everywhere  finite  factorial  functions  of  the  associated  system, 
and  FO'  is  a  particular  everywhere  finite  factorial  integral  of  the  associated 
system. 

Ex.  i.     In  case  of  a  factorial  system  given  by  p  =  0,  k  =  2,  Xt=  -f,  X2=  —  f,  prove  that 
<r-M=2,  a-'  +1=0,  or  =  0,  or'  =  2  ;  prove  that  the  factorial  function  of  the  primary  system 

with  fewest  poles  is  P  (x}  =  (x-aft  (x  -  @$l(x  -  x^)  (x-x^  (x-xj)  ;  obtain  the  form  of  the 
factorial  integral  of  the  second  kind  of  the  primary  system  with  fewest  poles,  and  prove 
that  it  can  be  expressed  in  the  form  AP(x)  +  B  ;  and  shew  that  the  everywhere  finite  fac 
torial  integrals  of  the  associated  system  are  expressible  in  the  form  (Ax+B)/\/(x  —  a)  (x  —  ft), 
their  initial  form  being 

(Ax+E)dx 


Ex.  ii.  When  we  take  p  =  Q  and  k,  =2n  +  2,  places  clt  ...,  c2tt+2,  and  each  X=-i, 
prove  that  the  original  and  the  associated  systems  coincide,  that  a  +  1  =  o-'  +  1  =  0,  w  =  •&'  =  n, 
that  the  everywhere  finite  factorial  integrals,  and  the  integral  with  one  pole  are  respec 
tively 

fo!)-irfr  /T/(a)    +i^'(a)1     dx 

J    -JfV)  JL(.'-«)2  +  *^^Jx//^)' 

where  f(x)  =  (x-cl)  ......  (^-c.2)l  +  2).       The    factorial    function    with    fewest    poles    is 

^/  (*)/(-r,  l)»  +  i;  express  this  in  the  form 

•JfW   _»+>       (T  ffa)    ../'(oi)!    dx     Lr(^l)»-x  ,    , 
/_,  i\        =  2  AI  I    -  -----  a+f  —  .  —   +  I  —  V-  —-  dx+  constant, 

(x,  l)n  +  1      ,-=i       j\_(x-ai}i     -  A'-aJv//(.r)      J     v(/(.^) 

a,,  ...  ,  nn  +  1  being  the  zeros  of  (x,  1),,  +  1,  and  determine  the  2?i  +  l  coefficients  on  the  right- 
hand  side. 

269.  One  of  the  simplest  applications  of  the  theory  of  this  chapter  is  to 
the  case  of  the  root  functions  already  considered  in  the  last  chapter  ;  such  a 
function  can  be  expressed  in  the  form  e+,  where 


27—2 


420  EXAMPLE   OF    RADICAL-FUNCTIONS.  [269 

where  /3l5  ...,  /3N  are  the  zeros,  al,  ...,  a.N  the  poles,  h;  is  a  rational  numerical 
fraction,  Hi  is  an  integer,  and  7  is  an  arbitrary  place.  The  singular  places, 
Cj,  ...,Cfc  are  entirely  absent.  The  zeros  and  poles  satisfy  the  equations 
expressed  by 


where  Gl}  ...,  Gp  are  integers;  and  since,  if  m  be  the  least  common  denomi 
nator  of  the  2p  numbers  g,  h,  the  rath  power  of  the  function  is  a  rational 
function,  there  is  no  function  of  the  system  which  is  everywhere  finite, 
and  the  same  is  true  of  the  associated  system.  Hence  er  +  l=0  =  o-'  +  l, 
•sr  =  OT'  =p  —  1  ;  thus  the  function  of  the  system  with  fewest  poles  has 
p  poles,  and  every  function  of  the  system  can  be  expressed  as  a  linear 
aggregate  of  such  functions  (§  267.  Cf.  §  245,  Chap.  XIII.). 

Ex.  i.     Prove  that  when  the  numbers  g,  h  are  any  half-integers,  the  everywhere  finite 
integrals  of  the  system  are  expressible  in  the  form 


„     [ 
V=j 


civ?-1. 
-    S 


where  v  is  an  arbitrary  integral  of  the  first  kind,  (f>  is  the  corresponding  (^-polynomial, 
and  3>t-,  <&i  are  (^-polynomials  with  p  —  1  zeros  each  of  the  second  order  (cf.  §  245, 
Chap.  XIII.).  It  is  in  fact  possible  to  represent  any  half-integer  characteristic  as  the 
sum  of  two  odd  half-integer  characteristics  in  2p~2(2p~1-l)  ways. 

Ex.  ii.     In  the  hyperelliptic  case,  when  the  numbers  g,  h  are  any  half-integers,  prove 
that  the  function  of  the  system  with  07'  + 1  =p  poles  is  given  by 


\f  > 

)} 


where  the  places  (xlt  y±),  ...  are  the  poles  in  question, 

^  (#)  =  (#-  #1)  ...  (%  -  xp),  V/  Or)  =  dty  (x}jdx,  u  =  (x  —  a)  (x  —  6), 
and  a,  b  are  two  suitably  chosen  branch  places*,  and  ui  =  (xi-a)(xi  —  'b').     Shew  that  in 

(T  (it  —  -  1)  l\    "Wi 

the  elliptic  case  this  leads  to  the  function  —  —.  -  r—  e~v  ("~"). 

cr  (u  -  V) 

270.  In  the  case  in  which  the  factors  at  the  period  loops  are  any 
constants,  the  places  c1?  ...,ck  being  still  absent,  it  remains  true  that  the 
number  of  zeros  of  any  function  of  the  system  is  equal  to  the  number  of 
poles;  but  here  there  may  be  an  everywhere  finite  function  of  the  system, 
and  there  will  be  such  a  function  provided 

gi  +  Ti,i  h,+  ......  +Tilphp  =  -[Gi  +  Tiil  H,  +  ......  +  Titp  Hp],  (i  =  l,  2,  ...,p) 

in  which  G1}  ...,  Hp  are  integers,  the  function  being,  in  that  case,  expressed  by 


*  For  the  association  of  the  proper  pair  of  branch  places  a,  b  with  the  given  values  of  the 
numbers  g,  h,  compare  Chap.  XI.  §  208,  Chap.  XIII.  §  245,  and  the  remark  at  the  conclusion  of 
Ex.  i. 


270]  A  MOKE  GENERAL  CASE.  421 

then  E~l  is  an  everywhere  finite  function  of  the  associated  system,  and 
a  +  I  =  a-'  +  1  =  1,  ur  =  CT'  =  p.  It  is  not  necessary  to  consider  this  case,  for 
it  is  clear  that  every  function  of  the  system  is  of  the  form  ER,  R  being  a 
rational  function. 

When  a-  +  1  =  a-'  +  1  =  0  we  have  or  =  p  —  1  =  CT'.  Then  every  function 
of  the  system  can  be  expressed  linearly  by  means  of  functions  of  the  system 
having  p  poles.  If  #, ,  . ..,  xp  be  the  poles  of  such  a  function  and  z1}  ...,  zv  the 
zeros,  and  the  relations  connecting  these  be  given  by 

»*»*>+ +  vz<»x»=f/+G  +  T(h  +  H). 

There  is  beside  the  expression  originally  given,  a  very  convenient  way  of 
expressing  such  a  function,  whose  correctness  is  immediately  verifiable, 
namely 


wherein 


and  m,  mly  ...,mp  are  related  as  in  §  179,  Chap.  X.     Omitting  a  constant 
factor  this  is  the  same  as 


r  v  />     j  » 


<s)  (u) 
since  the  difference  between  the  values  of  the  logarithm  of  <f>  (u)  at  the  two 

sides   of  any  period  loop  is   independent   of  u,  and  of  x,  it  follows  that 

o  p, 

^-  log  </>  (u)  is  a  rational  function  of  x,  and  that  ^-  log  <j>  (u)  is  a  periodic 

function  with   2p  sets   of  simultaneous   periods  ;    thus   the   function   <£  (a) 
satisfies  linear  equations  of  the  form 

^\.7  *o 

W  =  RlJ>    55^  -•B«*          <M  =  1,2,...,,C), 

where  R,  R,j  are  rational  functions  of  x,  and  2/;-ply  periodic  functions  of  u. 
given*  by 


The  2/»  constants  a,  X  can  be  chosen  so  that 


satisfies  the  equations  <£  (M  +  2«)  =  zl^(?«),  </>  (M  +  2»')  =  ^l'0(?0.  whore  .4,  J'  each  represents 
p  given  constants,  and  the  notation  is  as  in  §  189,  Chap.  X. 

*  Cf.  Halphen,  Fonct.  Ellipt.,  Prem.  Part.  (Paris  1886),  p.  235,  and  Forsyth,  Theory  of  Func 
tions,  pp.  275,  285,  for  the  case  p  =  l.  By  further  development  of  the  results  given  in  Chap.  XI. 
of  this  volume,  and  in  the  present  chapter,  it  is  clearly  possible  to  formulate  the  corresponding 
analytical  results  for  greater  values  of  j>. 


422  A   THETA    FUNCTION    OF    GENERAL    ARGUMENT  [271 

271.  We  have  seen  (§  261)  that  the  number  of  arbitrary  constants 
entering  into  the  expression  of  a  factorial  function  of  the  primary  system 
with  given  poles  is  N— jj+l+/i  +  l,  =R  say,  where  N  is  the  number  of 
zeros  of  the  function,  and  JL  + 1  is  the  number  of  linearly  independent 
differentials,  dv,  of  integrals  of  the  first  kind,  which  vanish  in  the  zeros 
of  the  function.  When  h  +  I  vanishes  the  assigning  of  the  poles  of  the 
function,  and  of  R  —  1  of  the  zeros  determines  the  other  N—R  +  l,  =p, 
zeros ;  in  any  case  the  assigning  of  the  poles  and  of  R  —  1  of  the  zeros 
determines  the  other  N  —  R  +  l,  =2)  —  (h+l),  of  the  zeros.  Denote  the 
poles  by  a1}  ...,OLM  and  the  assigned  zeros  by  j31}  ...,  @R-i',  then  the  remaining 
zeros  /3R,  ...,  ftN  are  determined  by  the  congruences 

0i ,«  0/(_i!  «          <*-i,  a  O-M,  a         „  er,  a        ,  ,  ,  . 

Vi         +  . . .  +  Vi  -Vi        -  ...  -  Vi          -    Z    \.Vi        -  (ffi  +  A,  Tit !+...+  IlpT{,p) 

r-l 


a  being  an  arbitrary  place.     Now,  let  the  form  of  the  factorial  function  when 
the  poles  are  given  be 


where  C\,  ...,  CR  are  arbitrary  constants,  and  F1(ac),  ...,  FR(x)  are  linearly 
independent  ;  then,  when  the  zeros  /3U  ...,/3JC_1  are  assigned,  the  function  is  a 
constant  multiple  of  the  definite  function 


the  zeros  of  this  function,  other  than  filt  ...,  fiR-1}  are  perfectly  definite,  and 
are  determined  by  the  congruences  put  down.  Let  H  denote  the  quantities 
given  by 

Hi  =  2  \.vc-'  a  +  gi  +  /tjTt,!  +  ......  +  hpTitp  ; 

r=l 

take  any  places  yl}  ...,  7^+1,  of  assigned  position,  and  take  a  place  m  and  p 
dependent  places  m1}  ...,  mp  defined  as  in  §  179,  Chap.  X.,  and  consider  the 
function  of  # 


if  the  function  does  not  vanish  identically,  its  zeros,  x1}  ...,  xp,  are  (§  179, 
Chap.  X.)  given  by  the  congruences  denoted  by 


'  m*+2 


271]  EXPRESSED   IN    FACTORS.  423 

or,  what  is  the  same  thing,  by 


now,  from  what  has  been  said,  it  follows,  comparing  these  congruences  with 
those  connecting  the  poles  and  zeros  of  A  (x),  that  if  xl}  ...,  xh^  be  taken  at 
7i,  ...,  7/,+i,  these  congruences  determine  xh+y,  ...,xp  uniquely  as  the  places 
&K>  •••>  ftx-  Thus  the  zeros  of  the  theta  function  are  the  places  7lf  ...,  yh+i 
together  with  the  zeros,  other  than  /31}  ...,  yS^_i,  of  the  function  A  (x). 

We  suppose  now  M  to  be  as  great  as  p  —  1,  =  r  +  p  —  1  ,  say  ;  as  in  §  184, 
p.  269,  we  take  nly  ...,  ?ip_j  to  be  the  zeros  of  a  (^-polynomial  of  which  all  the 
zeros  are  of  the  second  order,  so  that 


,  in  _ 


is  an  odd  half-period,  equal  to  £Hgi  s>  say  ;  and  we  take  the  poles  ar+1  ,...,«„  at 
nlt  ...,  Wp_i.     Further*,  in  this  article,  we  denote 

0  (v*>  z  +  ins,  ,.)  e**'*'*  by  X  (x,  z\ 

so  that  (§  175,  Chap.  X.)  \(x,  z)  is  also  equal  to  e-^>+^'>  6(t>*.  *;  i«,  I*'). 
The  function  X  (x,  z)  must  not  be  confounded  with  the  function  X  (£,  /A)  of  §  238. 

Then  in  fact,  denoting  the  arguments  of  the  theta  function  by   V,  we 
have  the  following  important  formula, 

r  h+l  k 

A  (x)  U  X  (a?,  Zj)  U  X  (x,  7j)  II  [X  (x,  C;)]*> 

' 


where  ^.  is  a  quantity  independent  of  a;.  In  order  to  prove  this  it  is 
sufficient  to  shew  (i)  that  the  right-hand  side  represents  a  single-valued 
function  of  x  on  the  Riemann  surface  dissected  by  the  2p  period  loops, 
(ii)  that  the  right-hand  side  has  no  poles  and  has  only  the  zeros  of  @(F), 
and  (iii)  that  the  two  sides  of  the  equation  have  the  same  factor  for  every  one 
of  the  2p  period  loops. 

Now  the  function  X  (x,  z)  has  no  poles  ;  its  zeros  are  the  place  z,  and  the 
places  ?ij,  ...,  np^.     The  places  nl}  ...,  np^l  occur  on  the  right  hand 

(a)    as  poles,  each  once  in  A(#),  each  (R  —  1)  times  in   the  product 


r  h+l 

(p)   as  zeros,  each  r  times  in  II  X  (x,  a,-),  h  +  l  times  in  II  X  (as,  7;),  and 

.7  =  1  j  =  l 

*  For  the  introduction  of  the  function  X  (x,  z)  see,  beside  the  references  given  in  chapter  XIII. 
(§  250),  also  Clebsch  u.  Gordan,  Abel.  Functnen.  pp.  251—256,  and  Riemann,  Math.  Werke  (1870), 
p.  134. 


424  A   THETA   FUNCTION   OF   GENERAL   ARGUMENT  [271 

k  k 

S  \j  times  in  II  [A,  (a,  GJ)]^  ;  thus  these  places  occur  as  zeros,  on  the  right 

.7  =  1  .7  =  1 

hand, 

M-  (p  -  1)  +h+  1+  SX;  -  A  =  -AT-  p  +  1+  h  +  1  -  H, 

times,  that  is,  not  at  all. 

Thus  the  expression  on  the  right  hand  may  be  interpreted  as  a  single- 
valued  function  on  the  Riemann  surface  dissected  by  the  2p  period  loops  — 
for  we  have  seen  that  the  places  nl}  ...,  np_l  do  not  really  occur,  and  the 
multiplicity,  at  c/,  in  the  value  of  such  a  factor  as  \\(x,  c/)]A>  is  cancelled  by 
the  assigned  character  of  the  factorial  functions  F(x)  occurring  in  A(.r). 
Nextly,  the  zeros  of  the  denominator  of  the  right-hand  side,  other  than  at 
MI,  ...,  iip-i,  are  zeros  of  A  (as),  and  the  poles  of  A  (#),  other  than  nlt  ...,  np_l, 

r 

are  zeros  of  the  product  II  \(x,  <Xj),  so  that  the  right-hand  side  remains 

j=i 
finite.     The  only  remaining  zeros  of  the  right-hand  side  consist  of  71,  ...,  yh+1 

and  the  zeros  of  A(#)  beside  &,  ...,  /3^_j  ;  and  we  have  proved  that  these  are 
the  zeros  of  ®  (  V).  It  remains  then  finally  to  examine  the  factors  of  the 
two  sides  of  the  equation  at  the  period  loops.  The  factors  of  the  left-hand 
side  at  the  i-ih  period  loops  respectively  of  the  first  and  second  kind  are 
(see  §  175,  Chap.  X.) 

e  -  27TJ  (hi  -  K)  and  e  ~  2^*    S    (V  -  J«V)  *>,  i  -  2iri  (  Vt  +  K  4). 

the  factor  of  the  right-hand  side  at  the  i-th  period  loop  of  the  first  kind  is 

e*,  where 

I 
^r  =  -  Vnrihi  +  ririsl  +  (h  +  1)  iriSi  +  irisl  2  \j  —  (R-l)  iris-  ; 

;=i 

k 

now  R  =  N  -  p  +  1  +  h  +  1  =  r  +  2  X,-  +  h  +  1  ;  thus  i/r  =  -  2Trih[  +  7m/,  and 

j=i 

e*  =  e-*ri(hi-W)}  or  the  factors  of  the  two  sides  of  the  equation  to  be  proved,  at 
the  i-th  period  loop  of  the  first  kind,  are  the  same.  Since  the  factor  of 
X  (x,  z)  at  the  t'-th  period  loop  of  the  second  kind  is  e^  where 

i'~  +  ^S{  +  faiTi,  1  +  •  •  •  +  s'pTi,  P  +  %ri, 


it  follows  that  the  factor  of  the  right-hand  side  at  the  i-ih  period  loop  of  the 
second  kind  is  ex  where 


[T       r    a  h  +  l     Cf    v  k  R~l      T 

v^'a;+  Svr^+SV?'-   2  v 
j=i  j=i  j=i  j=i 

r  h  -i 

-  iri  \r  +  h  +  1  +  l\j-R+l\  (T/  f  +  A-), 

L  .;=i 


2 


a!,|8. 


272]  EXPRESSED   IN   FACTORS.  425 

now  we  have 


a,,  a  a  ,  a         )i1(a 

-vf      -...-v-J     -Vi 

and 

£  (si  +  S/TI, ,+  ... 
thus 


.7  =  1 

further 

_  x,a       ,,        n  x    a;,  a.       /T3        ^  •.     x,  a  x,  a        ^  ~      x,  a 

0  =  —  Vi      -\-  \ll  -f-  1 )  Vi       —  \l~i  —  i)Vi       -f-  TVi       T    ^  "-jfj       ^ 

hence 

A+l   3.^.      JB-l   a.)  /3.         r     x>  a 


or 

/*  r  h+l  h  B-l 

S(AM-K')^i+^--flr,-  +  i*,-+  2t;?*>+    S  vf  v>  +  S  \X  '  -   ^  v?'*, 

/*  =  !  ./  =  !  ?  =  1  J  =  l  ;'  =  ! 

and  thence  the  identity  of  the  factors  taken  by  the  two  sides  of  the  equation 
to  be  proved,  at  the  t'-th  period  loop  of  the  second  kind,  is  manifest. 

And  before  passing  on  it  is  necessary  to  point  out  that  if  the  functions 

X  (x  z} 
\  (x,  z)  be  everywhere  replaced  by        r—  ,  and  A  (x)  be  replaced  by  i/r A  (x}, 

^r  being  any  quantity  whatever,  the  value  of  the  right-hand  side  of  the 
equation  is  unaltered.  For  there  are  R  factors  A,  (x,  z}  occurring  in  the 
numerator  of  the  right-hand  side  of  the  equation  beside  A  (x),  and  R  —  1 
factors  \(x,  z)  occurring  in  the  denominator  of  the  right-hand  side  of  the 
equation.  In  particular  ty  may  be  a  function  of  x. 

272.  We  can  now  state  the  following  result:  Let  a,  «n  ...,  «r  be  any 
assigned  places;  let  TO,,  n.2,  ...,  ?tj>_1  be  the  zeros  of  a  ^-polynomial,  or  of 
a  differential,  dv,  of  the  first  kind,  of  which  all  the  zeros  are  of  the  second 
order,  and 

>u,,,m         n,,»i,  n,,-i,  mt>-i        ,   , 

Vi  -V{  -...-Vi  =$(si  +  si'T;il+...+Sp/Ti,p),       (l  =  1,  2,  ...,})), 

111,  MI,,  ...,  mp  being  such  places  as  in  §  179,  Chap.  X.;  let  li+l  be  the 
number  of  linearly  independent  differentials,  dv,  which  vanish  in  the  zeros  of 
a  factorial  function  of  the  primary  system  having  cti,  ...,  or,.,  nlt  ...,  np_1  as 


42(j  STATEMENT   OF    THE   RESULT.  [272 

poles,  or   the   number   of  differentials  dV,   of  everywhere   finite   factorial 
integrals  of  the  associated  system,  which  vanish  in  the  places  nlt  ...,  np_1} 

k 

a,,  ...,  a,.;   let  yl,  ...,  yh+i  be  any  assigned  places;   denote  r  +  2  \j  +  h+l 

j=i 
by  R,  and  let*  xl}  ...,  XR  be  any  assigned  places;  let  the  general  factorial 

function  of  the  primary  system  having  a1}  ...,  a.,,  n1}  ...,  »ip_x  as  poles  be 

0^(0,)+ +  CRFR(x), 

wherein  Glt  ...,  GB  are  constants,  and  let 

(X), ,FR(xl]    \^(xl),...,^(xK)) 


,FH(xB} 
where  ty  (x)  denotes  any  function  whatever  ;  let 

7?  y  7i  4-  1  Z- 

Tr          £     x.,a        £     a.,  a       "JT1    y.,a         £          c.,  a 

U{=  2tv    -  2  Vi>'   -  2  v     -  2  \jvf   , 

j  =  l  j=l  j=l  ./  =  ! 

which  is  independent  of  a,  and  let  the  row  of^>  quantities 


i  >  x     ......        p  -     p     it  p 

be   denotedf   by   g-^8  +  r(h-^8')j    then  if,  modifying  the  definition  of 
X  (x,  z\  we  put 


we  have 


A.  (a-     r  r"»       R    (    r  h+l  k 

=  t,j-i,i'  ,2V"        n    n  \(^  «,)  n  x  (^  7j)  n  [x^,,  Cj) 
nri     x  (xit  Xj}  i=l  u=1  •;'=1 

i<j 

wherein  (7  is  a  quantity  independent  of  xlt  ...,  XR,  which  may  depend  on 
Cj,  ...,  Cfc,  «!,  ...,  «,.,  yl}  ...,  7A+1. 

273.  The  formula  just  obtained  is  of  great  generality;  before  passing 
to  examples  of  its  application  it  is  desirable  to  explain  the  origin  of  a  certain 
function  which  may  be  used  in  place  of  the  unassigned  function  ty  (as). 

We  have  (§  187,  p.  274),  in  the  notation  of  §  272, 


if  the  zeros  of  the  rational  function  of  x,  (x1  —  x)j(x'  —  2),  be  denoted  by 

*  These  replace  the  xl,  ft,  ...  ,  ^..j  of  §  271. 
t  So  that  V=  U  -  (g  -  $g)  -  r  (h  -  ^*'). 


273]  THE   SCHOTTKY-KLE1N    PRIME    FORM.  427 

x,  xl,  ...,  c£H_i,  n  being  the  number  of  sheets  of  the  fundamental  Riemann 
surface,  and  the  poles  of  the  same  function  be  denoted  by  z,  zlt  ...,  zn_^  we 
have,  by  Abel's  theorem, 


=  10  ^'-^_lr_ 

now  let  the  places  x,  z'  approach  respectively  indefinitely  near  to  the  places 
x,  z  which,  firstly,  we  suppose  to  be  finite  places  and  not  branch  places ;  then 
the  right-hand  side  of  the  equation  just  obtained  becomes 

log  \_-(x=zY  "  X(cc)X(z) 

where 

p  x  „  v 

\    i  /v»  i „    ^>    (—\    f  1  (~\        \      7~i  ~V  /    \          ^* 

•"^   \ *™ )  —    "^   ^^ /  \  "9"  •* ^x    v'  /  •  -*^ ^/       i        -^*-    \  -^  /  ^~    -  / 

Z)  denoting  a  differentiation,  and  a  denoting  an  arbitrary  place  ;  but  we  have 
(Chap.  X.  §  175) 

thus,  on  the  whole,  when  the  square  roots  are  properly  interpreted,  we 
obtain 

/ —                              — aTz' 
\un.X'=x  , •,__,  \/  —  (x'  —  x) (z'  —  z) e      x>z   =  — *'—"—- 

"V  A/V/\V/\ 

\i  \    i  np  i  \    i^i 
»  -*v  V     /    ^   V    / 


When  the  places  «,  ^  are  finite  branch  places  we  obtain  a  similar  result. 
Denote  the  infinitesimals  at  these  places  by  t,  t1}  and,  when  x,  z'  are  near  to 
as,  z,  respectively,  suppose  of  =  x  +  tw+1,  z  =z  +  ^1+1  ;  then  from  the  equation 
given  by  Abel's  theorem  we  obtain,  if  7  denote  an  arbitrary  place, 


w  r  x'  z1        i      "j:1     v'  /    wi  r  r-  /         i      »-!     -^  ,- 
S   n£;  -  log  d  +    s    nj;,;  +  2    n^;:  -  log  d  +    2    nj^ 

=l  L  J        r=w+l  r=l  L  J        r=w,+l 


where  X  (#),  X  (2)  are  of  the  same  form  as  before,  save  that  the  differentia 
tions  Dvi'  ,  Dvi  ,  are  to  be  performed  in  regard  to  the  infinitesimals  t,  ^. 
If  the  limit  of  the  first  member  of  this  equation,  as  x,  z'  respectively 
approach  to  x,  z,  be  denoted  by  Z,  we  therefore  have 


-  IT*  '  "        H  (vx>  z  -4-  ill      -\ 

**U          +g=  =(x-z)e^  (ii) 

x)  X(z) 


428  THE  SCHOTTKY-KLE1N    PRIME    FORM.  [273 

The  equations  (i),  (ii)  are  very  noticeable  ;  there  is  no  position  of  x  for 
which  the  expression  ®  (vx'  z  +  J  Hg)  g')  .  e^18**'  z/vX  (x)  X  (z)  is  infinite,  and  there 
is  only  one  position  of  so,  namely  when  x  is  at  z,  for  which  the  expression 
vanishes;  for  (§  188,  p.  281)  the  expression  *J  X  (x)  vanishes,  to  the  first 
order,  only  when  x  is  at  one  of  the  places  nlt  ...,  np^,  and  ®  (vx>  z  +  ^£ls,s') 
vanishes  only  when  x  is  at  one  of  the  places  z,  nlt  ...,  np^  ;  there  is  no 
position  of  x  for  which  \/X  (x}  is  infinite.  Putting 

T(x     ._®( 

we  have  further  •GTI  (x,  z}  =  —  TSI  (z,  x},  and  if  t  denote  the  infinitesimal  near 
to  z,  we  have,  as  x  approaches  to  z,  limita;=z  [CTZ  (x,  z)jt\  =  1.  For  every 
position  of  a;  and  z  on  the  dissected  Riemann  surface  •sr1  (x,  z)  has  a  perfectly 
determinate  value,  save  for  an  ambiguity  of  sign,  and,  as  follows  from 
the  equations  (i),  (ii),  this  value  is  independent  of  the  characteristic 

(H  iO- 

There  are  various  ways  of  dealing  with  the  ambiguity  in  sign  of  the 
function  tal  (x,  z).  For  instance,  let  (f>  (x)  be  any  ^-polynomial  vanishing  in 
an  arbitrary  place  m,  and  in  the  places  A1}  ...,  A.2p_3  (cf.  §  244,  Chap.  XIII.), 
and  let  Z  (x)  be  that  polynomial  of  the  third  degree  in  the  p  fundamental 
linearly  independent  ^-polynomials  which  vanishes  to  the  second  order  in 
A1)...,A2p^3  and  in  the  places  ml}  ...,  mp.  Further  let  3?(x)  be  that 
^-polynomial  which  vanishes  to  the  second  order  in  the  places  nj,  ...,  ?ip_!. 
Then  we  have  shewn  (§  244)  that  the  ratio  \/Z  (x)/(f>  (x)  \/<I>  (x),  save  for  an 
initial  determination  of  sign  for  an  arbitrary  position  of  x,  is  single-valued  on 
the  dissected  Riemann  surface  ;  hence  instead  of  the  function  CTJ  (x,  z)  we 
may  use  the  function 


E  (x  z}  = 


which  has  the  properties  ;  (i)  on  the  dissected  Riemann  surface  it  is  a  single- 
valued  function  of  x  and  of  z,  (ii)  El  (x,  z)  =  —  E1  (z,  x},  (iii)  as  a  function  of  x 
it  has,  beside  the  fixed  zeros  m1,  ...,  mp,  only  the  zero  given  by  x  =  z,  and  it 
has  no  infinities  beside  the  fixed  infinity  given  by  x  =  m,  where  it  is  infinite 
to  the  first  order.  At  the  r-th  period  loops  respectively  of  the  first  and 
second  kind  it  has  the  factors 

I  g-  *»<<«»?  *+  tort) 

But  there  can  be  no  doubt,  in  view  of  the  considerations  advanced  in 
chapter  XII.  of  the  present  volume,  as  to  the  way  in  which  the  ambiguity  of 
the  sign  of  •srl  (x,  z}  ought  to  be  dealt  with.  Suppose  that  the  Riemann 
surface  now  under  consideration  has  arisen  from  the  consideration  of  the 


273]  THE   SCHOTTKY-KLEIN    PRIME   FORM.  429 

functions  there  considered  (§  227)  which  are  unaltered  by  the  linear  substitu 
tions  of  the  group.  Let  the  places  in  the  region  S  of  the  f  plane  which 
correspond  to  the  places  x,  z,  x  ',  z'  of  the  Riemann  surface  be  denoted  by 
£>  £•  £  .  £"•  Then  by  comparing  the  equation  obtained  in  chapter  XII.  (§  234), 


with  the  equation  here  obtained, 

z 


and  noticing  that  X  (x),  -^  agree  in  being  differential  coefficients  of  an 

a£ 

integral  of  the  first  kind,  which  vanish  to  the  second  order  at  w,,  ...,  np^l, 
we  deduce  the  equation 


,       .  I     /  dt      dt^ 

<«.*>/V3   "3? 


f  " 

now  we  have  shewn  that  ro-(£,  £)  is  a  single-valued  function  of  f  and  £;  and 
any  one  of  the  infinite  number  of  values  of  £,  which  correspond  to  any  value 
of  #,  has  a  continuous  and  definite  variation  as  x  varies  in  a  continuous  way; 

hence  it  is  possible,  dividing  «TJ  (x,  z)  by  the  factor  A  /  -^  .  -^  ,  which  by 

V     Okc^        ft'^ 

itself  is  of  ambiguous  sign,  to  destroy  the  original  ambiguity  while  retaining 
the  essential  character  of  the  function  CTJ  (x,  z).  The  modified  function  is 
infinitely  many-valued,  but  each  branch  is  separable  from  the  others  by  a 
conformal  representation.  Thus  the  question  of  the  ambiguity  in  the  sign  of 
CTI  (x,  z)  is  subsequent  to  the  enquiry  as  to  the  function  £  which  will  conform 
ably  represent  the  Riemann  surface  upon  a  single  f  plane  in  a  manner 
analogous  to  that  contemplated  in  chapter  XII.  §§  227,  230*. 

In  what  follows  however  we  do  not  need  to  enter  into  the  question  of  the 
sign  of  vrl  (x,  z}.  It  has  been  shewn  in  the  preceding  article  that  the  final 
formula  obtained  is  independent  of  the  form  taken  for  the  function  there 
denoted  by  ty  (x).  It  is  therefore  permissible,  for  any  position  of  x,  to  take 


for  it  the  expression  VZ  (x),  with  any  assigned  sign,  without  attempting  to 
give  a  law  for  the  continuous  variation  of  this  expression.  The  advantage  is 
in  the  greater  simplicity  of  nyl  (x,  z)  ;  for  example,  when  x  is  at  any  one 

*  Klein  has  proposed  to  deal  with  the  function  •srl  (x,  z)  by  means  of  homogeneous  variables. 
The  reader  may  compare  Math.  Annal.  xxxvi.  (1890)  p.  12,  and  Eitter,  Math.  Annal.  XLIV.  (1894) 
pp.  274  —  284.  In  the  theory  of  automorphic  functions  the  necessity  for  homogeneous  variables 
is  well  established.  Cf.  §  279  of  the  present  chapter.  For  the  theory  of  the  function  •&1  (x,  z)  in 
the  hyperelliptic  case  see  Klein,  and  Burkhardt,  Math.  Annul,  xxxn.  (1888). 


430 


THE   GENERAL   FORMULA    FOR   ROOT-FUNCTIOXS. 


[273 


of  the  places  nlt  ...,  np_lt  the  function  \(as,  z),  as  denned  in  §  271,  vanishes 
independently  of  z  ;  but  this  is  not  the  case  for  TS^  (x,  z). 

Ex.  i.     Prove  that 

c) 


*'  z=\oe    i  i 

«•«       B  »,(*,«)»,(*  a)' 


Ex.  ii.     Prove  that  any  rational  function  of  which  the  poles  are  at  at,  ...  ,  a.,,  and  the 
zeros  at  /3j  ,  .  .  .  ,  /Sj,,  can  be  put  into  the  form 


where 


**!(#,  a^  ......  or^a?,  a*) 

j,  ...  ,  X;,  are  constants,  and  a  is  a  fixed  place. 

Tn  what  follows,  as  no  misunderstanding  is  to  be  apprehended,  we  shall 
omit  the  suffix  in  the  expression  ^l  (x,  z},  and  denote  it  by  •OT  (as,  z).  The 
function  -a  (£  £)  of  chapter  XII.  does  not  recur  in  this  chapter. 

274.  As  an  application  of  the  formula  of  §  272  we  take  the  case  of  the 
root  form  \/X<3>  (x)j®  (as)*/  X  (x),  where  Z(3)  (x)  is  a  cubic  polynomial  of  the 
differential  coefficients  of  the  integrals  of  the  first  kind,  having  3  (p  -  1)  zeros, 
each  of  the  second  order  (cf.  §  244,  Chap.  XIII.).  Then  the  poles  a1}  ...,  a,,  are 
the  2p  —  2  zeros  of  any  given  polynomial  <I>  (x),  which  is  linear  in  the 
differential  coefficients  of  integrals  of  the  first  kind.  Thus  r  =  2p  —  2, 

A  +  1  =  0,  R,  =r  +  h+I  +  '2\j  =2p  -2  +  0  +  0  =  2p  -2;   U=P^  ^>"y,  and, 

i  i 

taking  for  the  function  i/r  (x),  the  expression  V  X  (x),  the  formula  becomes 

" 


2p-2  2p-S 

n    n 


i,  j=l,  2,  ..., 

n  n 


n 


Herein  4>(«)  is  a  given  polynomial  with  zeros  at  Oj,  ...,  a»p-2,  and  the  forms 
v  JTj    («),  ..., 


_^(x)  are  any  set  of  linearly  independent  forms,  derived 
as  in  §  245,  Chap.  XIII.,  and  having  (—g1,...,  —  h-l,...,  —  hp)  for  characteristic. 

From  this  formula*  that  of  §  250,  Chap.  XIII.  is  immediately  obtainable. 
The  result  is  clearly  capable  of  extension  to  the  case  of  a  function 


*  Cf.  Weber,  Theorie  der  AbeVschen  Functionen  vom  Geschlecht  3,  Berlin,  1876,  §  24,  p.  156; 
Noether,  Math.  Annul,  xxvm.  (1887),  p.  367;  Klein,  Math.  Annal  xxxvi.  (1890),  p.  40.  For  the 
introduction  of  ^-polynomials  as  homogeneous  variables  cf.  §§  110—114,  Chap.  VI.  of  the  present 
volume.  See  also  Stahl,  Crelle,  cxi.  (1893),  p.  106;  Pick,  Math.  Annal.  xxix.  "  Zur  Theorie  der 
AbeFschen  Functionen." 


276] 


THE   GENERAL    FORMULA    FOR    RATIONAL    FUNCTIONS. 


431 


275.  A  general  application  of  the  formula  of  §  272  to  the  case  of  rational 
functions  may  be  made  by  taking  al}  ...,  a,,  to  be  any  places  whatever,  r 
being  greater  than  p-l.  Then  A +  1=0  and  R  =  r\  and  if  the  general 
rational  function  with  poles  in  a,,  ...,  ar,  nl}  ...,  np,l  be 

A-Fi  (x)  + +  A^F^  (x)  +  A,, 

where  Aly  ..^Ar  are  constants,  and  we  take  for  the  function  ^  (x)  the 
expression  V 'X  (x\  and  modify  the  constant  C  which  depends  in  general  upon 
«,,  ...,  <xr,  we  obtain  the  result  (cf.  §  175,  Chap.  X.) 


,  .. 
II 


II 


f,  O;) 


^T(xl)...X(xr}X(a,}  ...X  ( 


276.  This  formula  includes  many  particular  cases*.  We  proceed  to 
obtain  a  more  special  formula,  deduced  directly  from  the  result  of  §  272. 
Let  «!,  ....  ar  =  nll  ...,  np_lf  Then  the  everywhere  finite  factorial  integrals 
of  the  associated  system  are  the  ordinary  integrals  of  the  first  kind, 
and  the  number,  h  +  1,  of  dV  which  vanish  in  the  places  a,,  ...,  aj, 
nl}  ...,  ?i_p_1>  that  is,  which  vanish  to  the  second  order  in  the  places 


i,  is  1.    The  number  ^,  = 
general  function  having  the  poles 


1,  = 


,  =p.    The 


...,?iVi  mf(»)»^(te)/Z(ai)t  where 

X  (x)  is  the  expression  employed  in  §  273,  and  <&  (x)  denotes  the  differential 
coefficient  of  the  general  integral  of  the  first  kind.     Further 


a-  2  vni'a- 
i 


7  being  an  arbitrary  place.     Hence 


-8-    rs  = 


and 

eirw'df+J.+  i 

is  equal  (§175,  Chap.  X.)  to 


=      say, 


.',  @  (  7+ 


since  ss    is  an  odd  integer.     Therefore  taking  for  the  function 
expression  VZ  (ar),  X  (x,  z)  is  CT  (x,  z),  and 

A (f  T     \  — 

LA  \^i,    .  .  .  ,   O/y.^  — 


(x}  the 


.  xxxvi.  p.  38. 


432  THE    GENERAL    FORMULA    FOR   RATIONAL    FUNCTIONS.  [276 

where  <I>  (a;),  .  .  .  ,  4>p  (x)  denote  dv*'  "fdt,  ...,  dv%  */dt.     Thus  on  the  whole 

-^l-  n  *  * 


.. 
n  n 


where  G  is  a  quantity  which,  beside  the  fixed  constants  of  the  surface,  depends 
only  on  the  place  7.     Let  us  denote  the  expression 


which  clearly  has  no  zeros  or  poles,  by  p  (#;)  ;  then  we  proceed  to  shew  that 
in  fact  G  =  Ap,  (7),  where  A  is  a  quantity  depending  only  on  the  fixed 
constants  of  the  surface,  so  that  we  shall  have  the  formula 


™'  v  0  (  V)  = 


n  n  •nr  (xi,  Xj}  /i  (7) 

i<j 

where 

p 

i 
In  this  formula  7  only  occurs  in  the  factors 


_ 
— 


herein  the  factor  JT  (7)  occurs  once  in  the  denominator  of  each  of  CT(^-,  7), 
and  p  times  as  a  denominator  in  /j,  (7)  ;  thus  this  factor  does  not  occur  at  all. 
In  determining  the  factors  of  M*,  as  a  function  of  7,  it  will  therefore  be  suffi 
cient  to  omit  this  factor.  Thus  the  factor  of  ^  at  the  t'-th  period  loop  of  the 
first  kind  is  enis'(p~P~l)  or  e™'  .  At  the  t'-th  period  loop  of  the  second  kind  the 

factor  of  ®(vx'z  +  %(ls,S')  e™'1'*'  *  is  e-2l">f>e+K.  •)-"*«,  and  therefore  the 
factor  of  ^  is 

e  -  iris,  -  2*i  (vy'  XP  +  vn>  '  *4  ......  +  f71"-1  '  Xp'1  +  IT,.  ,). 

Consider  now  the  expression 


at  the  i-th  period  loop  of  the  first  kind,  this  function,  regarded  as  depending 
upon  7,  has  the  factor  e™'  ;  at  the  i-ih  period  loop  of  the  second  kind  it  has 
the  factor 


TJH 


277]  THE   FORMULA   FOR  THE   HYPERELLIPTIC   CASE.  433 

but  since 

iti  (Si  +  Ti,ls\+  ......  +  Ti.ps'y) 

it  follows  that 


is  equal  to 

-  irisi 
thus,  changing  7  into  x,  we  have  proved  that  the  function  of  x 


has  the  same  factors  at  the  period  loop  as  the  function,  of  x,  given  by 
w  0»,  #1)  ......  «•  (#,  arp)//*  (a;)  ; 

it  is  clear  that  these  functions  have  the  same  zeros,  and  no  poles. 
Hence  the  formula  set  down  is  completely  established*. 

277.  We  pass  now  to  the  particular  case  of  the  formula  of  §  272  which 
arises  when  the  fundamental  Riemann  surface  is  hyperelliptic,  and  associated 
with  the  equation 

if  =  4* 


Then  the  places  n1}  ...,  np^  are  branch  places.  We  suppose  also  that  p  +  1 
of  the  places  alt  ...,ar  are  branch  places,  say  the  place  for  which  x  =  dl,  ..., 
c£M+1)  and  that  //.  +  1  of  the  places  xly  ...,xr  are  branch  places,  say  those 
at  which  #  =  b1}  ...,  b^+1.  It  is  assumed  that  the  branch  places  n1}  ..., 
WP_,,  dl}  ...,  c^+i,  b1}  ...,  6^+1  are  different  from  one  another.  We  put 
r  —  (/j,+  l)  =  v,  then  the  determinant  of  the  functions  Ft  (xj\  (§  272), 
regarded  as  a  function  of  asl,  is  a  rational  function  with  poles  in  nl}  ...  ,  Wp_1} 
flj,  ...,  a.v,  d1}  ...,  c?M+1  and  zero  in  ar2,  ...,  «„,  6X,  ...,  6M+1.  Provided  v  is  not 
less  than  //,,  such  a  function  is  of  the  form 

-ttl^-fo-Wp.^-^...^^^ 

(^-^."(afi-Wp-iX^-^  —  C^-^+iX^-ai)---  («i-«r) 

where  the  degrees  of  (a?,,  !)„_!_„,  (a?,,  1),_1+M  are  determined  by  the  condition 
that  the  function  is  not  to  become  infinite  when  a^  is  infinite.  When  v  =  //,, 
the  terms  (a^,  l)^.^  are  to  be  absent.  When  i>  <  //,,  the  conditions  assigned 
do  not  determine  the  function  ;  we  shall  suppose  v  5  /A.  The  2y  —  1  ratios 
of  the  coefficients  in  the  numerator  are  to  be  determined  by  the  conditions 
that  the  numerator  vanishes  in  x2,  ...,#„  and  in  the  places  conjugatef 

*  See  the  references  given  in  the  note  *,  §  274,  and  in  particular  Klein,  Math.  Annul,  xxxvi. 
p.  39. 

t  The  place  conjugate  to  (x,  y)  is  (x,  -y) 

B-  28 


434 


DEFINITION   OF   THE   HYPERELLIPTIC   THETA   FUNCTION 


[277 


to  «!,  ...,  «„.     Hence,  save  for  a  factor  independent  of  x1}  the  determinant 
of  the  functions  F{  (xj)  is  given  by 


wherein  i/r  (as)  =  (x-n1)...(x-  n____)  (x-d^)...(x-  d^)  (x-b^...(x-  6M+1), 
0  (a?)  =  y^l^r  (x),  and  the  determinant  has  2v  rows  and  columns  ;  denoting 
this  determinant  by  D^  +,  the  determinant  of  the  functions  Fi  (xj)  (§  272)  is 
therefore  equal  to 


*  1  /(xi-b1)...(xi- 

'  *  i=i  (a?i-o1)...(a?<-a,)V(a;i-n1)...(a!f-v5  V  («»  -  dj.  ..(xt- 


-bl.+l) 


Hence,  from  §  272,  taking  ^(x)  =  ^(x  -n,)  ...(x-n^),  so  that  «•  (a;,  *)  will 
denote 


we  have 


where  C  is  independent  of  #_,  ...,  xv. 

Now,  if  b,  d  be  any  two  branch  places,  and  a  an  assigned  branch  place, 


and  hence,  if 


r,  6) 


b,a 


where  ft,  ...,  /Op',  S1}  ...,  8/  are  integers,  we  have  (§  175,  Chap.  X.) 


277]          BY   THE   FUNCTION  ta  (x,  z)  AND   ALGEBRAICAL   FUNCTIONS.  435 

where  A  is  independent  of  x.     Thus  the  expression 

„•  (8Hn  &  a  *r  (x,  d)      /x-b 
vr(x,b)  V   x-d' 

which  clearly  has  no  poles  or  zeros,  is  such  that  its  factors  at  the  period  loops 
are  all  +  1.  The  square  of  this  function  is  therefore  a  constant,  and  the 
expression  itself  is  a  constant. 

Therefore  if 

M+l     di    l. 

«  «<  '    »  f(<r<  4  a-i'Tt  ,  i  +  ......  +  <rp'Ti>p), 

where  o-,,  ...,<rp  are  integers,  it  follows  that  the  function 

e-Ki<r'(vx"a>  +  ......  +t*»M   jj  Mjj^0t,  <£;)        /Xj  -  bj 

i  =  l   j=l  -57  (#i,   bj)     V    «fc  —  (^ 

is  independent  of  a^,  ...,  a?,,.     Further 

@  (u  -  \<r  -  \-rcr  ;  \s,  \s}  =  Be™'*  ®[u;  %(S-<T),I  (s  -  a-')] 
by  §  175,  Chap.  X.     Thus  on  the  whole  we  have 

eejji  «•»••«;  K'-'XW- 


,  ,  t-«  ^  a 

•<j  f=ij=i  j<j 

where  C  is  independent  of  ^,  ...,  a?,.  Hence  we  can  infer  that  C  is  in  fact 
independent  also  of  a,  ,...,«„.  For  when  the  sets  xlt  ...,#„,  alt  ...,«„  are 
interchanged,  ^^  is  multiplied  by  (-)"2^-M  =  (_  I}M  and>  since  CT  (^  ^ 
=  -  -sr  (^  «),  this  is  also  the  factor  by  which  the  whole  right-hand  side  is 
multiplied.  The  theta  function  on  the  left-hand  side  is  also  multiplied 
by  +  1.  Thus  the  square  of  the  ratio  of  the  right-hand  side  to  the  theta 
function  on  the  left  is  unaltered  by  the  interchange  of  the  set  xlt  ...,  xv  with 
the  set  «,,  ...,  «„.  Thus  C2  is  independent  of  ^,  ...,  Xv  and  unaltered  when 
a?,,  ....  av  are  changed  into  a,,  ...,«„.  Hence  C  is  an  absolute  constant. 

It   follows   that   the    characteristic   *(*  -  er),   W  -  *\   and    the   theta 
functions,  are  even  or  odd  according  as  ^  is  even  or  odd. 

In  the  notation  of  §  200,  Chap.  XL,  the  half-periods  \^,  are  given  by 


hence,  if  the  half-periods  given  by 


be    denoted    by  ^ft,   the    half-periods    associated   with    the   characteristic 
f(*-*)i  $(s  -  o-')  are  congruent  to  expressions  given  by 


28—2 


436  RULE    FOR   THE   THETA-CHARACTERISTIC  [277 

while  -fy,  which  is  of  degree  p  +  1  +  2/i,  is.  equal  to 

(an-  O  ...(a?-  n^)  (x  -  &0  ...(a?-  6M+1)  (a;  -  dj  ...  (a;  -  d^+1); 
by  means  of  the  formula  (§  201,  Chap.  XI.) 


the  half-periods  associated  with  the  characteristic  ^(s  —  a),  ^(s'  —  <r')  can  be 
reduced  to  be  congruent  to  expressions  denoted  by 


where  elt  ...,  ep-2li+1  are  given  by 


also,  in  taking  all  possible  odd  half-periods  £ng)S<,all  possible  sets  of  p  —  1 
of  the  branch  places  will  arise  for  the  set  nly  ...,  np^.  Hence  it  follows  that 
the  formula  obtained  includes  as  many  results  as  there  are  ways  of  resolving 
(x,  l)ap+2  into  two  factors  ^+1_2F,  T/r^+i+2M>  °f  orders  p  +  1  —  2/A,  p  +  1  +  2/4, 
and  (§  201)  that  all  possible  half-integer  characteristics  arise,  each  associated 
with  such  a  resolution.  We  have  in  fact,  corresponding  to  fj,  =  0,  1,  2,  ..., 

E  (^—~  —  )  ,  a  number  of  resolutions  given  by 


It  has  been  shewn  (§  273)  that  the  expression  ta  (x,  z)  may  be  derived, 
by  proceeding  to  a  limit,  from  the  integral  II  Jt  J.  Hence  the  formula  that 
has  been  obtained  furnishes  a  definition  of  the  theta  function  in  terms 
of  the  algebraic  functions  and  their  integrals,  and  has  been  considered  from 
this  point  of  view  by  Klein,  to  whom  it  is  due.  After  the  investigation 
given  above  it  is  sufficient  to  refer*  the  reader,  for  further  development,  to 
Klein,  Math.  Annal.  xxxn.  (1888),  p.  351,  and  to  the  papers  there  quoted. 

Ex.  i.  Prove  that  the  function  6  [u  ;  i  (s  -  <r),  i  (*'  -  o-')]  vanishes  to  the  /*th  order  for 
zero  values  of  the  arguments. 

Ex.  ii.  In  the  notation  of  §  200,  Chap.  XL,  prove,  from  the  result  here  obtained,  that 
each  of  the  sums 

r+2   Ci,a         a,,  a       <r+4   cita         a,,a    ,  4r+3   cifa 
2    v*     ,    v  '      +    2  vl     ,    v  }      +   2  vl 


represents  an  odd  half-  period  ;  here  c<  is  any  one  of  the  places  c,clt  ...  ,  cp,  a»  is  any  one  of 
the  places  «15  ...  ,  ap,  a,-  is  any  one  of  the  places  a1}  ...  ,  ap,  and  r  is  an  arbitrary  integer 

*  See  also  Brill,  Grelle,  LXV.  (1866),  p.  273;  and  the  paper  of  Bolza,  American  Journal,  vol. 
xvii.,  referred  to  §  221,  note,  where  Klein's  formula  is  fundamental. 

By  means  of  the  rule  investigated  on  page  298,  of  the  present  volume,  the  characteristic 
£  (s  -  ff),  J  (s'  -  ff')  can  be  immediately  calculated  from  the  formula  here  (p.  436)  given  for  it.  Cf., 
also,  Burkhardt,  Math.  Annal.  xxxii.,  p.  426;  Thompson,  American  Journal,  xv.  (1893),  p.  91. 


278]  WHEN   THE   ALGEBRAICAL   CHARACTERISTIC    IS   GIVEN.  437 

whose  least  value  is  zero,  and  whose  greatest  value  is  given  by  the  condition  that  i  cannot 
be  greater  than  p  +  1.     Prove  also  that  each  of  the  sums 


4r+l  4r  4r4-2  4r-M 

2   /'•'",     S/*°,    *«*•+*%**,    va*'a+     l 
1=1  i=l  i=l  t=l 


represents  an  even  half-period.    For  a  more  general  result  cf.  the  examples  of  §  303  (Chap. 
XVII.). 


Ex.  iii.     By  taking  i/=p  +  l,/x  =  0,  and  the  places  b,  d  so  that  ^Qit  s,  =  iP>d)  finally 
putting  nv,  ...  ,  np_l,  b,  d  for  a^  ...  ,  ap,  aj,  +  1,  obtain,  from  the  formula,  the  result 


(x,  q)  s-q   P  (x-xi 


izr  (.£,  #;)  zzr  (2.  Ov) 
—    —  ' 


i  a;,  z  i  ,       izr   .£,  #;    zzr  2.  Ov  .          ,  ,  .      . 

where  n         replaces  log  —  j-2  —  K  —  p  —  L'    J,  (^)  =  (^  -  a)  ...  (x  —  «„),  and  the  branch  places 

xi'ai  TZ  (X,  tti)  •&  (z,  Xi)  ' 

a,  a,  ,  ...  ,  ap  are,  as  in  §  203,  Chap.  XI.,  such  that  the  theta  function  in  the  numerator  of 
the  left-hand  side  vanishes  as  a  function  of  x  at  the  places  £1?  ...,  gp,  conjugate  to 
x±  ,  .  .  .  ,  xp  ;  and  verify  the  result  d  priori.  By  the  substitution 


xi,ai=e 


this  formula  can  be  further  simplified.     Deduce  the  results 

x.z  x,*  =1    e(^>a-pa?"a'-  ......  -tr^p»a 

n  -   °g 


9  dx 

where  w  =  'y-r"ai-|-  ......  +  vx"'  a",  Zi(u)  =  ^-\oge(u),  and  -^  ,...  are  as  in  §  123,  Chap.  VII. 

These  results  have  already  been  given  (Chap.  X.). 
278.     It  is  immediately  proved,  by  the  formula  (§  187) 


_ 

- 


that  the  general  expression  of  a  factorial  function  given  in  §  254  can  be 
written  in  the  form 


n  [®(^.-i  +  ^n,  ^e™'"*'*^  n 
1  L  J  i  L 


And,  by  the  use  of  the  expression  TS  (x,  z),  this  may  be  put  into  the  form 

_2Tri£()l.  +  H.)vx'y  £  M  [  "I"1  *  f  ~|-\ 

t  f    *'       t  [      *>  «*  J     t  [CT  (*•  ^  J 


438  CONNECTION   OF  THEORY   OF   FACTORIAL   FUNCTIONS  [278 

Ex.  i.     In  the  hyperelliptic  case  associated  with  an  equation  of  the  form 

y*  =  (x,l)w  +  s, 
if  x  denote  the  place  conjugate  to  the  place  x,  it  follows  from  the  formula  of  §  273  that 

in*'2 

•si  (x,  z}  =  (x  —  z)e2    x,z, 

unless  x  or  z  is  a  branch  place. 

Ex.  ii.     In  the  hyperelliptic  case,  if  £,  &15  ...,£„  denote  branch  places,  and 


and  the  equation  associated  with  the  surface  be  yz  =  f(x\  where  f(x)  =  <£(#)  ty(x\  and  if 
we  take  places  x,  xv,  ...  ,  xp,  z,  zlt  ...  ,  zp,  such  that 

<»*'  +  ......  +  „?'*>=$*,  %•*>  +  ......  +  i>J"*"Stf*,       (t=l,2,...fp), 

then  it  is  easily  seen  that  the  rational  function  having  x,x^  ...,  xp  as  zeros  and  Z,ZI}...,ZP 
as  poles,  can  be  put  into  the  form  [y1^  (x)+y(f>  (•*')]  -^I»  (*)  +  «<£  (*01  wb-ere  ^>  /  are  the 
variables  and  s  is  the  value  of  y1  at  the  place  z.  Hence  prove,  by  Abel's  theorem,  that 


Ex.  iii.     Suppose  now  that  a,  a^  ...,  «p  are  the  branch  places  used  in  chapter  XL 
(§  200),  so  that 


......  +u 


x>z 


and  suppose  further  that  |Q,=£(s  +  rs')>  is  an  even  half-period  such  that 


and 

then  deduce  that 


_ 


The  results  of  examples  i,  ii,  iii  are  given  by  Klein. 

Ex.  iv.     Prove  that,  if  z,  f,  cx ,  . . . ,  cp  be  arbitrary  places,  and  yv ,  . . . ,  yp  be  such  that 
the  places  £,  yls  ... ,  yp  are  coresidual  with  the  places  z,  ct,  ... ,  cp,  then 

p      -&(x,z)w  (f,  z) 
hence  deduce,  by  means  of  the  result  given  in  Ex.  iv.,  page  174,  that 


where  a  is  an  arbitrary  place. 

279.  The  theory  of  the  present  chapter  may  be  considered  from  another 
point  of  view.  We  have  already  seen,  in  chapter  XII.,  that  the  theory  of 
rational  functions  and  their  integrals  may  be  derived  with  a  fundamental 
surface  consisting  of  a  portion  of  a  single  plane  bounded  by  circles,  and  the 


279] 


WITH   THEORY   OF  AUTOMORPHIC   FUNCTIONS. 


439 


change  of  independent  variables  involved  justified  itself  by  suggesting  an 
important  function,  CT  (f,  7).  We  explain  now*,  as  briefly  as  possible,  a  more 
general  case,  in  which  the  singular  points,  c1}  ...,  Ck,  of  this  chapter,  are 
brought  into  evidence. 

Suppose  that  a  function  £  exists  whereby  the  Riemann  surface,  dissected 
as  in  §  253,  can  be  conformally  represented  upon  the  inside  of  a  closed 
curvilinear  polygon,  in  the  plane  of  f,  whose  sides  are  arcs  of  circles^;  to  the 
four  sides,  (a;),  (a/),  (&;),  (&/),  of  a  period-pair-loop  are  to  correspond  four  sides 
of  the  polygon,  to  the  two  sides  of  a  cut  (7)  are  to  correspond  two  sides  of 
the  polygon ;  the  polygon  will  therefore  have  2  (2p  -f  k)  sides. 

Fig.  11. 


Then  it  is  easily  seen  that  if  C  be  the  value  of  £  at  the  angular  point  C  of 
the  polygon,  which  corresponds  to  one  of  the  singular  points  c1}  ...,  Ck  on  the 
Riemann  surface,  and  D  be  the  value  of  £  at  the  other  intersection]:  of  the 
circular  arcs  which  contain  the  sides  of  the  polygon  meeting  in  C,  we  can 
pass  from  one  of  these  sides  to  the  other  by  a  substitution  of  the  form 


where  ITTJI  is  the  angle  G  of  the  polygon,  (I  being  supposed  an  integer  other 
than  zero) ;  as  we  pass  from  a  point  £  of  one  of  these  sides  to  the  corresponding 
point  of  the  other  side,  the  argument  of  the  function  [(£-  C)/(£-  D)]*  increases 
by  2?r  ;  if  therefore  t  be  the  infinitesimal  at  the  corresponding  singular  point  on 

the  Riemann  surface,  we  may  write,  for  small  values  of  t,  (f-  C)/(£-D)  =  tf , 

i  i_ 

so  that  £-  C  =  t'  (C  -  D)  (1  -  *)-!.     Further  if  £  £  be  corresponding  points 

*  Klein,  Math.  Annal.  xxi.  (1883),  "Neue  Beitrage  zur  Kiemann'schen  Functionentheorie  " ; 
Ritter,  Math.  Annal.  XLI.  (1893),  p.  4;  Ritter,  Math.  Annal.  XLIV.  (1894),  p.  342. 

t  See  Forsyth,  Theory  of  Functions,  chapter  XXII.,  Poincare,  Acta  Math,  vol's.  i.— v.  We  may 
suppose  that  the  polygon  is  such  as  gives  rise  to  single-valued  automorphic  functions. 

J  Supposed  to  be  outside  the  curvilinear  polygon. 


440  A    FACTORIAL   FUNCTION    MAY    BE    REGARDED  [279 

011  the  sides  of  the  polygon  which  meet  in  C,  we  have  for  small  values  of  t, 

"     "*'  =    *  "  '*' 


d£  =     (C  _  D)  tl     dt,  d?  =    (C-D)  t      e     V    '  dt,  or 

V  V 

I 

ultimately,  the  factor  omitted  being  a  power  series  in  tl  or  (£  —  C)/(£—  D), 
whose  first  term  is  unity. 

We  shall  suppose  now  that  the  numbers  Xx,  ...,  \k  of  this  chapter  are 
given  by  X^  =  —  mt/li,  where  mi,  li  are  positive  integers.  Then  a  function 
whose  behaviour  near  a  is  that  of  an  expression  of  the  form  t~*  </>,  will,  near 
Gi,  behave  like  (£  —  Ci)mi<f>,  that  is,  will  vanish  a  certain  integral  number  of 
times.  Further,  for  a  purpose  to  be  afterwards  explained,  we  shall  adjoin  to 
the  k  singular  points  cl5  .  ..,  Ck,  m  others,  ely  ...,  em,  for  each  of  which  the 
numbers  X  are  the  same  and  equal  to  —  e,  so  that,  if  t  be  the  infinitesimal 
at  any  one  of  the  places  el}  ...,  em,  the  factorial  functions  considered  behave 
like  £'<£  at  this  place.  These  additional  singular  points,  like  the  old,  are 
supposed  to  be  taken  out  from  the  surface  by  means  of  cuts  (ej),  .  .  .  ,  (em)  ; 
and  it  is  supposed  that  the  corresponding  curves  in  the  curvilinear  polygon 
of  the  £-plane  are  also  cuts  passing  to  the  interior  of  the  polygon,  as  in  the 
figure,  so  that  at  the  point  E^  of  the  £-plane  which  corresponds  to  the  place  el 
of  the  Riemann  surface,  £  is  of  the  form  ^  =  E^-\-  t<j>,  where  <f>  is  finite  and  not 
zero  for  small  values  of  t,  t  being  the  infinitesimal  at  el, 

Factorial  functions  having  these  new  singular  points  as  well  as  the 
original  singular  points  will  be  denoted  by  a  bar  placed  over  the  top. 

Let  dv  denote  the  differential  of  an  ordinary  Riemann  integral  of  the 
first  kind  which  has  p  —  I  zeros  of  the  second  order,  at  the  places 
MI,  ...,  %_j.  Consider  the  function 


where   a,  c   are    arbitrary  places,  and  p  is  determined  so  that  Z2  is   not 
infinite  at  the  place  c,  or 


this  function  is  nowhere  infinite  on  the  Riemann  surface  ;  it  vanishes  to  the 
first  order  only  at  £  =  oo  ;  for  each  of  the  cuts  (e^,  .  .  .  ,  (em)  it  has  a  factor 

nip  1 

em  ;    at  a  singular   point   c;   it   is   expressible   as  a  power  series  in  t1  ,  or 
(?—  ty/(£-D),  whose  first  term  is  unity.     The  values  of  Z2  at  the  two  sides 


of  a  period  loop  are  such  that  Z2'/Z2  =  Vc^/c^'  ;  but  since  these  two  sides 
correspond,  on  the  £-plane,  to  arcs  of  circles  which  can  be  transformed  into 
one  another  by  a  substitution  of  the  form  £'  =  (a£  +  /3)/(7£  +  8),  wherein  we 
suppose  aS  -  fiy  =  1,  it  follows  that  Z2'/Z2  =  y^+8.  If  then  we  also  introduce 


279]  AS   AN   AUTOMORPHIC    FORM.  441 

the  function  Zlt  =  £Z.2>  we  have  for  the  two  sides  of  a  period  loop,  equations  of 

the  form 

Za'  =  j 

Consider  now  a  function 


where  K  is  a  factorial  function  with  the  k  +  m  singular  points,  and  R=2me/p. 

i 

At  a  singular  point  C;,  or  (7{,  its  behaviour  is  that  of  a  power  series  in  r  or 
(£_(?)/(£_£),  multiplied  by  (?-Ci)mi;  at  a  singular  point  a,  or  Eit  its 
behaviour  is  that  of  a  power  series  in  the  infinitesimal  t  multiplied  by 


or  unity  ;  at  a  period  loop  it  is  multiplied  by  a  factor  of  the  form  p,  (y%+  &)~R, 
where  p,  is  the  factor  of  K.  The  function  has  therefore  the  properties  of 
functions  expressible  by  series  of  the  form* 


wherein  the  notation  is,  that  ft83  (&t  £+&)/(?<  £+$0  is  one  °f  the  finite 
number  of  substitutions  whereby  the  sides  of  the  curvilinear  polygon  are 
related  in  pairs  and  R(£i)  is  a  rational  function  of  &.  The  equation 
connecting  the  values  /',  /,  of  the  function  /,  at  the  two  sides  of  a  period 
loop,  may  be  put  into  the  form 


and  we  may  regard   Z.2  f,  or  K,  as  a  homogeneous  form  in  the  variables 
Zlt  Z2,  of  dimension  R. 

The  difference  between  the  number  of  zeros  and  poles  of  such  a  factorial 
function  K  is  (§  254) 


adding  the  proper  corrections  for  the  zeros  of  the  automorphic  form  K  at 
the  angular  points  Gl,  ...,  Ck  (Forsyth,  Theory  of  Functions,  p.  645)  we  have, 
for  the  excess  of  the  number  of  zeros  of  the  automorphic  form  over  the 
number  of  poles 

2  X  +  2      =  -       2   -  2  +  k  +  m  +  1  -    2    +  m  +  1 

* 


where  q  =  k  +  m  +  1,  2  -  =  2  7-  +  m  +  1. 
/^         ti 

We   may   identify  this  result  with  a  known  formula    for  automorphic 
*  Forsyth,  Theory  of  Functions,  p.  642.     The  quantity  R  is,  in  Forsyth,  taken  equal  to  -  '2m. 


442  HOMOGENEOUS   VARIABLES   ON   THE   RIEMANN   SURFACE.  [279 

functions      Forsyth,    Theory    of   Functions,    p.    648 ;     if    in    the    formula 

m  ( n  —  1  —  2  - ) ,  there  given,  we  substitute,  by  the  formula  of  p.  608,  §  293, 
V  f^/ 

n  =  2JV—  1  +  q,  we  obtain  m  (ZN—  2  +  q  —  2  -  ]    ;  for  each  of  the  angular 

V  A1/ J 

points  G!,  ...,  Ck  is  a  cycle  by  itself,  each  of  the  points  E1}  ...,  Em  is  a  cycle 
by  itself,  and  the  remaining  angular  points  together  constitute  one  cycle 

(cf.  Forsyth,  p.  596) ;  the  sum  of  the  angles  at  the  first  k  cycles  is  2?rS  T-  , 

k 

the  sum  of  the  angles  at  the  second  m  cycles  is  2?rm,  the  sum  of  the  angles 
at  the  other  cycle  is  2?r*. 

There  is  a  way  in  which  the  adjoint  system  of  singular  points  elt  ...,  em 
may  be  eliminated  from  consideration.  Imagine  a  continuously  varying 
quantity,  xZ)  which  is  zero  to  the  first  order  at  et,  ...,  em  and  is  never  infinite, 
and  put  xl  =  xxz ;  the  expression  Kx2~e  may  then  be  regarded  as  a  homo 
geneous  form  in  xlt  #2  on  the  Riemann  surface,  without  singular  points  at 
el ,  ...,  em\  and  instead  of  the  function  Zz  we  may  introduce  the  form 

_j>_ 
£2  =  Z^x2  Zm ,  which  is  then  without  factor  for  the  cuts  (ej),  . . . ,  (em),  or,  as  we 

may  say,  is  unbranched  at  the  places  e1;  ...,  em ;  and  may  also  put  ^=  ^2. 

Thus,  (i),  a  factorial  function,  considered  on  the  £-plane,  is  a  homogeneous 
automorphic  form,  (ii),  introducing  homogeneous  variables  on  the  Riemann 
surface,  the  consideration  of  factorial  functions  may  be  replaced  by  the  con 
sideration  of  homogeneous  factorial  forms. 
Ex.     Shew  that  the  form 

1  f-fX,  a      1  /r,x,  a   .  r,x,  a  \  ,    „  x         x,  a    z,  c 

-        n'   — (n      + +n      j+sXj.-v.     v. 

n,        \        »«   /•/  \       z,  c       m\     eltc  '  em,  c'      ,  ,    t'-7    t         j 

P(x,z)=x2  f(z)e  *J  , 

where  a,  c  are  arbitrary  places  and  X£i  y  are  constants,  is  unbranched  at  e^  ... ,  em,  that  it 
has  no  poles,  and  vanishes  only  at  the  place  z.  Here  f(z)  is  to  be  chosen  so  that,  when  x 
approaches  2,  the  ratio  of  P  (x,  z)  to  the  infinitesimal  at  z  is  unity.  At  the  t-th  period 
loop  of  the  second  kind  the  function  has  a  factor  ( —  )•*  where 

If       n      •      i    ^7r*  /    /  \        "ifl    i    C,,  C    .  .       6m,  CN    .      _   N  z,  c 

M=2mr+—(q't-q)-—(vt1'    + +^      )  +  ^ _Xi>y  v'  °  rit  t , 

q'2  —  q  denoting  the  number  of  circuits,  made  in  passing  from  one  side  of  the  period  loop  to 
the  other,  of  x2  about  #2=0  other  than  those  for  which  x  encloses  places  elt  ... ,  em,  and  r 
denoting  the  number  of  circuits  t  of  x  about  z. 

*  The  formula  is  given  by  Ritter,  Math.  Annal.  XLIV.  p.  360  (at  the  top),  the  quantity  there 
denoted  by  q  being  here  -  \  p.  We  do  not  enter  into  the  conditions  that  the  automorphic  form 
be  single-valued. 

t  The  reader  will  compare  the  formula  given  by  Ritter,  Math.  Annal.  XLIV.  p.  291.  It  may  be 
desirable  to  call  attention  to  the  fact  that  the  notation  <r  + 1,  <r'  + 1,  as  here  used,  does  not  coincide 
with  that  used  by  Ritter.  The  quantities  denoted  by  him  by  a,  a1  may,  in  a  sense,  be  said  to 
correspond  respectively  to  those  denoted  here,  for  the  factorial  system  including  the  singular 
points  elt  ...,  em,  by  <r'  +  l  and  w'. 


281] 


CHAPTER  XV. 

RELATIONS  CONNECTING  PRODUCTS  OF  THETA  FUNCTIONS  —  INTRODUCTORY. 

280.  As  preparatory  to  the  general  theory  of  multiply-periodic  functions 
of  several  variables,  and  on  account  of  the  intrinsic  interest  of  the  subject,  the 
study  of  the  algebraic  relations  connecting  the  theta  functions  is  of  great 
importance.     The  multiplicity  and  the  complexity  of  these  relations  render 
any  adequate  account  of  them  a  matter  of  difficulty  ;  in  this  volume  the  plan 
adopted  is  as  follows  :  —  In  the  present  chapter  are  given  some  preliminary 
general  results  frequently  used  in  what  follows,  with  some  examples  of  their 
application.     The  following  Chapter  (XVI.)  gives  an  account  of  a  general 
method  of  obtaining  theta  relations  by  actual  multiplication  of  the  infinite 
series.     In  Chapter  XVII.  a  remarkable  theory  of  groups  of  half-integer 
characteristics,  elaborated  by  Frobenius,  is  explained,  with  some  of  the  theta 
relations  that  result  ;  from  these  the  reader  will  perceive  that  the  theory  is  of 
great  generality  and  capable  of  enormous  development.     References  to  the 
literature,  which  deals  mostly  with  the  case  of  half-integer  characteristics,  are 
given  at  the  beginning  of  Chapter  XVII. 

281.  Let  <j>(ul}  ...,Up)  be  a  single-valued   function  of  p   independent 
variables   wlf  ...,vp,  such  that,  if  a1}  ...,ap  be   a  set   of  finite   values  for 
MJ,  ...,  up  respectively,  the  value  of  <j>  (u^,  ...,  up),  for  any  set  of  finite  values 
of  Wj,  ...,up,   is  expressible  by  a  converging  series  of  ascending   integral 
positive  powers  of  u^  -  a1}  u^  —  a2,  .  .  .  ,  up  —  ap.     Such  a  function  is  an  integral 
analytical  function.     Suppose  further  that  <f)(u1}  ...,  up)  has  for  each  of  its 
arguments,  independently  of  the  others,  the  period  unity,  so  that  if  m  be  any 
integer,  we  have,  for  a  =  1,  2,  .  ..  ,  p,  the  equation 


Then*  the  function  <£(?*!,  ...,  up)  can  be  expressed  by  an  infinite  series  of 
the  form 


S        ......       2        Ani  ..... 

W,=  -oo  wp=-oo 

*  For  the  nomenclature  and  another  proof  of  the  theorem,  see  Weierstrass,  Abhandlungen 
aiis  dcr  Functionenlehre  (Berlin,  1886),  p.  159,  etc. 


444  PROOF   OF   THE    FUNDAMENTAL  [281 

wherein  n1}  ...,np  are  integers,  each  taking,  independently  of  the  others,  all 
positive  and  negative  values,  and  AHj> ...,  np  is  independent  of  u1}  ...,  up. 

Let  the  variables  ul9  . . . ,  up  be  represented,  in  the  ordinary  way,  each  by 
the  real  points  of  an  infinite  plane.  Put  xl  =  e2niUt ,  . . . ,  xp  =  e2™"? ;  then  to 
the  finite  part  of  the  wa-plane  (a=l,  "-,p)  corresponds  the  portion  of  an 
avplane  lying  between  a  circle  Fa  of  indefinitely  great  but  finite  radius  Ra, 
whose  centre  is  at  xa  =  0,  and  a  circle  ja  of  indefinitely  small  but  not  zero 
radius  ra,  whose  centre  is  at  xa  =  0.  The  annulus  between  these  circles  may 
be  denoted  by  Ta.  Let  aa  be  a  value  for  xa  represented  by  a  point  in  the 
annulus  Ta ;  describe  a  circle  (Aa)  with  centre  at  aa,  which  does  not  cut  the 
circle  ^a ;  then  for  values  of  aca  represented  by  points  in  the  annulus  Ta  which 
are  within  the  circle  (^o),  u*  may  be  represented  by  a  series  of  integral 
positive  powers  of  xa  —  aa ;  and  by  the  ordinary  method  of  continuation,  the 
values  of  ua  for  all  points  within  the  annulus  Ta  may  be  successively  re 
presented  by  such  series;  the  most  general  value  of  wa,  for  any  value  of  xa,  is 
of  the  form  xa  +  m,  where  m  is  an  integer.  Thus,  in  virtue  of  the  definition, 
(f)(u1,  ...,up)  is  a  single-valued,  and  analytical,  function  of  the  variables 
xl}  ...,xp,  which  is  finite  and  continuous  for  values  represented  by  points 
within  the  annuli  Tl,...,Tp  and  upon  the  boundaries  of  these.  So  considered, 
denote  it  by  -\Jr  (^ ,  . . . ,  xp). 

Take  now  the  integral 
1 


wherein  xl,...,xp  are  definite  values  such  as  are  represented  by  points 
respectively  within  the  annuli  T1}  ...,  Tp;  let  its  value  be  formed  in  two 
ways; 

(i)  let  the  variable  ta  be  taken  counter-clockwise  round  the  circum 
ference  Fa  and  clockwise  round  the  circumference  7a(a  =  l,  ...,j9);  when  ta  is 
upon  the  circumference  F0  put 

JL  -1.  Xd          *™a.  x*  ft 

—         "1       ^  "•"   ~~Q     i     *•        ^  -j-i  > 

ta  —  Xa          Va.          ta  ta  »-~      "a 

when  ta  is  upon  the  circumference  7a  put 

4+..-)  =  - 


.         T      2^      l~     "I  .      '  .*tt+l  ' 

ta.-X,.  \Xa         Xa          X.  '  fca=~C°^ft 


then  the  integral  is  equal  to 


where  dZa  represents   an  element   dta   taken   counter-clockwise   along   the 
circumference  F0,  and  dza  represents  an  element  dta  taken  clockwise  along 


281]  EXPONENTIAL  SERIES.  445 

the  circumference  ya  ;  since  the  component  series  are  uniformly  and  absolutely 
convergent,  this  is  the  same  as 

Mi  ftp 

i  oo  oo       r  r       r  T*..          T 

1       2    ...    2   //..,/*(« .W^Sr^*...^ 

^.iiTn^r  «1=-oo         np=-<x>JJ         J  ti          ...tp 

where  for  4  the  course  of  integration  is  a  single  complete  circuit  coincident 
with  F0  when  na  is  positive  or  zero,  and  a  single  complete  circuit  coincident 
with  70  when  na  is  negative,  the  directions  in  both  cases  being  counter 
clockwise  ;  thus  we  obtain,  as  the  value  of  the  integral, 

00  00 

2-^  A  "I  nP 

2*       A. n,,  ... ,  np  &\     . . .  Xp   , 
n\=  —  °o        MJ>= — oo 

where 


and  the  course  of  integration  for  ta  may  be  taken  to  be  any  circumference 
concentric  with  Fa  and  ya,  not  lying  outside  the  region  enclosed  by  them ; 

(ii)     let  the  variable  ta  be  taken  round  a  small  circle,  of  radius  pa, 
whose  centre  is  at  the  point  representing  xa  (a  =  1,  . . . ,  w) ;  putting 

we  obtain,  as  the  value  of  the  integral,  -v/r  (as1}  ...,  xp). 

The  values  of  the  integral  obtained  in  these  two  ways  are  equal*;  thus 
we  have 

00  00 

<p  (Ui,  . . . ,  Up)  =       _*       ...       — <       •"-«!,  ...,  nlt  &  » 

w,=  — oo          rip=— cc 

where 

/•I          /"I 

^!MI n  =      ...      g-2«(»»1«1+...+«pMp)  ^(-Wi)       ;  i^)dtt,  ...  dup. 

Jo      Jo 

By  the  nature  of  the  proof  this  series  is  absolutely,  and  for  all  finite 
values  of  ult  . . . ,  up ,  uniformly  convergent.  If  ua  =  va  +  iw*  (a.  =  1,  . . . ,  p),  and 
M  be  an  upper  limit  to  the  value  of  the  modulus  of  (f>  (MJ  ,  . . . ,  up)  for  assigned 
finite  upper  limits  of  wl}  ...,  wp,  given  suppose  by  |  wa  \  ^>  Wa,  we  have 

where  Na  = 

Ex.  i.     Prove  that 

—  r 

OW     i  n 
as  " 

Ex.  ii.     In  the  notation  of  §  174,  Chap.  X., 


*  Cf.,  for  instance,  Forsyth,  Theory  of  Functions,  p.  47.     The  reader  may  also  find  it  of 

interest  to  compare   Kronecker,   Vorlesungen  iiber Integrate  (Leipzig,  1894),  p.   177,    and 

Pringsheim,  Math.  Annal.  XLVII.  (1896),  p.  121,  ff. 


446  LINEAR   INDEPENDENCE    OF   THE    2^   THETA    FUNCTIONS  [282 

282.     Further  it  is  useful  to  remark  that  the  series  obtained  in  §  281  is 
necessarily  unique  ;  in  other  words  there  can  exist  no  relation  of  the  form 

00  00 

V  V  A  ni  Mp         f\ 

2,       ...       2,      AHi>  ^ttlpXi    ...Xp   =  0, 

«!=—  00  Wp=-00 

valid  for  all  values  of  xlt  ...,  xp  which  are  given,  in  the  notation  of  §  281,  by 
^a<|^0|<  -Ra,  unless  each  of  Ani<  ___>np  be  zero.    For  multiplying  this  equation 

by  #1    '      ...  xp         dx1  ...  dxp,  and  integrating  in  regard  to  xa  round  a  circle, 
centre  at  xa  =  0,  of  radius  lying  between  ra  and  Ra,  (a=  1,  ...,  p),  we  obtain 


An  important  corollary  can  be  deduced.  We  have  remarked  (§  175, 
Chap.  X.)  on  the  existence  of  2^  theta  functions  with  half-integer  character 
istics  ;  it  is  obvious  now  that  these  functions  are  not  connected  by  any  linear 
equation  in  which  the  coefficients  are  independent  of  the  arguments.  For  an 
equation 

22P  oo  oo 

2    Cgg  kg      2      ...      S      e^«(n+i*«>+&(»-H*«)*+ttrgr«(n+i*,)  =  0, 

S  =  l  »»i  =  —  °°  Wp=-oo 

where  the  notation  is  as  in  §  174,  Chap.  X.,  and  ks,  gs  denote  rows  of  p 
quantities  each  either  0  or  1,  can  be  put  into  the  form 


i  ..... 

NI  =  -  oo         Np=-<x> 

where   27n'£71,   ...,  ZiriUp  are   the   quantities   denoted  by  hu,  A^  .....  Np  is 
given  by 


ANl,  ....  Np  =  2  Cffii 

!)> 

where  the  summation  includes  2^  terms,  and  N1}  ...,  Np  take  the  values 
arising,  by  the  various  values  of  n  and  ks,  for  the  quantities  2n  +  ks  ;  it  is  clear 
that  the  aggregate  of  the  values  taken  by  2n  +  ks  when  n  denotes  a  row  of  p 
unrestricted  integers,  and  ks  a  row  of  quantities  each  restricted  to  be  either  0 
or  1,  is  that  of  a  row  of  unrestricted  integers. 

Hence  by  the  result  obtained  above  it  follows  that  -Ajr,,  ....  jyp  =  0,  for  all 
values  of  n  and  ks.  Therefore,  if  A,  denote  a  row  of  arbitrarily  chosen 
quantities,  each  either  0  or  1,  we  have 

=  0  ; 


adding  the  2^  equations  of  this  form  in  which  the  elements  of  n  are  each 
either  0  or  1,  the  value  of  ks  being  the  same  for  all,  we  have 


where  n,l,  ...,  /JLP  are  the  elements  of  the  row  letter  /JL  given  by  fj.  =  gs  +  \; 
the  product  (1  +  ein^}  ...  (1  +eiwfj-")  is  zero  unless  all  of  /^,  ...,  yuy  are  even, 


284]  WITH   HALF-INTEGER   CHARACTERISTICS.  447 

that  is,  unless  every  element  of  gg  is  equal  to  the  corresponding  element  of  X. 
Hence  we  infer  that  C^  k,  =  0  ;  and  therefore,  as  \  is  arbitrary,  that  all  the  22^ 
coefficients  C(Ji  t  ^  are  zero. 

Similarly  the  r2?  possible  theta  functions  whose  characteristics  are  rth 
parts  of  unity  are  linearly  independent. 

283.  Another*  proof  that  the  2'*  theta  functions  with  half-integer 
characteristics  are  linearly  independent  may  conveniently  be  given  here  :  we 
have  (§  190),  if  m  and  q  be  integral, 


and  therefore  if  A;  be  integral  and  Q'  =  q'  +  k',  Q  =  q  +  k, 


Therefore  a  relation 


8=1 

leads  to 

2  CU™  <™<2*'-™'<W  *  (u  •  fa)  =  0, 
8=1 

where  Qg  =  qs  +  k,  Qg'  =  qs'  +  k'  ;  in  this  equation  let  (m,  m')  take  in  turn  all 
the  2^  possible  values  in  which  each  element  of  m  and  m'  is  either  0  or  1  ; 
then  as 

•^gwUmQg'-m'Q,)  t    _  []_  +  gfilQ,'),-]  ...  [1  +  e«(Q«')p]  [1  -f  g-«(Q«)i]  ...  [1  +  e 

is  zero  unless  every  one  of  the  elements  (Q/X,  ...,  (Q«)^  is  an  even  integer, 
that  is,  unless  qs  =  k,  qg'=  k',  we  have 


2  £.«•<••*'-*•««  ^  (M  ;  fa)  =  2*pCk<$  (u  •  P)  =  0  ; 


TO  8  =  1 

thus,  for  any  arbitrary  characteristic  (k,  k'),  C^  =  0.     Thus  all  the  coefficients 
in  the  assumed  relation  are  zero. 

284.  We  suppose  now  that  we  have  four  matrices  o>,  &>',  77,  77',  each  of  p 
rows  and  columns,  which  satisfy  the  conditions,  (i)  that  the  determinant  of  o> 
is  not  zero,  (ii)  that  the  matrix  a)"1^'  is  symmetrical,  (iii)  that,  for  real  values 
of  !&!,...,  np,  the  quadratic  form  co^ca'n2  has  its  imaginary  part  positive^, 
(iv)  that  the  matrix  7]w~l  is  symmetrical,  (v)  that  77'  =  v)w~l<o  —  ^  7ria)~l  ;  then 
the  relations  (B)  of  §  140,  Chap.  VII.,  are  satisfied  ;  we  put  a  =  ^rjco"1, 
h  =  %iri(D~~l,  b  =  Triarla>,  so  that  (cf.  Chap.  X.,  §  190) 

77  =  2aeo,     t]'  =  2aa>'  —  h,     hat  =  \tn,     hco'  =  ^b  ; 

*  Frobenius,  Crelle,  LXXXIX.  (1880),  p.  200. 

t  Which  requires  that  the  imaginary  part  of  the  matrix  <a~lu'  has  not  a  vanishing  de 
terminant. 


448  EXPRESSION    FOR   A   GENERAL  [284 

as  in  §  190  we  use  the  abbreviation 

\m  (u)  =  Hm  (u  +  £Hm) 


where 

Hm  =  2r)m  +  2r)'m',     Hm  =  2&>m  +  2&>'?n/. 

We   have   shewn   (§   190)   that   a   theta   function  ^  (u,  q)  satisfies  the 

equation 

^  (u  +  Slm,q)  =  e*mW+*ri(™/-»W  ^  (u>  g,), 

m  and  m   each  denoting  a  row  of  integers;  it  follows  therefore  that,  when 
m,  m  each  denotes  a  row  of  integers,  the  product  of  r  theta  functions, 

n  (u)  =*  (u,  q(»)  *  (u,  ?(2>)  ......  *t(u,  q^l 

satisfies  the  equation 

n  (U  +  nm)  =  e»*m(W)+2«<mQ'-m'Q)  n  (u), 

wherein  Qit  Q/  are,  for  i=l,  2,  ...,  p,  the  sums  of  the  corresponding  com 
ponents  of  the  characteristics  denoted  by  q{l),  ...,  q(r). 

Conversely*,  Q,  Q'  denoting  any  assigned  rows  of  p  real  rational 
quantities,  we  proceed  to  obtain  the  most  general  form  of  single-  valued, 
integral,  and  analytical  function,  II  (u),  which,  for  all  integral  values  of 
m  and  m,  satisfies  the  equation  just  set  down.  We  suppose  r  to  be  an 
integer,  which  we  afterwards  take  positive.  Under  the  assigned  conditions 
for  the  matrices  o>,  &>',  77,  ?/,  such  a  function  will  be  called  a  theta  function 
of  order  r,  with  the  associated  constants  2«,  2&>',  2?;,  2V,  and  the  characteristic 
(Q,  Q'l 

Denoting  the  function  3(u;  Q),  of  §  189,  either  by  3  (it;  2o>,  2«',  fy,  2i/;  <?,  (?)  or 
3(u;  a,b,h;  Q,  Q'),  the  function  3(u;  2a>/r,  2w',  2rj,  2n/  ;  Q,  Q'/r)  is  a  theta  function  of 
the  first  order  with  the  associated  constants  2o>/r,  2o>',  2?;,  2rr)',  and  (Q,  Q'/r)  for  charac 
teristic  ;  increasing  u  by  2<am  +  2a>'m',  where  m,  m'  are  integral,  the  function  is  multiplied 
by  a  factor  which  characterises  it  also  as  a  theta  function  of  order  r,  with  the  associated 
constants  2«,  2<o',  2rj,  ty  and  ($,  <7)  for  characteristic.  We  have,  also, 

B(u;  ra,  rb,  rh)  =  $(u;   —  ,  2«',  2^,  irVj-^fnt;  2a,  2>-o>';  -^,  2^'J  =  sfra;  ",  A,  rfcj, 

where  the  omitted  characteristic  is  the  same  for  each. 

Let  ki  be  the  least  positive  integer  such  that  kiQJ  is  an  integer,  =/j,  say  ; 
denote  the  matrix  of  p  rows  and  columns,  of  which  every  element  is  zero 
except  those  in  the  diagonal,  which,  in  order,  are  kl}  kz>  ....  kp,  by  k;  the 
inverse  matrix  Ar1  is  obtained  from  this  by  replacing  k^  ...  respectively  by 

*  Hermite,  Compt.  Rend.  t.  XL.  (1855),  and  a  letter  from  Brioschi  to  Hermite,  ibid.  t.  XLVII. 
Schottky,  Abriss  einer  Theorie  der  AbeVschen  Functionen  von  drei  Variabeln  (Leipzig,  1880),  p.  5. 
The  investigation  of  §  284  is  analogous  to  that  of  Clebsch  and  Gordan,  Abel.  Funct.,  pp.  190,  ff. 
The  investigation  of  §  285  is  analogous  to  that  given  by  Schottky.  Of.  KSnigsberger,  Crelle,  LXIV. 
(1865),  p.  28. 


284]  THETA  FUNCTION  OF  ORDER  r.  449 

l/&i  ,  ... ;  iu  place  of  the  arguments  u  introduce  arguments  v  determined  by 
the  p  equations 

hiilu1  + +hi>pup  =  kivi,  (i  =  1 ,  . . . ,  p), 

which  we  write  hu  =  kv;  then,  by  the  equations  hw  =  ^TTI,  ha)'  =  £6,  it  follows 
that  the  increments  of  the  arguments  v  when  the  arguments  u  are  increased 
by  the  quantities  constituting  the  p  rows  of  a  period  ftw,  are  given  by  the  p 
rows  of  Um  defined  by 

kUm  =  Trim  +  bmf ; 

we    shall    denote    the    right-hand    side    of   this    equation    by    Tm;     thus 


Now  we  have 

a  (u  +  nm)2  —  auz  = 

and,  since*  the  matrix  a  is  symmetrical,  and  Hm  =  2aflm  -  2hm',   this  is 
equal  to 

2atlmu  +  a£lm  =  2aHm  (u  +  £flm)  =  (Hm  +  2hm')  (u 
and  therefore  equal  to 

\n  (u)  +  Trimm'  +  2hum'  +  h£lmm' 
or 

^•m  (u)  +  Trimm'  +  2kvm'  +  Tmm' ; 
thus,  by  the  definition  equation  for  the  function  II  (u),  we  have 

e  n  (u  +  n,n) = Q—rau  n  (ii) . 

therefore,  if  Q  (v)  denote  e~rau*  U  (u), 

G  (11  -4-  JT    \  —  f)  I  w\  a—r[Trimm'+ 

W  \v  -\-  um)  —  \j  \u)  e    L 


now  let  m  =  0,  and  m  =  ks,  where  s  denotes  a  row  of  integers  s1}  . . . ,  sp ;  then 

mQ'  =  ksQ  =&1s1Q/+ +  kpspQp  =skQ',  =  sf,  is  also  a  row  of  integers; 

and  Um  =  Trik~lm  +  k~*bm'  =  TTIS  ;  thus  we  have 

Q  (v  +  Tris)  =  Q  (v), 

or,  what  is  the  same  thing,  the  function  Q(v)  is  periodic  for  each  of  the 
arguments  vlt  ...,««,  separately,  the  period  being  TTI;  it  follows  then  (§  281) 
that  the  function  is  expressible  as  an  infinite  series  of  terms  of  the  form 
tfn1,n2,...,«pe2(n'l'1+"'~Hv'p)>  where  nlt  ...,  np  are  summation  letters,  each  of 
which,  independently  of  the  others,  takes  all  integral  values  from  -  x  to 

+  00,  and  the  coefficients  (?„, np  are  independent  of  vlt  ...,  vn.     This  we 

denote  by  putting 

Q(v)  =  e-rau*n(u)  =  2Cne™\ 

To  this  relation,  for  the  purpose  of  obtaining  the  values  of  the  coefficients 

*  By  a  fundamental  matrix  equation,  if  M  be  any  matrix  of  p  rows  and  columns,  and  «,  7-  be 
row  letters  of  p  elements,  n  u  v  =  fi.  v  u. 

B-  29 


450  EXPRESSION  OF  A  GENERAL  [284 

Cn,  we  apply  the  equation,  obtained  above,  which  expresses  the   ratio  to 
Q  (v)  of  Q  (v  +  Um)  or  Q  (v  +  k~lTm)  ;  thence  we  have 

26' 


in  this  equation,  corresponding  to  a  term  of  the  left-hand  side  given  by  the 
summation  letter  n,  consider  the  term  of  the  right-hand  side  for  which  the 
summation  letter  s  is  such  that 

Si  =  n{  +  rkinii,  (i  =  1,  2,  .  .  .  ,  p)  ; 

thus  s  =  n  +  rkm',  and  2vtSi  =  2^w;  -I-  2rkiVtmi',  or  2vs  =  2wn  +  2rkvmf  ;  hence 
we  obtain 


therefore,  equating  coefficients  of  products  of  the  same  powers  of  the 
quantities  e2"1,  .  .  .  ,  e?°p,  we  have 

n  _  n      0->k-lYmn+r(irimm'+Ymm')—zni(m<X—m'Q) 

^n+rkm'  —  ^n  •  &  > 

and  this  equation  holds  for  all  values  of  the  integers  denoted  by  n,  m,  m. 

By  taking  the  particular  case  of  this  equation  in  which  the  integers  m' 
are  all  zero  we  infer  that  the  quantity 

—  .  k-irrmn  —  mQ',  =  —.  k~l  (Trim)  n  —  mQ',  =  S  ms  (  r  ns  —  Q,'] 

TTl  Til  s  =  l  \KS  / 

must  be  an  integer  for  all  integral  values  of  the  numbers  rag  and  ns  ;  therefore 
the  only  values  of  the  integers  n  which  occur  are  those  for  which  the 
numbers  (ng  -k8Qs')/ks  are  integers;  thus,  by  the  definition  of  ks,  we  may  put 
n  =f+  kN,  N  denoting  a  row  of  integers,  and/=  kQ'. 

With  this  value  we  have 

k~lftmn  —  k~l  (Trim)  n  =  k~l  (bmf)  n  =  k~ln  (bin'}  =  k~ln  .  bin' 

=  (&-'/+  N)  .  bm  =  (Q'  +  N)  .  bm'  =  bm  (Q'  +  N)  ; 
hence,  as  mQ'  =  k~lmn  —  mN,  the  equation  connecting  Cn  and  Cn+rkm>  becomes 


—  g 

e27rtVmm'  being  equal  to  unity  because  r  is  an  integer,  and  bm'  Q'  —  bQ'm  =  bQ'm  ; 
therefore 

--Hm'r-fAT)2  „  ~1&^2  ov      , 

e  *  Cf+k(m.r+N}  =  e  *      Gf+kN  .  e^'n  , 

TQ  being  mQ  +  bQ',  or 


284]  THETA  FUNCTION  OF  ORDER  r.  451 

thus,  if  the  right-hand  side  of  this  equation  be  denoted  by  DN,  we  have,  for 
every  integral  value  of  m,  DN+rm>  =  DN ;  therefore  every  quantity  D  is  equal 
to  a  quantity  D  for  which  the  suffix  is  a  row  of  positive  integers  (which  may 
be  zero)  each  less  than  the  numerical  value  of  the  integer  r.  If  then  p  be 
the  numerical  value  of  r,  the  series  breaks  up  into  a  sum  of  pP  series;  let  J9M 
be  the  coefficient,  in  one  of  these  series,  in  which  the  integers  p  are  less  than 
p ;  then  the  values  of  the  integers  N  occurring  in  this  series  are  given  by 
JV"  =  fj,  +  rM,  M  being  a  row  of  integers,  which,  as  appears  from  the  work, 
may  be  any  between  —  oo  and  oo  ;  and  the  general  term  of  Q  (v)  is 


for  k.(Q'  +  N)v  =  kv(Q'  +  N)=kv(Q'  +  N)  =  hu  (Q'  +  N) ;  thus  the  general 
term  is 

now,  as  Tg  =  TriQ  +  bQ',  and  b  is  a  symmetrical  matrix,  the  quantity 


is  immediately  seen  to  be  equal  to 

rb  M  +  thi?1  +  2«<3 

r        r 

therefore  the  general  term  of  n  (u),  or  erau~  Q  (v),  with  the  coefficient  DM,  is 
e++x,  where 


=  rait  +  Zrhu  (j\f  +  ?-±-£}  +  rb(M+      ±^Y  +  2-rriQ  (  M  + 

\  r     I  \  r     J  V  T 


'  V  M  M 

and  this  is  the  general  term  of  the  function 

Q'  +  n 


where  ^  denotes  a  theta  function  differing  only  from  that  before  represented 
(§  189,  Chap.  X.)  by  ^,  in  the  change  of  the  matrices  a,  b,  h  respectively  into 
ra,  rb,  rh  ;  the  condition  for  the  convergence  of  the  series  ^  requires  that  r 
be  positive  ;  thus  p  =  r  ;  recalling  the  formulae 


we  see,  as  already  remarked  on  p.  448,  that,  instead  of 

w,  &>',  77,  ij', 


29—2 


452  EXPRESSION    OF   A   GENERAL  [284 

the  quantities  to  be  associated  with  the  function  ^  are 

6) 

- ,  a ,  97,  rrj  , 
with  this  notation  then  we  may  write,  as  the  necessary  form  of  the  function 

it(«X 

n  (u)  =  2tf  „*  (u  •  Q,  Q±P] 

~  \  r     ) 

wherein  K^,  =  D^e  r  r  is  an  unspecified  constant  coefficient,  ft  denotes 
a  row  of  p  integers  each  less  than  the  positive  integer  r,  and  the  summation 
extends  to  the  rp  terms  that  arise  by  giving  to  yu,  all  its  possible  values. 

From  this  investigation  an  important  corollary  can  be  drawn ;  if  a  single- 
valued  integral  analytical  function  satisfying  the  definition  equation  of  the 
function  II  (M)  (p.  448),  in  which  r  is  a  positive  integer  and  the  quantities 
Q,  Q'  are  rational  real  quantities,  be  called  a  theta  function  of  the  rth  order 
with  characteristic  (Q,  Q'),  then*  any  rp  +  l  theta  functions  of  the  rth  order, 
having  the  same  associated  quantities  2o>,  2&>',  2rj,  2rj'  and  the  same  charac 
teristic,  or  characteristics  differing  from  one  another  by  integers,  are  connected 
by  a  linear  equation  or  by  more  than  one  linear  equation,  wherein  the 
coefficients  are  independent  of  the  arguments  u^,  ...,  up ;  and  therefore  any 
of  the  functions  can  be  expressed  linearly  by  means  of  the  other  rp  functions, 
provided  these  latter  are  not  themselves  linearly  connected. 

For  the  determining  equation  satisfied  by  II  (u)  is  still  satisfied  if,  in 
place  of  the  characteristic  (Q,  Q'),  we  put  (Q  +  N,  Q'  +  N'),  N  and  N'  each 
denoting  a  row  of  p  integers;  and  if 

p  +  N'  =  v  (mod.  r),  say  p  +  N'  =  v  +  rL', 
we  have  (§  190,  Chap.  X.) 


and  therefore 


where  Hv  =  K^nlN~^  ;  and  the  aggregate  of  the  rP  values  of  —    -  is  the 

CV  -i. 

same  as  that  of  the  values  of  — . 

r 

Thus  any  rp  + 1  theta  functions  of  the  rth  order,  with  the  same  charac 
teristic,  or  characteristics  differing  only  by  integers,  and  associated  with  the 

*  The  theorem  is  attributed  to  Hermite  :  cf.  Compt.  Rendus,  t.  XL.  (1855),  p.  428. 


285]  THETA  FUNCTION  OF  ORDER  r.  453 

same  quantities  2<w,  2o>',  2??,  2tj',  are  all  expressible  as  linear  functions  of 

the   same  r#   quantities  ^  (  u  ;  Q,  —  —  -  )  with  coefficients  independent  of 

\  r     I 

u1}  ...,  up.     Hence  the  theorem  follows  as  enunciated. 

Ex.  i.     Prove  that  the  r"  functions  3  (u  ;  Q,  ^-^-\  are  linearly  independent  (§  282). 


Ex.  ii.  The  function  $  (u  +  a  ;  Q)  $  (u-a  •  Q)  is  a  theta  function  of  order  2  with 
(2Q,  2<7)  as  characteristic.  Hence,  if  2P+1  values  for  the  argument  a  be  taken,  the 
resulting  functions  are  connected  by  a  linear  relation. 

For  example,  when  p  =  l,  we  have  the  equation 

o-2  (a)  a-  (u  -b)<r(u  +  b)-  a*  (b)  or  (u  -  a)  <r  (u  +  a)  =  a3  (u)  .  <r  (a-b)tr  (a  +  b). 

Ex.  iii.  The  function  9  (ru,  Q)  is  a  theta  function  of  order  r2  with  (rQ,  r(?)  as 
characteristic.  Prove  that  if  £  denote  a  theta  function  with  the  associated  constants 

w>  r2&)'>  ^  '  •/»  m  place  of  a),  w',  T),  T)'  respectively,  then  we  have  the  equations 


where  the  summation  letters  /*,  j/  are  row  letters  of  p  elements  all  less  than  r,  and  each 
summation  contains  f?  terms. 

Ex.  iv.     The  product  of  k  theta  functions,  with  different  characteristics, 


is  a  theta  function  of  order  k  for  which  the  quantities 


2 
Lr= 


2  $r)-  2r/  2  wM,     2   ^'(r>  +  2^   2 
r=l  r=l 


enter  as  characteristic.     Thus  a  simple  case  is  when  uW  +  .  ..  +  uW  =  0. 
For  p  =  l  a  linear  equation  connects  the  five  functions 


4 


4  4 

n  a(u+ut),          n  ir  (v+«|+4»X  u  r(«+«t+»7,  n 

!=1  = 


Ex.  v.  Any  (p  +  2)  theta  functions  of  order  r,  for  which  the  characteristic  and  the 
associated  constants  w,  o>',  ,,  ^'  are  the  same,  are  connected  by  an  equation  of  the  form 
P=0,  where  P  is  an  integral  homogeneous  polynomial  in  the  theta  functions.  For  the 
number  of  terms  in  such  a  polynomial,  of  degree  N,  is  greater  than  (Nrf,  when  N  is  taken 
great  enough.  That  such  an  equation  does  not  generally  hold  for  (p  +  l)  theta  functions 
may  be  proved  by  the  consideration  of  particular  cases. 

285.  The  following,  though  partly  based  on  the  investigation  already 
given,  affords  an  instructive  view  of  the  theorem  of  §  284. 

Slightly  modifying  a  notation  previously  used,  we  define   a   quantity, 
depending  on  the  fundamental  matrices  <a,  &>',  rj,  r}',  by  the  equation 
X  (u  ;  P,  P)  =  HP  (U  +  $np)  -  -n-iPP' 

=  (2r)P  +  27/P')  (U  +  0)P  +  0)'P')  -  TTiPP, 


454  ANOTHER  PROOF  [285 

where  P,  P'  each  denotes  a  row  of  p  arbitrary  quantities.  The  corresponding 
quantity  arising  when,  in  place  of  &>,  &/,  77,  if  we  take  other  matrices  <o(1), 
w'w,  77(1),  ?/(1)  may  be  denoted  by  X(1)  (u;  P,  P').  With  this  notation,  and  in 


case 

are  respectively 


, 

-    ,  eo     ,  77     ,  rrj  , 
r 


where  r  is  an  arbitrary  positive  integer,  we  have  the  following  identity 

r    2<»    *r   /i 

r\\u-\  --  s  ;  Jv  ,  m 


=  X<»  [M  +  n^  ;  A;,  0]  +  X'1*  [u  ;  m,  m']  -  X*1'  [M  ;  s,  0]  - 

where  s,  N,  m,  m,  k  each  denotes  a  row  of  p  arbitrary  quantities  subject  to 

the  relation 

s  +  rN  =  m+k; 

this  the  reader  can  easily  verify  ;  it  is  a  corollary  from  the  result  of  Ex.  ii., 
§190. 

Let  the  abbreviation  R  (u  ;  /)  be  denned  by  the  equation 

R  (u  ;  /)  =  SeT2*  («+  v)  -2"ifr  n  (u  +  2«  -V 
fc  V  T> 

^    -\(1)[tt;/(-,  0]-2iri/-  ,-r   /        .    0      M 

=  Ze  f  II    M  +  2&)  -    , 

«  V        r; 

wherein  A;  denotes  a  row  of  p  positive  integers  each  less  than  r,  and  the 
summation  extends  to  all  the  rP  values  of  k  thus  arising,  /  is  a  row  of  p 
arbitrary  quantities,  and  II  (u)  denotes  any  theta  function  of  order  r. 

Consider  now  the  value  of  R  (u  +  fl'i'  ;  /)  ;  by  definition  we  have 

n  rt*  +  2«  +  n)  =n 


therefore,  if  m  +  k  =  s  (mod.  r),  say  m  +  k  =  s  +  rN,  we  have,  by  the  defin 
ition  equation  (§  284)  satisfied  by  II  (M), 


where  (Q,  Q')  is  the  characteristic  of  II  (u),  and  hence 

R(u+  n|l';  /)  =  2e*II  (M+  2ft><1>s), 

in  which 

.„* 

r 


285]  OF   THE   EXPRESSION.  455 

by  the  identity  quoted  at  the  beginning  of  this  Article,  i/r  can  also  be  put 
into  the  form 

i/r  =  \a>  [u  ;  ra,  m']  -  X">  [u  ;  s,  0]  -  Zirim'k  -  Zirif-  +  Z-rri  (NQ1  -  m'Q), 


=  X(1)  [u  ;  Tii,  m']  -  V"  [it  ;  s,  0]  -  2-jrim'k  -  2-irim'Q  +  2-iriN(Q'  -/) 


"  s 


in  the  definition  equation  for  II  (u),  the  letters  m,  m  denote  integers  ;  and 
k  has  been  taken  to  denote  integers  ;  if  further  f  be  chosen  so  that  Q'  —f  is 
a  row  of  integers,  we  have,  since,  by  definition,  N  denotes  a  row  of  integers, 

_(D  A(1)[M;  m,  m']  +  2iri(mf-m'Q)          -\(1)  (u  ;  s,  0)  -Zirifi  ,_, 

12  (M  +  ftjf  ;  /)  =  e  \    r       '  2e  r  II  (u  +  2<w(1>  s) 


=  e 


;  m,  m']+2iri  ^w  ~-m'Q\ 

>  R  (u  •  f). 


Hence  R(u;  f)  satisfies  a  determining  equation  of  precisely  the  same 
form  as  that  satisfied  by  II  (u),  the  only  change  being  in  the  substitution  of 

—  ,  w',  77,  rrj'  respectively  for  <w,  <y',  77,  77'  ;  so*  considered  R(u;  f)  is  a  theta 

function  of  the  first  order  with    (Q,  -  J   as  characteristic;    putting,  in   ac 

cordance  with  the  definition  of  f  above,  f=  Q'  +  fj,,  where  p  is  a  row  of  p 
integers,  we  therefore  have,  by  §  284, 

R  (u  ;?+»)-  KQ^  *  (u  ;  Q,  Q^}  ,  =  Kq+.  *  (ru  •  *  ,  h,  rb  ;  *?}  , 

\  r     /  \        r  Q  / 

(p.  448)  where  Kq+lli  is  a  quantity  independent  of  u,  and  ^  is  the  same  theta 
function  as  that  previously  so  denoted  (§  284),  having,  in  place  of  the  usual 
matrices  a,  6,  h,  respectively  ra,  rb,  rh. 

Remarking  now  that  the  series 


wherein  p  denotes  a  row  of  p  integers  (including  zero),  each  less  than  r,  and 
the  summation  extends  to  all  the  rp  terms  thus  arising,  is  equal  to  r?  when 
the  p  integers  denoted  by  k  are  all  zero,  and  is  otherwise  zero,  we  infer  that 
the  sum 


1     . 
which,  by  the  definition  of  R  (u,  /),  putting  /=  Q'  +  p,  is  equal  to 

i  2  [.-*"*"  *••'-««'*  n  («+  a.^ 

B  («  ;  /)  may  also  be  regarded  as  a  theta  function  of  order  r,  with  the  associated  constants 
2tu,  2u',  2?;,  217'  and  characteristic  (Q,  f). 


456  EXAMPLES  OF   THE   APPLICATION  [285 

is,  in  fact,  equal  to  II  (u).     Hence  as  before  we  have  the  equation 


286.     Ex.  i.     Suppose  that  m  is  an  even  half-integer  characteristic,  and  that 


are  s,  =  W,  half-integer  characteristics  such  that  the  characteristic  formed  by  adding  the 
three  characteristics  m,  ait  a,-  is  always  odd,  when  i  is  not  equal  to  j.  Thus  when  m 
is  an  integral,  or  zero,  characteristic,  the  condition  is  that  the  characteristic  formed  by 
adding  two  different  characteristics  at,  0,-may  be  odd.  The  characteristic  whose  elements 
are  formed  by  the  addition  of  the  elements  of  two  characteristics  a,  b  may  be  denoted  by 
a  +  b  ;  when  the  elements  of  a  +  b  are  reduced,  by  the  subtraction  of  integers,  to  being  less 
than  unity  and  positive  (or  zero),  the  reduced  characteristic  may  be  denoted  by  ab. 

For  instance  when  p  =  2,  if  a,  ft,  y  denote  any  three  odd  characteristics,  so  that  *  the 
characteristic  afty  is  even,  and  if  /*  be  any  characteristic  whatever,  characteristics  satis 
fying  the  required  conditions  are  given  by  taking  m,  alt  a.2,  a3,  a4  respectively  equal  to 
afty,  p.,  fifty,  pya,  ^aft  ;  in  either  case  a  characteristic  mo^o,-  is  one  of  the  three  a,  ft,  y  and  is 
therefore  odd. 

When  jo  =  3,  corresponding  to  any  even  characteristic  m,  we  can  in  8  ways  take  seven 
other  characteristics  a,  ft,  y,  K,  X,  p,  v,  such  that  the  combinations  a,  ft,  y,  K,  X,  p,  v,  ma/3, 
man,  mX/i  constitute  all  the  28  existent  odd  characteristics  ;  this  is  proved  in  chapter 
XVII.  ;  examples  have  already  been  given,  on  page  309.  Hence  characteristics  satisfying 
the  conditions  here  required  are  given  by  taking 

m,  «19  «2>  «3>  -•>  as 
respectively  equal  to 

m,  m,  a,  ft,  ...,  v. 

Now,  by  §  284,  every  2"  +  1  theta  functions  of  the  second  order,  with  the  same  periods 
and  the  same  characteristic,  are  connected  by  a  linear  equation.  Hence,  if  p,  q,  r  denote 
arbitrary  half-integer  characteristics,  and  v,  w  be  arbitrary  arguments,  there  exists  an 
equation  of  the  form 

A9(u  +  w;  q)S(u-iv;  r)=   2 

A~*=l 

wherein  A,  A^  are  independent  of  u  ;  for  each  of  the  functions  involved  is  of  the  second 
order,  as  a  function  of  u,  and  of  characteristic  q  +  r. 

We  determine  the  coefficients  A^  by  adding  a  half  period  to  the  argument  u  ;  for  u 
put  u  +  Qm-aj-p  ;  then  by  the  formula 

S  (u  +  QP,  <?)  =  /  <";  P]  -*"iP'q  B  (u  ;  P+q), 
where 

X  (u  ;  1>]  =  HP  (u  +£aP)  -  viPl", 

noticing,  what  is  easy  to  verify,  that 

(u-v;  P)-\  (u+w;  P}-\(u-iv\  P)  =  0 


As  the  reader  may  verify  from  the  table  of  §  204  ;  a  proof  occurs  in  Chap.  XVII. 


286]  OF   THE  THEOREM.  457 

we  obtain 


=  2   A^[u  +  v;  (m-aj-a^  +  q  +  r-2p)]$[u-v;  (m  -  a,-  -f  « 


But  since  m-aj  +  a^  (which,  save  for  integers,  is  the  characteristic  maja^  is  an  odd 
characteristic  when./  is  not  the  same  as  X,  we  can  hence  infer,  putting  u  =  v,  that 


Hence  the  form  of  the  relation  is  entirely  determined.  The  result  can  be  put  into 
various  different  shapes  according  to  need.  Denoting  the  characteristic  m  +  q  +  r 
momentarily  by  k,  so  that  k  consists  of  two  rows,  each  of  p  half-integers,  and  similarly 
denoting  the  characteristic  (t^+p  momentarily  by  aA,  and  using  the  formula  for  integral  M, 


el$(u;  q), 
we  have 


e-'a^3(Zv;  k); 
we  shall  denote  the  right-hand  side  of  this  equation  by 

e-4rf<aA+P)(,»'+9'+r')  .jra,,  ;  (m+q  +  r)]  ; 
hence  the  final  equation  can  be  put  into  the  form 

;  m] 


It  may  be  remarked  that,  with  the  notation  of  Chap.  XI.,  if  615  ...,  bp  be  any  finite 
branch  places,  and  Ar  denote  the  characteristic  associated  with  the  half-period  ub>--a,  and 
we  take  for  the  characteristics  a:,  ...,  «g  the  2»  characteristics  A,  AA^  ...  Ak,  formed  by 
adding  an  arbitrary  half-integer  characteristic  A  to  the  combinations  of  not  more  than  p 
of  the  characteristics  A1,  ...,  Ap,  and  take  for  the  characteristic  m  the  characteristic 
associated  with  the  half-period  iibi>ai  +  ...  +  ubp>ap,  then  each  of  the  hyperelliptic  functions 
5(0;  raaiO,-)  vanishes  (§  206),  though  the  characteristic  rn.^^  is  not  necessarily  odd. 
Hence  the  formula  here  obtained  holds  for  any  hyperelliptic  case  when  m,  alt  ...,  a,,  have 
the  specified  values. 

Ex.  ii.     When  p  =  2,  denoting  three  odd  characteristics  by  a,  /3,  y,  we  can  in  Ex.  i.  take 

P,  q,  r,  m,  «i,  «2>  «a>  ai 
respectively  equal  to 

a^y,  q,  0,  a/3y,  0,  /3y,  ya,  a/3, 

wherein  0  denotes  the  characteristic  of  which  all  the  elements  are  zero,  and  £y  denotes 
the  reduced  characteristic  obtained*  by  adding  the  characteristics  #  and  y.  Then  the 
general  formula  of  Ex.  i.  becomes,  putting  v  =  0  and  retaining  the  notation  m  for  the 
characteristic  a/3y, 

3(u+w;  q)3(u-w;  0)5(0;  q  +  m)3(0;  TO) 

«A  +  '")(-'  +  «-)  3  (u;  q-m-a^3(u;  m+a^S(w;  q-aj9(w,  aA). 

So  that  all  the  elements  of  £7  are  zero  or  positive  and  less  than  unity. 


2 

A  —  1 


458  A   GENERAL   ADDITION   THEOREM  [286 

EM.  iii.     As  one  application  of  the  formula  of  Ex.  ii.  we  put 

'10\  ,  /10\  ,  /01\  ,  /Ol 


and  therefore 

'ION         ,  /oo\        ,  /oo 

m  = 


hence  we  find,  comparing  the  table  of  §  204,  and  using  the  formula 


where  M,   =(M^/},  consists  of  integers,  f-Cffi),  and  Mf  =  MJ^  +  MJ^  that* 
\M1M2J  V/i/2/ 

(u-<w;  0)  =  56(M-w),  5(0;  ?  +  m)  =  5J2  (0),  5(0;  m)  =  301(0;, 


3(u;q-m-a3)  =      524(w),5( 
5  (M  ;  ?  -  m  -  o4)  =  -  514(«),  5  (M  ;  m  +  eg  =  -  53  (w),  5  (w  ;  g-  -  a4)  =     5M(w),  5  (w  ;  a4)  =  -  524(w), 
all  the  factors  of  the  form  eiwi(a\+  mXm'  +  q">  being  equal  to  1  ;   by  substitution   of  these 
results  we  therefore  obtain 

502  (u  +  w)  55  (u-w)  512  (0)  501  (0)  =  51250150256  +  5025651850,  +  50152453514+535M5045!J4, 
where  512  denotes  512  (w),  etc.,  and  302  denotes  502  (w),  etc.  ;   this  agrees  with  the  formula 
of  §§  219,  220  (Chap.  XI.). 

Ex.  iv.     By  putting  in  the  formula  of  Ex.  ii.  respectively 


obtain  the  result 


which  is  in  agreement  with  the  results  of  §§  219,  220. 

Dividing  the  result  of  Ex.  iii.  by  that  of  Ex.  iv.  we  obtain  an  addition  formula  for  the 
theta  quotient  502  (tt)/56  (w),  whereby  9oz(u  +  w)/$5(u+w)  is  expressed  by  theta  quotients 
with  the  arguments  u  and  w. 

Ex.  v.  The  formula  of  Ex.  ii.  may  be  used  in  different  ways  to  obtain  an  expression 
for  the  product  3  (u  +  w;  q)  5(w  —  w;  0).  It  is  sufficient  that  the  characteristics  m  and 
o+m  be  even  and  that  the  three  odd  characteristics  a,  /3,  y  have  the  sum  m.  Thus, 
starting  with  a  given  characteristic  y,  we  express  it,  save  for  a  characteristic  of  integers, 
as  the  sum  of  two  even  characteristics,  m  and  q+m,  which  (unless  q  be  zero)  is  possible 
in  three  wayst,  and  then  express  m  as  the  sum  of  three  odd  characteristics,  a,  /3,  y, 
which  is  possible  in  two  waysj;  then§  we  take  ^  =  0,  a2  =  /37>  a3  =  yat  «4=o£.  Taking 
, 

'    ave 

*  In  Weierstrass's  reduced  characteristic  symbol  the  upper  row  of  elements  is  positive,  and 
the  lower  row  negative  ;  cf.  §§  203,  204,  and  p.  337,  foot-note. 

t  This  is  obvious  from  the  table  of  §  204,  or  by  using  the  two-letter  notation  ;  for  instance 
the  symbol  (a^J^a^)  +  (a2c)  =  (a1c1)  +  (a2c1)=(a1c2)  +  (a^). 

t  For  example,  (ac)  =  (t^a)  +  (a2a)  +  (c^)  =  (a^)  +  (cjc)  +  (cc2).  See  the  final  equation  of  §  201. 
The  six  odd  characteristics  form  a  set  which  is  a  particular  case  of  sets  considered  in 
chapter  XVII. 

§  Moreover  we  may  increase  M  and  w  by  the  same  half-period.  But  the  additions  of  the  half- 
periods  P,  P  +  fl3  lead  to  the  same  result  ;  and,  when  q  is  one  of  a,  /3,  7,  the  same  result  is 
obtained  by  the  addition  of  P  +  ttm  and  of  P  +  QTO  +  i2a. 


286]  FOR  THE  CASES  p  =  2,  p  =  3.  459 

10\         /10\         /00\         /01\         /11\         /00\         /IO 


putting  m=\    fwvi  we  may 

10 


Hence  obtain  the  result 

502  (u+w)  55  (M-  w)  512  (0)  301  (0)-*M5w5tt5,+3w5il51458+  Vu^^+^^S^,, 

where,  on  the  right  hand,  512  denotes  512(w),  etc.,  and  502  denotes  502(w),  etc.     Comparing 
this  result  with  the  result  of  Ex.  iii.,  namely 


5  (u-w)  512  (0)  501  (0)  =  ^125010255  +  502^5512501  +  50^2453514  +  53^4504524, 
we  deduce  the  remarkable  identity 
54  (u)  513  (M)  523  (w)  503  (  w)  +  ^  (w)  5M  («)  50  (w)  32  (w) 

=  502  (w)  55  (u)  31S  (w)  501  (w)  +33  (M)  514  (w)  5M  (w)  524  (w), 

wherein   w,  w  tare  arbitrary  arguments  ;    this  is  one  of  a  set  of  formulae  obtained  by 
Caspary,  to  which  future  reference  will  be  made. 

Ex.  vi.     By  taking  in  Ex.  v.  the  characteristics  q,  m  to  be  respectively 


(•   *($' 

and  resolving  m  into  the  sum  a+/3  +  y  in  the  two  ways 


respectively,  obtain  the  formulae 

502  (M  +  w)  $B  (u-w)  B0  (0)  52  CO)»^^JA+\^U    -  54^i85M5M  -  3M3M51S$4) 

502  («  +  w)  5-  (M  -  w)  50  (0)  32  (0)  =  505250255  -  SM5W54513  -  5145,503523  +  ^5^0,  512, 
and  the  identity 

•^34  ^1  ^01  ^12  +  °i  °13  ^24  ^04  =  ^5  ^02  ^0  ^  2  +  ^14  ^3  °03  ^23  ' 

Putting  in  this  equation  w  =  0,  we  obtain  a  formula  quoted  without  proof  on  page  340. 

Ex.  vii.  Obtain  the  two  formulae  for  502  (?<  +  w)  55  (u  —  w)  which  arise,  similarly  to 
those  in  Exs.  v.  vi.,  by  taking  for  m  the  characteristic  |  (  J  ,  the  characteristic  q  being 
unaltered. 

Ex.  viii.     Obtain  the  formulae,  for  p  =  2, 


523  (u  +  w)  ^  (u  -  w)  56  (0)  523  (0;  =  ^^ia^^  +  ^  5,^5!  5^  -  53525352  -  513512513512, 
where  the  notation  is  as  in  Ex.  v. 

For  tables  of  such  formulae  the  reader  may  consult  Konigsberger,  Crelle,  LXIV.  (1865), 
p.  28,  and  ibid.,  LXV.  (1866),  p.  340.  Extensive  tables  are  given  by  Rosenhain,  M4m.  par 
divers  Savants,  (Paris,  1851),  t.  XL,  p.  443  ;  Cayley,  Phil.  Trans.  (London,  1881), 
Vol.  171,  pp.  948,  964  ;  Forsyth,  Phil.  Tram.  (London,  1883),  Vol.  173,  p.  834. 


460  A   MORE   GENERAL   FORMULATION.  [286 

Ex.  ix.     We  proceed  now  to  apply  the  formula  of  Ex.  i.  to  the  case  p  =  3  ;  taking  the 
argument  v  =  0,  the  characteristics  p,  r  both  zero,  and  the  characteristics  TO,  CTJ,  a2,  ......  ,  as 

to  be  respectively  TO,  m,  a,  /3,  ......  ,  f,  where  a,  /3,  y,  K,  X,  p,  v  are  seven  characteristics 

such  that  the  combinations  a,  /3,  y,  K,  X,  p.,  v,  ma/3,  TOOK,  mX/x  are  all  odd  characteristics, 
TO  being  an  even  characteristic,  and  removing  the  negative  signs  in  the  characteristics  by 
such  steps'*  as 


=  e-  47rim(a'  A  +  p'+  m')  $  ( 
=  e-47rim(p'  +  a'A)^(M;. 

the  formula  becomes  t 


8 

=  2  e~'Mm«'A.  +  «'aA>.»( 
\=i 

In  order  that  the  left-hand  side  of  this  equation  may  not  vanish,  the  characteristic 
q  +  m  must  be  even;  now  it  can  be  shewn  that  every  characteristic  (q),  except  the  zero 
characteristic,  can  be  resolved  into  the  sum  of  two  even  characteristics  (TO  and  q  +  m) 
in  ten  ways,  and  that,  to  every  even  characteristic  (TO)  there  are  8  ways  of  forming  such 
a  set  as  a,  /3,  y,  K,  X,  /x,  v  (cf.  p.  309,  Chap.  XI.).  Hence,  for  any  characteristic  q  there 
are  various  ways  of  forming  such  an  expression  of  3(u  +  w;  q)3(u  —  w;  0)  in  terms 
of  theta  functions  of  u  and  w  ;  moreover  by  the  addition  of  the  same  half-period  to  u 
and  w,  the  form  of  the  right-hand  side  is  altered,  while  the  left-hand  side  remains 
effectively  unaltered.  In  all  cases  in  which  q  is  even  we  may  obtain  a  formula  by 
taking  TO  =  0. 

Ex.  x.     Taking,  in  Ex.  ix.,  the  characteristics  q,  m  both  zero,  prove  in  the  notation 
of  §  205,  when  a,  /3,  ......  ,  v  are  the  characteristics  there  associated  with  the  suffixes 

1,  2,  ......  ,  7,  that 

3(u+u;)3(u-w)9*  =  2  $?(u}S?(w}. 

i=0 

Prove  also,  taking  m=0,  q  =  ^  (  AAn  )  ,  that  3456  (u  +  w)  3  (u  -  w)  5456  9  is  equal  to 

\UUv/ 


3  (u)  3  (w)  Sm  (u)  3456  (w)  +$t  (u)  54  (w)  $56  (u)  556  (w)  +  S5  (u)  9,  (w)  \4  (u)  364  (w) 

+V«)  ?•(* 

-  37  (u)  57  (w)  3123  (u)  $m  (w)  -  ^  (u)  3,  (w)  9237  (u}  3237  (w)  -  32  (u)  $2  (w)  3317  (u)  9317  (w) 

-$3(u)93(w)9ia(u)9l27(w), 
where  3,  #456  denote  respectively  9  (0),  £456  (0). 

Hence  we  immediately  obtain  an  expression  for  •9456(«+  w)j§(u  +  w}  in  terms  of  theta 
quotients  $t  (u)/3  (u),  3*  (w)/&  (w). 


Ex.  xi.  The  formula  of  Ex.  i.  can  by  change  of  notation  be  put  into  a  more  symmetrical 
form  which  has  theoretical  significance.  As  before  let  TO  be  any  half-integer  even 
characteristic,  and  let  «:,  ......  ,  as  be  s,  =2",  half-integer  characteristics  such  that  every 

*  Wherein  the  notation  is  that  the  characteristic  p  is  written  (Pl  P*  Ps  }  and  p'  denotes  the 

\PiPzPs  I 
row  (  PI,  p2',  p3')  ;  and  similarly  for  the  characteristics  m,  a^. 

t  This  formula  is  given  by  Weber,  Theorie  der  AbeVschen  Functionen  vom  Geschlecht  3 
(Berlin,  1876),  p.  38. 


287]  ODD  AND   EVEN   FUNCTIONS.  461 

combination  mc^o,-,  in  which  i  is  not  equal  to  ,;',  is  an  odd  characteristic  ;  let  /,  g,  h  be 
arbitrary  half-integer  characteristics ;  let  J  denote  the  matrix  of  substitution  given  by 

J=\(-\     1     1     1), 
1-111 
1     1-1     1 
1     1     1-1 

and  from  the  arbitrary  arguments  u,  v,  w  determine  other  arguments  U,  V,  W,  T  by  the 
reciprocal  linear  equations 

(Uit  Vit  W<,  Ti}  =  J(ui,  vit  wt,  0),  (i  =  l,  2, ,  p\ 

or,  as  we  may  write  them, 

( U,  V,  \V,  T)  =  J(u,  v,  w,  0) ; 

further  determine  the  new  characteristics  F,  O,  ff,  K  by  means  of  equations   of  the 
form 

(F,  G,H,  K)=J(f,g,h,m), 

noticing  that  there  are  2p  such  sets  of  four  equations,  one  for  every  set  of  corresponding 
elements  of  the  characteristics  ; 

then  deduce  from  the  equation  of  Ex.  i.  that 

3(0;  m)3(u;f)3(t>;  g)3(w;  h) 
ZP 

A  =  l  A  '  A  ' 

Putting  m  =  0,  we  derive  the  formula 
3(0;  Q)3(v  +  w;  g+h)3(w  +  u;  h+f)  3(u  +  v;  f+g) 

=  2  3(u+v  +  w;  f+g  +  h  +  a,,)  3(u;  /—  a.)  3(v:  a  —  a  )  3  (w  h  —  a  ) 

A=l 

wherein  u,  v,  w  are  any  arguments  and/,  g,  h  are  any  half-integer  characteristics. 

Ex.  xii.  Deduce  from  Ex.  i.  that  when  jo  =  2  there  are  twenty  sets  of  four  theta 
functions,  three  of  them  odd  and  one  even,  such  that  the  square  of  any  theta  function  can 
be  expressed  linearly  by  the  squares  of  these  four. 

287.  The  number,  r?,  of  terms  in  the  expansion  of  II  (u)  may  be 
expected  to  reduce  in  particular  cases  by  the  vanishing  of  some  coefficients 
on  the  right-hand  side.  We  proceed  to  shew*  that  this  is  the  case,  for 
instance,  when  II  (u)  is  either  an  odd  function,  or  an  even  function  of  the 
arguments  u.  We  prove  first  that  a  necessary  condition  for  this  is  that  the 
characteristic  (Q,  Q')  consist  of  half-integers. 

For,  if  II  (-  u)  =  ell  (u),  where  e  is  +  1  or  -  1,  the  equation 

n<ti 

gives 


Schottky,  Abrins  einer  Theorie  der  Abel'nchen  Functional  von  drn  Varialeln  (Leipzfg,  1880). 


402  NUMBER   OF   LINEARLY    INDEPENDENT   FUNCTIONS  [287 

while,   the    left-hand   side   of  this   equation   is,  by  the   same  fundamental 
equation,  equal  to 

€er\-m{-u)-2m(mQ'-m'Q)  H  (—  w)  ' 

hence,  for  all  values  of  the  integers  m,  m',  the  expression 

r  |>m  (M)  -  \_m  (-  M)]  +  4ffiri  (mQf  -  m'Q) 
must  be  an  integral  multiple  of  2?™  ;  since,  however, 

Xm  (u)  =  Hm  (a  +  £Hm)  -  irimm  =  X_m  (-  u), 

this  requires  that  2  (raQ'  -  m'Q)  be  an  integer  ;  thus  2Q,  2Q'  are  necessarily 
integers. 

Suppose  now  that  Q,  Q'  are  half-integers;  denote  them  by  q,  q  ;  and 
suppose  that  II  (u)  =  ell  (-  u),  where  e  is  +1  or  -  1.  Then  from  the 
equation 


T 

since,  for  any  characteristic,  S-  (u,  q)  =  ^  (—  zt,  —  q),  we  obtain 


(M)  =  eH  (-  M)  =  eSJf^  (-  w  ;  q,  ^-]  =  eZK,,.*  (u  ;  -  q,  - 

/A  \  ^'/u\ 

*  L  2 

^    t*;  q  — 


where  v  is  a  row  of  positive  integers,  each  less  than  r,  so  chosen  that 

'),  (mod.  r)  ; 


thus  the  aggregate  of  the  values  of  v  is  the  same  as  the  aggregate  of  the 
values  of  p,\  therefore,  by  the  formula  (§  190),  ^(u-,  q  +  M,  q'  +  M'  ) 
.  ^  q'^  wnerein  M,  M'  are  integers,  we  have 


„    .     .  ^T.       --  V 

=  H  (u)  =  eS^e          '  ^  f  «  ;  q, 


comparing  these  two  forms  for  II  (u)  we  see  that  in  the  formula 


the  values  of  /A  that  arise  may  be  divided  into  two  sets  ;  (i)  those  for  which 
2/4  +  2q'  =  0  (mod.  r)  ;  for  such  terms  the  value  of  v  defined  by  the  previously 
written  congruence  is  equal  to  /*,  and  the  transformation  effected  with  the 
help  of  the  congruence  only  reproduces  the  term  to  which  it  is  applied  ;  thus, 

_  fX  +  g' 

for  all  such  values  of  /j,  which  occur,  e          r    is  equal  to  e  ;  (ii)  those  terms 


288]  ALL  ODD  OR  ALL  EVEN- 

_       v+V 

for  which  2/z,  +  2g'  $  °  (mod-  r)  5  for  such  terms  ^  =  e^e          r  '     Hence 
on  the  whole  II  (u)  can  be  put  into  the  form 


where  the  first  summation  extends  to  those  values  of  p  for  which 
2/A  +  2q'  =  0  (mod.  r),  and  the  second  summation  extends  to  half  those  values 
of  fj,  for  which  2//,  +  2q'  $  0  (mod.  r).  The  single  term 


which  can  also  be  written  in  the  form 


is  even  or  odd  according  as  II  (u)  is  even  or  odd  ;  and  this  is  also  true  for  the 
term  ^  (u  ;  q,  —  —  J  arising  when  2/u  +  2g'  =  0  (mod.  r). 

Hence  if  x  be  the  number  of  values  of  p,,  incongruent  for  modulus  r, 
which  satisfy  the  congruence  2/*  +  2^'  =  0  (mod.  r\  and  y  be  the  number  of 

-*ir'    ^ 

these  solutions  for  which   also  the  condition  e  r    =  e  is  satisfied,  the 

number  of  undetermined  coefficients  in  II  (u)  is  reduced  to,  at  most, 


288.  We  proceed  now  to  find  x  and  y  ;  we  notice  that  y  vanishes  when 
x  vanishes,  for  the  terms  whose  number  is  y  are  chosen  from  among  possible 
terms  whose  number  is  x.  The  result  is  that  when  r  is  even  and  the 
characteristic  (q,  q)  is  integer  or  zero,  and  II  (—  11)  =  ell  (u),  the  number  of 
terms  in  II  (u)  is  ^rf  +  2p~1e;  while,  when  r  is  odd,  or  when  r  is  even  and 
the  half-integer  characteristic  (q,  q')  does  not  consist  wholly  of  integers,  or 
zeros,  the  number  of  terms  in  II  (u)  is  ^  r?  +  £  [1  —  (—  )r]  ee4™59'. 

Suppose  r  is  even  ;  then  the  congruence  2/i  +  2q  =  0  (mod.  r)  is  satisfied 

by  taking  p.  =  M  -  —  q,  and  in  no  other  way,  M  denoting  a  row  of  p  arbitrary 

z 

integers.  Thus  unless  q'  consists  of  integers,  x  is  zero,  and  therefore,  as 
remarked  above,  y  is  zero,  and  the  number  of  terms  in  II  (11)  is  \rp.  While, 
when  q'  is  integral,  the  incongruent  values  for  /i  (modulus  r)  are  obtained  by 
taking  the  incongruent  values  for  M  for  modulus  2,  in  number  2^  ;  in  that 

_4-io^t?' 

case  x  =  2p  ;  the  condition  e  r  =  e  is  the  same  as  e~ZwiqM  '  =  e  ;  when  q  is 
integral,  this  is  satisfied  by  all  the  2P  values  of  Jl/,  or  by  no  values  of  M, 
according  as  e  is  -f  1  or  is  —  1  ;  in  both  cases  y  =  '2^~l  (1  +  e)  ;  when  q  is  not 


464  NUMBER   OF   ODD   OR   EVEN   FUNCTIONS.  [288 

integral,  p  —  1  of  the  elements  of  M  can  be  taken  arbitrarily  and  the  con 
dition  e-2«?.af=e  determines  the  other  element,  so  that  y  =  2?"1.  Thus, 
when  r  is  even,  we  have 

(1)  when   q,   q'   are    both   rows   of    integers    (including    zero),   ac  =  %p, 
y  =  2*'~1  (1  +  e),  and  the  number  of  terms  in  II  (u)  is 

2"-1  (1  +  e)  +  £  (rf  -  2»)  =  £  7*  +  %>~l  e, 

as  stated,  there  being  \  rp  +  2^-1  terms  when  II  (u)  is  an  even  function,  and 
^rp  —  %>-i  terms  when  II  (u)  is  an  odd  function  ; 

(2)  when  q'  is  integral,  and  q  is  not  integral,  #  =  2p,  y  =  2*"1,  and  there 
fore  the  number  of  terms  in  II  (u)  is 

2?-i  +  %(rP  -  2*)  =  rP, 
in  accordance  with  the  result  stated  ; 

(3)  when  q'  is  not  integral,  both  x  and  y  are  zero,  and  the  number  of 
terms  is  ^r?,  also  agreeing  with  the  given  formula. 

Suppose  now  that  r  is  odd,  then  the  equation 

rM-2q'                        M-2q' 
2/1,  +  2q  =  rM,  or  p  = ^-±- ,  =  integer  + 1-4  , 

wherein  Jlf  is  a  row  of  integers,  requires  M  to  have  the  form  2q'  +  22V,  where 
.2V  is  a  row  of  integers,  and  therefore 


this  equation,  since  p  consists  of  positive  integers  all  less  than  r,  determines 
the  value  of  N  uniquely  ;  hence  x  =  1.     The  condition 


determines  y  =  1  or  y  =  0   according  as  ee^iqq'  =  +  1   or  =  —  1  ;    hence   the 
number  of  terms  in  II  (u)  is 


-,  or 

according  as  ee^iqq'  =  +  1  or  —  1  ;  this  agrees  with  the  given  result  when  r  is 
odd,  the  number  of  terms  being  always  one  of  the  numbers  £(r*>  +  1). 

289.  It  follows  from  the  investigation  just  given  that  if  we  take  pro 
ducts  of  theta  functions,  forming  odd  or  even  theta  functions  of  order  r,  with 
the  same  half-integer  characteristic  (q,  q),  and  associated  with  the  same 
constants  2o>,  2&/.  2?/,  2?/,  then  when  r  is  even,  the  number  of  these  which 
are  linearly  independent  is,  at  most,  |  T?  +  ^>~l  e  when  the  characteristic  is 
integral  or  zero,  and  is  otherwise  \r?  ;  while,  when  r  is  odd,  the  number 
which  are  linearly  independent  is,  at  most,  |  (rP+ee^w'),  e  being  ±  1  accord 
ing  as  the  products  are  even  or  odd  functions. 


289]  GOPEL'S  BIQUADRATIC  RELATION.  465 

Ex.  i.  In  case  jt?  =  2  there  are  six  odd  characteristics,  and  the  sum  of  any  three  of 
them  is  even*,  as  the  reader  can  easily  verify  by  the  table  of  page  303.  Let  a,  /3,  y,  8,  e,  f 
denote  the  odd  characteristics,  in  any  order,  and  let  a/3y  denote  the  characteristic  formed 
by  adding  the  characteristics  a,  ;3,  y.  Then  the  product 

n(u)  =  3  (u,  a)  3  (u,  ft)  3  (u,  y)  3  (u,  afty) 

is  an  odd  theta  function  of  the  fourth  order  with  integral  characteristic.     Hence  this 
product  can  be  written  in  the  form 


where  p.  has  the  42  values  arising  by  giving  to  each  of  the  two  elements  of  /*,  independently 
of  the  other,  the  values  0,  1,  2,  3.     Changing  the  sign  of  u  we  have 


where  v  is  chosen  so  that 

^  +  i/  =  0(mod.  4). 

This  congruence  gives  16  values  of  v  corresponding  to  the  16  values  of  /x;   of  these 
there  are  4  values  for  which  n=v  and  2/x=0  (mod.  4)  ;  these  are  the  values 

M  =  (0,0),    (0,2),    (2,0),    (2,2), 

greater  values  for  the  elements  of  /*  being  excluded  by  the  condition  that  these  elements 
must  be  less  than  4.     We  have  by  the  formula  (§  190)  3  (u;  q  +  M)  =  eZlriMi'  3  (u), 


comparing  this  with  the  original  formula  for  n  (u},  we  see  that 


so  that  the  terms  in  the  original  formula  for  n(u)  for  which  v=p  are  absent,  and  the 
remaining  twelve  terms  may  be  arranged  as  six  terms  in  the  form 


where  the  summation  extends  to  the  following  values  of  /*, 

M  =  (0,  1),   (1,0),    (1,1),   (1,2),    (1,3),    (2,3); 

these  values  may  be  interchanged  respectively  with 

M  =  (0,3),    (3,0),    (3,3),    (3,2),    (3,1),    (2,1), 

if  a  proper  corresponding  change  be  made  in  the  coefficients  A.^. 


The  number  6  is  that  obtained  from  the    formula  $i*  +  2p-le,   by   putting  r  =  4, 
f=-l,  p  =  2. 

Ex.  ii.     In  case  p  =  2,  denoting  the  odd  characteristics  by  a,  ft,  y,  8,  t,  £,  and  the  sum 
of  two  of  them,  say  a  and  /3,  by  a£,  and  so  on,  each  of  the  four  products 

3  (11,  a)  3  (u,  oefl,  3  (u,  ft)  3  (u,  /3,f),  3  (u,  y)  3  (u,  y({),  3  (u,  d)  3  (u, 


or,  in  Weierstrass's  notation,  if  a,  ft,  y,  8,  e,  f  be  taken  in  the  order  in  which  they  occur  in 
the  table  of  page  303,  each  of  the  products 


*  This  is  a  particular  case  of  a  result  obtained  in  chapter  XVII. 

"•  30 


466  GOPEL'S  BIQUADRATIC  RELATION.  [289 

is   an  odd  theta  function  of  order  2,  and  of  characteristic  differing  only  by  integers 
from  the  characteristic  denoted  by  «£,  or,  in  the  arrangement  here  taken,  £  (      j  ;  thus 

any  three  of  these  products  are  connected  by  a  linear  equation  whose  coefficients  do  not 
depend  upon  u. 

Similarly  each  of  the  products 

3  (u,  aSe)  3  (u,  aSO,    -9  (^  08*)  3  («,  /Mflt    5  (u,  78f)  3  (u,  ySf),  *  (u,  0  3  (u,  f), 

or,  in  Weierstrass's  notation,  if  a,  £,  y,  8,  e,  f  be  taken  in  the  order  in  which  they  occur 
in  the  table  of  p.  303,  each  of  the  products 

314(«)V»),   3oi(*)V»),   SiM^M,   Si3(tt)S8(tt), 
is  an  even  theta  function  of  order  2,  and  of  characteristic  differing  only  by  integers 

from  the  characteristic  denoted  by  e£,  or,  in  the  arrangement  here  taken,  £  (      j  ;  thus 

any  three  of  these  products  are  connected  by  a  linear  equation  whose  coefficients  do  not 
depend  upon  u. 

Ex.  iii.  For  p  =  2  the  number  of  linearly  independent  even  theta  functions  of  the 
fourth  order  and  of  integral  characteristic  is  £42  +  2  =  10.  If  q,  r  be  any  half-integer 
characteristics,  it  follows  that  any  eleven  functions  of  the  form  32  (u,  q)  32  (u,  r)  are 
connected  by  a  linear  equation.  Taking  now,  with  Weierstrass's  notation,  the  four 
functions* 

t  =  $&(u),   x  =  3M(u),  ,y  =  312(tt),   z  =  \(u\ 

it  follows  that  there  exists  an  identical  equation 


in  which  the  eleven  coefficients  A0,  ......  ,  H2  are  independent  of  u. 

The  characteristics  of  the  theta  functions  #6(«),  ^(u),  3l2(u),  B0(u)  may  be  taken, 
respectively,  to  be  (cf.  §  220,  Chap.  XL) 

/O,  0\  ,   /O,  0\  _  //>/,  P2'\  .  A  0\  _  /ft',  ?2'\  /O,  0\  _  /<,  rA  . 

U  oj  '  u  i;  -  U.«;  '  y  '  Vi  oj  -  u,  &  ;  '  y  '  U  y  ~  W;  v  '  y  ' 

hence,  by  the  formulae  (§  190) 

5(M  +  0P;  ?)  =  eA^M)-2'riP'^(u;  q  +  p),$(U't  q  +  M  }  =  <?***'  3  (u  •  q], 
wherein  M  denotes  a  row  of  integers,  we  obtain 

35  (U  +  Op)  =  «M«>  ^34  («)>    ^34  («  +  0P)  =  ^(W>  -»6  («)>    512(«  +  Op)  =  <^(M)  ^0  («), 


hence  the  substitution  of  u  +  Qp  for  u  in  the  identity  replaces  t,  x,  y,  z  respectively  by 
x,  t,  z,  y.     Comparing  the  new  form  with  the  original  form  we  infer  that 


Similarly  the  substitution  of  u  +  Qq  for  u  replaces  t,  x,  y,  z  respectively  by  y,  z,  t,  x  ; 
making  this  change,  and  then  comparing  the  old  form  with  the  derived  form,  we  infer 
that 


*  Which  are  all  even  and  such  that  the  square  of  every  other  theta  function  is  a  linear 
function  of  the  squares  of  these  functions.  It  can  be  proved  that  these  functions  are  not 
connected  by  any  quadratic  relation. 


289]  NUMBER   OF   SUCH    RELATIONS.  467 

Thus  the  identity  is  of  the  form 


Taking  now  the  three  characteristics 

(&',  /A  =  /O,  i\     /<?/,  <72'\  _  ft,  0\     //V,  h2'\  _  ft,  £\ 

v/i,  fj  \o,  oj  '  u>  ffj  ~  vo,  <>;  '  U.  v  "  v>,  o;  > 


and  adding  to  the  argument  u,  in  turn,  the  half-periods  Q,,  a,,  OA  and  then  putting  u  =  0, 
we  obtain  the  three  equations 


where  3*  denotes  ^(0),  etc.,  and  the  notation  is  Weierstrass's,  as  in  §  220.  By  these 
equations  the  constants  F,  G,  H  are  determined  in  terms  of  zero  values  of  the  theta 
functions.  The  value  of  C  can  then  be  determined  by  putting  u  =  Q  in  the  identity 
itself. 

Thus  we  may  regard  the  equation  as  known  ;  it  coincides  with  that  considered 
in  Exx.  i.  and  iv.  §  221,  Chap.  XL,  and  represents  a  quartic  surface  with  sixteen  nodes. 
With  the  assumption  of  certain  relations  connecting  the  zero  values  of  the  theta  functions, 
proved  by  formulae  occurring  later  (Chap.  XVII.  §  317,  Ex.  iv.),  we  can  express  the 
coefficients  in  the  equation  in  terms  of  the  four  constants  S6(0),  SM(0),  5ia(0),  40(0). 
We  have  in  fact,  if  these  constants  be  respectively  denoted  by  d,  a,  b,  c 


hence  the  identity  under  consideration  can  be  put  into  the  form 


^-^+*^ 

where  the  ri  denotes  the  product  of  the  four  factors  obtained  by  giving  to  each  of  Cl,  e2 
both  the  values  +1  and  -1.  The  quartic  surface  represented  by  this  equation  (Ma 'be 
immediately  proved  to  have  a  node  at  each  of  the  sixteen  points  which  are  obtainable 
from  the  four, 

(d,  a,  6,  c),  (d,  a,  -b,  -c),  (d,  -a,  b,  -c),  (d,  -a,  -b,  c), 
by  writing  respectively,  in  place  of  d,  a,  b,  c, 

(i)  (d,  a,  b,  c),    (ii)  (a,  d,  c,  6),    (iii)  (b,  c,  d,  a),    (iv)  (c,  b,  a,  d). 
Ex.  iv.     We  have  in  Ex.  iii.  obtained  a  relation  connecting  the  functions 

in  Ex.  iv.  §  221  we  have  obtained  the  corresponding  relation  connecting  the  functions 

and  in  Ex.  i.  §  221  we  have  explained  how  to  obtain  the  corresponding  relation  connecting 
the  functions 


30—2 


468  EXAMPLES.  [289 

There  are*  in  fact  sixty  sets  of  four  functions  among  which  such  a  relation  holds  ;  and 
these  sixty  sets  break  up  into  fifteen  lots  each  consisting  of  four  sets  of  four  functions, 
such  that  in  every  lot  all  the  sixteen  theta  functions  occur,  and  such  that  in  every  lot  one 
of  the  sets  of  four  consists  wholly  of  even  functions  while  each  of  the  three  other  sets 
consists  of  two  odd  functions  and  two  even  functions.  This  can  be  seen  as  follows  :  using 
the  letter  notation  for  the  sixteen  functions,  as  in  §  204,  and  the  derived  letter  notation 
for  the  fifteen  ratios  of  which  the  denominator  is  9  (u),  as  at  the  top  of  page  338,  it  is 
immediately  obvious,  as  on  page  338,  that  any  four  ratios  of  the  form 

l>  2*,*.  2Al.V  2*,  » 

in  which  the  letters  k,  I,  £lf  llt  k%  constitute  in  some  order  the  letters  alt  «2,  c>  ci>  C2>  are 
connected  by  a  relation  of  the  form  in  question.  Now  such  a  set  of  four  ratios  can  be 
formed  in  fifteen  ways  ;  there  are  firstly  six  such  sets  in  which  all  the  ratios  are  even 
functions  of  u,  obtainable  from  the  set 

1>  2e»  2a,,  c,»  ?aa,  c3 

by  permuting  the  three  letters  c,  clt  c2  among  themselves  in  all  possible  ways  ;  and  nextly 
nine  such  sets  in  which  two  of  the  ratios  are  odd  functions,  obtainable  from  the  set 


by  taking  instead  of  the  pair  a^  each  of  the  three  pairs  t  a1«2,  aalt  aa2,  and  instead  of 
the  pair  CjC2  each  of  the  three  pairs  c^,  ccj,  cc2.  Since  (§  204)  the  letter  notation  for  an 
odd  function  consists  always  of  two  a-s  or  two  e-s,  and  for  an  even  function  consists  of 
one  a  and  one  c,  the  number  of  odd  and  even  functions  will  remain  unaltered.  Further 
from  each  of  these  fifteen  sets  we  can  obtain  three  other  sets  of  four  ratios  by  the  addition 
of  half-periods  to  the  argument  u,  in  such  a  way  that  all  the  sixteen  theta  functions 
enter  into  each  lot  of  sets.  The  fifteen  lots  obtained  may  all  be  represented  by 
the  scheme 

1,         a    ,         /3    ,         a/3 

«i  >       aai  >       ^ai  >       a/3ai 

ft  ,       aft  ,        #3,  ,       a/3ft 

ajft,     aajft,     /Sajft,     a/3aift, 

where  1,  a,  ft  a/3  denote  the  characteristics  of  one  of  the  fifteen  sets  of  four  theta  functions 
just  described,  such  as  S  (u),  &e(u),  \Ci  (w),  ^  (u),  or  &(u),  $c(u),  \tta  («),  ^(u), 
aft  denoting  the  characteristic  formed  by  the  addition  of  the  characteristics  a,  /3  ;  and  at  ,  ft 
denote  any  other  two  characteristics  other  than  a,  ft  or  aft  and  such  that  a/3  is  not  the 
same  characteristic  as  axft.  This  scheme  must  contain  all  the  sixteen  theta  functions  ; 
for  any  repetition  (such  as  a  =  /3ajft,  for  example)  would  be  inconsistent  with  the 
hypothesis  as  to  the  choice  of  a,,  ft  (would  be  eqxiivalent  to  a^  =  ajft).  It  is  easily  seen, 
by  writing  down  a  representative  of  the  six  schemes  in  which  the  first  row  consists 
wholly  of  even  functions,  and  a  representative  of  the  nine  schemes  in  which  the  first 
row  contains  two  odd  functions,  that  in  every  scheme  there  are  three  rows  in  which  two 
odd  functions  occur  J. 

Ex.  v.  There  are  cases  in  which  the  number  of  linearly  connected  theta  functions,  as 
given  by  the  general  theorem,  is  subject  to  further  reduction.  For  instance,  suppose  we 

*  Borchardt,  Crelle,  LXXXIII.  (1877),  p.  237.  Each  of  the  sixty  sets  of  four  functions  may  be 
called  a  Gopel  tetrad. 

t  The  letter  a,  when  it  occurs  in  a  suffix,  is  omitted. 

J  A  table  of  the  sixty  sets  of  four  theta  functions  is  given  by  Krause,  Hyperelliptische 
Functionen  (Leipzig,  1886),  p.  27. 


289]  REDUCTION    OF   THE   CHARACTERISTIC.  469 

have  w  =  2p~1  odd  half-integer  characteristics  Alt  ...,  Jm,  and  another  half-integer  charac 
teristic  P,  not  (integral  or)  zero,  such  that  the  characteristics*  A{P,  ...,  AmP,  obtained 
by  adding  P  to  each  of  Alt  ...,  Am,  are  also  odd  +  ;  suppose  further  that  A  is  an  even 
half-integer  characteristic,  and  that  ylPis  also  an  even  characteristic,  and  that  the  theta 
functions  3  (u  ;  A),  3(u;  AP)  do  not  vanish  for  zero  values  of  the  argument.  Then,  by 
§  288  the  W^  +  l  following  theta  functions  of  order  2, 

3(u;  A)3(u;  AP),  3  (u  •  Al)3(u;  A,P),  ...,  3(u;  Am)3(u;  AmP), 

which  are  all  even  functions  with  a  characteristic  differing  only  by  integers  from  the 
characteristic  P,  are  connected  by  a  linear  equation  with  coefficients  independent  of  u. 
But  in  fact,  if  we  put  u  =  0,  all  these  functions  vanish  except  the  first.  Hence  we  infer 
that  the  coefficient  of  the  first  function  is  zero,  and  that  in  fact  the  other  2p~l  functions  are 
themselves  connected  by  a  linear  equation. 

Ex.  vi.  In  illustration  of  the  case  considered  in  Ex.  v.  we  take  the  following  :  —  When 
/>  =  3,  it  is  possible  £,  if  P  be  any  characteristic  whatever,  to  determine  six  odd  characteristics 
A19  ...,  A6,  whose  sum  is  zero,  such  that  the  characteristics  AtP,  ...,A6P&re  also  odd,  and 
such  that  all  the  combinations  of  three  of  these,  denoted  by  AiAjAk,  AiAjAkP,  are  even. 
By  the  previous  example  there  exists  an  equation 

AS  (u  ;  J4)  3  (u  ;  J4P) 

;  A2)3(u;  A2P)+\33(u;  As)  3  (u  •  A3P), 


wherein  X,  A1}  A2,  A3  are  independent  of  u.     Adding  to  u  any  half-period  Qfi,  this  equation 
becomes 


A3  (u  ;  AiQ)  3  (u  ;  AtPQ) 
=  X1«1S(M;  AlQ)S(u;  A1PQ)  +  \2f23(u;  A2Q)3(u;  AzP<j)  +  \^(u;  A3Q)3(u;  A3PQ), 

where  fi(i=l,  2,  3)  is  a  certain  square  root  of  unity  depending  on  the  characteristics 
^4>  ^i>  P,  Q,  whose  value  is  determined  in  the  following  example.  Taking  in  particular 
for  Q2  the  half-period  associated  with  the  characteristic  AZA3,  so  that  the  characteristics 
A2PQ,  A3PQ  become  respectively  the  odd  characteristics  A3P,  A2P,  and  putting  «  =  0, 
we  infer 

A4(0;  A4AZA3)3(0-  A,A2A3P)  =  \lfl'3(0  •  ^2J3)3(0;  A,A2A3P), 

where  */  is  the  particular  value  of  fl  when  Q  is  A2A3.  This  equation  determines  the  ratio 
of  At  to  A  ;  similarly  the  ratios  A2  :  A  and  A3  :  A  are  determinable. 

Ex.  vii.     If  £r,  $q  be  half-integer  characteristics  whose  elements  are  either  0  or  £,  and 
$k=$rq  be  their  reduced  sum,  with  elements  either  0  or  £,  prove  §  that 

*.  =  »-.  +  ?.-2rB?a>     *.'  =  »-.'  +  ?.'-  2ra'?a',         (a  =  l,2,  ...,p), 
and  thence,  by  the  formulae  (§  190) 

e**™*  S  (u  ;  2), 


*  A  characteristic  formed  by  adding  two  characteristics  A,  P  is  denoted  by  A  +  P.  Its 
reduced  value,  in  which  each  of  its  elements  is  0  or  £,  is  denoted  by  AP. 

t  It  is  proved  in  chapter  XVII.  that,  when  j»2,  the  characteristic  P  may  be  arbitrarily 
taken,  and  the  characteristics  Alt...,Am  thence  determined  in  a  finite  number  of  ways. 

t  This  is  proved  in  chapter  XVII. 

§  Schottky,  Crelle,  en.  (1888),  pp.  308,  318. 


EXAMPLES.  [289 


where  M  is  integral,  prove  that 

X  (u  ;  i  r\  +  wi  I  (raga?a'  +  gjy-J 
3  (w+i  QP  ;£?)  =  « 
If  ^  ^a,  \q  be  any  reduced  characteristics,  infer  that 


where 

«r  2  [ragfta.'  +  (raga'  +  ra'?a  +  ra')  o  J 
e  =  e    a=1  -;  .; 

^p.  viii.  If  ^u  ^42,  ^3,  AI  denote  four  odd  characteristics,  for  jt>  =  2,  and  5  denote  an 
even  characteristic,  the  12»  +  2P-1  +  1  =  5  theta  functions,  of  order  2  and  zero  (or  integral) 
characteristic,  &(u;  B),  &(u;  AJ,  ...,52(«;  Aj  are,  by  §  288,  connected  by  a  linear 
equation.  As  in  Ex.  v.  we  hence  infer  an  equation  of  the  form 


adding  to  w  the  half-period  associated  with  the  characteristic  AZA3,  and  putting  M=0,  we 
deduce  by  Ex.  vii.  that 

Xe**1'0*  52  (0  ;  A,AzA.}  =  \,eivk^  V  (0  ;  ^^2^3), 

where  A2Az  =  \k^  Al  =  ^a1,  ^4  =  ^a4.     Hence  we  obtain  an  equation  which  we  may  write 
in  the  form 


where  (A^At3\  denotes  a  certain  square  root  of  unity.    Such  a  relation  holds  between  every 

VM4/ 

four  of  the  odd  theta  functions. 

If  A  !,...,  A6  be  the  odd  characteristics,  and  Q  be  any  other  characteristic,  the  six 
characteristics  A$t  ...,  A6Q  are  said  to  form  a  Kosenhain  hexad.  It  follows  that  the 
squares  of  every  four  theta  functions  of  the  same  hexad  are  connected  by  a  linear  relation. 


291] 


CHAPTER    XVI. 

A  DIRECT  METHOD  OF  OBTAINING  THE  EQUATIONS  CONNECTING  ^-PRODUCTS. 

290.  THE  result  given  as  Ex.  xi.  of  §  286,  in  the  last  chapter,  is  a 
particular  case  of  certain    equations  which    may  be    obtained    by  actually 
multiplying   together   the   theta   series    and    arranging    the   product   in   a 
different  way.     We  give  in  this  chapter  three  examples  of  this  method,  of 
which  the  last  includes  the  most  general  case  possible.     The  first  two  furnish 
an  introduction  to  the  method   and  are    useful   for   comparison    with    the 
general  theorem.     The  theorems  of  this  chapter  do  not  require  the  charac 
teristics  to  be  half-integers. 

291.  Lemma.     If  b  be  a  symmetrical  matrix  of  p2  elements,  U,  V,  u,  v, 
A,  B,  f,  g,  q,  r,f,  g',  q',  r,  M,  N,  s,  t',  m,  n  be  columns,  each  of  p  elements, 
subject  to  the  equations 

n  -f  m  =  2N  +  *',         q'  +  r'=f',         q  +  r=f, 


then 

2  U  (n  +  q)  +  b  (n  +  qj  +  Zniq  (n  +  q')  +  2  V  (m  +  r')  +  b  (m  +  rj  +  2-Trir  (m  +  r') 

±/'  +  26 


This  the  reader  can  easily  verify. 

Suppose  now  that  the  elements  of  s  and  t'  are  each  either  0  or  1,  and 
that  n  and  m  take,  independently,  all  possible  positive  and  negative  integer 
values.  To  any  pair  of  values,  the  equations  n  +  m  =  2JV  +  s',  —  n  +  m  =  2M  +  1' 
give  a  corresponding  pair  of  values  for  integers  N  and  M,  and  a  pair  of 
values  for  s'  and  t'.  Since  2m  =  2JV+  2M  +  s'  +  t',  s'  +  t'  is  even,  and  there 
fore,  since  each  element  of  s'  and  t'  is  <  2,  s'  must  be  equal  to  t'.  Hence  by 
means  of  the  2?  possible  values  for  s',  the  pairs  (n,  m}  are  divisible  into  2^ 
sets,  each  characterised  by  a  certain  value  of  s'.  Conversely  to  any  assignable 


472  ACTUAL   CALCULATION   OF   PRODUCT  [291 

integer  value  for  each  of  the  pair  (N,  M)  and  any  assigned  value  of  s  (<  2) 
corresponds  by  the  equations  n  =  N—M,  m  =  N+M  +  s'  a  definite  pair  of 
integer  columns  n,  m. 

Hence,  b  being  such  a  matrix  that,  for  real  x,  ba?  has  its  real  part  negative, 

(n+tf)  +b  (n+q1)  «  +2mq  (n+q')  j  T^g2  V  (m+r')  +b  (m+r1)  s+2jrir  (m+r')  1 
m 

-z 


thus,  if  *(u;   \),  or  *u;         ,  denote  S^ujn+vj+Kn+vj^+shrtxjn+x^  ^(Mj  X)  or 

V          A,/  n 

/       A/\ 
^  ft*;         denote  2e4M(n+V)+26(n+v>2+2'riA(n+v>,  we  have 

V       A/  n 


_ 

where  the  equation  on  the  right  contains  2?  terms  corresponding  to  all 
values  of  s',  which  is  a  column  of  p  integers  each  either  0  or  1  ;  all  other 
quantities  involved  are  quite  unrestricted. 

Therefore  if  a  be  a  symmetrical  matrix  of  p*  elements  and  h  any  matrix 
of  p-  elements,  we  deduce,  replacing  u  by  hu,  and  v  by  hv,  and  multiplying 
both  sides  by  eau'+av\  the  result 


where  e  denotes  all  possible  2^  columns  of  p  elements,  each  either  0  or  1, 
and  ^  differs  from  S-  only  by  having  2a,  2h,  2b  instead  of  a,  h,  b  in  the 
exponent  ;  thus  we  may  write,  more  fully, 

2&), 


jEvp.  i.     When  the  characteristics  q,  r  are  equal  half-integer  characteristics,  say 

>',  ""i  '- 

the  equation  is 


multiplying  this  equation  by  ewwn,  when  n  denotes  a  definite  row  of  integers,  each  either 


291]  OF  TWO   THETA   FUNCTIONS.  473 


0  or  1,  and  adding  the  equations  obtained  by  ascribing  to  a  all^he  2^'  possible  sets  of  values 
in  which  each  element  of  a  is  either  0  or  1,  we  obtain 


for  we  have 


a  f=l 

Ex.  ii.     Deduce  from  Ex.  i.  that  when  p  =  l,  the  ratio  of  the  two  functions 


is  independent  of  «.. 

^r.  iii.     Prove  that  the  2?>  functions  ^  (  u  ;         ft       )  j  obtained  by  varying  «',  are  not 
connected  by  any  linear  equation  with  coefficients  independent  of  u. 

Ex.  iv.     Prove  that  if  a,  a'  be  integral, 


From  this  set  of  equations  we  can  obtain  the  linear  relation  connecting  the  squares  of 
(or  less)  assigned  theta  functions  with  half-integer  coefficients. 

Ex.  v.     Using  the  notation  (X,-,,-)  for  the  matrix  in  which  the  j-th  element  of  the  i-th 
row  is  Xf,y,  prove  that  if  ul,  ...,  u,.,  vt,  ...,  vr  be  2.2?  arguments,  and  $(a  J  any  half- 


integer  characteristic, 


.[•>'  *o] 


and,  denoting  the  determinant  of  the  matrix  on  the  left  hand  by  {?/f,  v}}  and  the  determi 
nant  of  the  second  matrix  on  the  right  hand  by  {v},  deduce  that 


where  A  is  the  sum  of  the  p  elements  of  the  row  letter  a.     When  the  characteristic  |  (     J 

is  odd,  {u(,  Uj}  is  a  skew  symmetrical  determinant  whose  square  root  is*  expressible 

tionally  in    terms    of   the    constituents    $Ffc|+1^j    i{*  ji  *[««<-%  i    iff]-      For 


instance  when  p  =  I,  we  obtain,  with  a  proper  sign  for  the  square  root,  the  equation  of 
three  terms  t. 

Since  any  2*  +  1  functions  of  the  form  3  \  u+vp  ;  \  (  a  J    5  1  u  -  vp  ;  %  (  a  j  |  are  connected 

by  a  linear  equation  with  coefficients  independent  of  u,  it  follows  that  if  w1?  ...,  um, 
vi>  ...»  ^m  be  any  2m  arguments,  m  being  greater  than  2",  the  determinant  of  m  rows  and 

columns,  whose  (/,  »th  element  is  *|n+«y;  ^  (°)~|^  F^-  vs  ;  i(")l,  vanishes  identi 
cally.     When  ^  f  a  j  is  odd  and  m  is  even,  for  example  equal  to  2"  +  2,  this  determinant  is 

*  Scott,  Theory  nf  determinants  (Cambridge,  1880),  p.  71. 
t  Halphen,  Fonet.  EUip.  (Paris,  1886),  t.  I.  p.  187. 


474  CALCULATION    OF   THE   PRODUCT  [291 

a  skew  symmetrical  determinant  whose  square  root  may  be  expressed  rationally  in  terms  of 
the  functions  5|  tlf-HV  j  ill  rH  ui~vi  >  if)  •  The  resu^  obtained  may  be  written 

{ut,  «,-}*  =  (), 

wherein*  the  determinant  {uit  v}]  has  m  rows  and  columns,  m  being  even  and  greater  than 
2  p.  When  m  is  odd  the  determinant  {«;,  Vj]  itself  vanishes. 

A  proof  that  for  general  values  of  the  arguments  the  corresponding  determinant 
{ut,  ^j},  of  2P  rows  and  columns,  does  not  identically  vanish  is  given  by  Frobenius,  Crelle, 
xcvi.  (1884),  p.  102. 

A  more  general  formula  for  the  product  of  two  theta  functions  is  given  below 
Ex.  ii.  §  292. 

292.  We  proceed  now  to  another  formula,  for  the  product  of  four  theta 
functions.  Let  J  denote  the  substitution 

l         1         1         1), 
1-111 
11-11 
111-1 

and  Jrs  be  the  element  of  the  matrix  which  is  in  the  r-th  row  and  the  5-th 

4 

column  ;  then  2  Jir  Jis  =  0  or  1,  according  as  r  =f=  s,  or  r  =  s  (r,  s  =  1,  2,  3,  4). 

i  =  l 

Let  MU  u2,  u3,  u4  denote  four  columns,  each  of  p  quantities;  written  down 
together  they  will  form  a  matrix  of  4  columns  and  p  rows.  Let  U1}  U2,  U3, 
U4  be  four  other  such  columns,  such  that  the  j-th  row  of  the  first  matrix 
(j  =  1,  2,  ...,  p)  is  associated  with  thej-th  row  of  the  second  by  the  equation 


Let  vlt  vz,  v3,  v4  and  V1}  F2,  Vs,  V4  be  two  other  similarly  associated  sets, 
each  of  four  columns  of  p  elements.  Then  if  h  be  any  matrix  whatever,  of  p 
rows  and  columns,  we  have 

hu^  +  h  uzvz  +  hu3v3  +  hu4v4  =  hU1V1  +  hU2V2  +  hU3V3  +  hUtV^; 

this  is  quite  easy  to  prove  :  an  elementary  direct  verification  is  obtained  by 
selecting  on  the  left  the  term  hj^u^v^j  +  hjk(u2)k(vz)j+hjk(u3)k(v3)j+  hj 

=  hjk  2  [Jrl  (  ujk  +  J*  (  u,\  +  Jr3  (  u3)k  +  Jr4  (  u4)k]  [Jrl 


=  hk 


=  hjk  {(U1\(Vl)j  +  (U2)k  (F2)j 

and  this  is  the  corresponding  element  of  hUl  Vl  +  hU2V2  +  hU3V3  +hU4V4. 

*  The  theorem  was  given  by  Weierstrass,  Sitzungsber.  der  Berlin.  Ak.  1882  (i.  —  xxvi.,  p.  506), 
with  the  suggestion  that  the  theory  of  the  theta  functions  may  be  a  priori  deducible  therefrom,  as 
is  the  case  when|?  =  l  (Halphen,  Fonct.  Ellip.  (Paris  (1886)),  t.  i.  p.  188).  See  also  Caspary, 
Crelle,  xcvi.  (1884),  and  ibid.  xcvu.  (1884),  and  Frobenius,  Crelle,  xcvi.  (1884),  pp.  101,  103. 


292]  OF   FOUR  THETA   FUNCTIONS.  475 

Now  we  have 
Sr  (Ml,  ?1)  ^  (u.2,  qa)  $•  (u3,  q3} 


In  the  exponent  here  there  are  four  sets  each  of  four  columns  of  p  quantities 
namely  the  sets 

Mr,    Kr,    qr,    tfr', 

we  suppose  each  of  these  transformed  by  the  substitution  J.     Hence  the 
exponent  becomes 


Flf  2T,,  2T,.  JT, 

wherein  the  summation  extends  to  all  values  of  Nrj  given  by 

t 
Nrj  =  %  (nl}  +  nzj  +  n3j  +  n4j  -  2nrj), 

for  which  all  of  nrj  are  integers. 

All  the  values  Nrj  will  not  be  integral.  But  since  Nrj  —  Ngj  =  rigj  —  nrj  the 
fractional  parts  of  N^,  N2j,  N3j,  Ntj  will  be  the  same,  =  £  e/,  say,  (e/  =  0  or  1). 
Let  rrirj  be  the  integral  part  of  Nrj.  We  arrange  the  terms  of  the  right  hand 
into  %P  classes  according  to  the  2?  values  of  e/.  Then  since 


every  term  of  the  left-hand  product,  arising  from  a  certain  set  of  values  of 
the  4>p  integers  nrj,  gives  rise  to  a  definite  term  of  the  transformed  product  on 
the  right  with  a  definite  value  for  e/,  while,  since 


every  assignable  set  of  values  of  the  4<p  integers  mrj  and  value  for  e/  (which 
would  correspond  to  a  definite  term  of  the  transformed  product)  will  arise, 
from  a  certain  term  on  the  right,  provided  only  the  values  assigned  for  mrj  be 
such  that  ^  (rn^j  +  m%j  +  m3j  +  m4j  +  e/)  is  integral. 


Now  we  can  specify  an  expression  involving  the  quantities 

A*j,  =1  0»ij  +  m*j  +  msj  +  m4j  +  c/), 

which  is  1  or  0  according  as  ft  =  (/A1,  /A2,  ...,  fip)  is  a  column  of  integers  or 
not.  In  fact  if  e  =  (e!,  ...,  ep)  be  a  column  of  quantities  each  either  0  or  1  — 
so  that  e  is  capable  of  2^  values  —  the  expression 

J_  2e*nV  =  1  (^ea-nv.M,)  .  .  .  (^ez™^  =  J_  (i  +  e2«>,)  (j  +  ezm^  .  .  .  (i  +  #**,) 

has  this  property  ;  for  when  ^  ,  .  .  .  ,  /j.p  are  not  integers  they  are  half- 
integers. 


476  FOUR  THETA   FUNCTIONS.  [292 

Hence  if  the  series  =-  2e7ri'6(mi+"l2+m3+m<+O  be  attached  as  factor  to  every 

2P  f 

term  of  the  transformed  product  on  the  right  we  may  suppose  the  summation 
to  extend  to  all  integral  values  of  mrj,for  every  value  of  e. 

Then  the  transformed  product  is 

1 


V          pZaUr+VZhUr  (mr+be'+Q'rl+'S.b  (mr+K+Q'r)2+2Jrt2Qr  (mr+Je'  +  QVl+jrie  (?«,+Jn1!+?ft3+m1+e') 
Op 

sf  mlm.im3m,te 

1  2 

=  _  ^n^Ur+'ihUr  (mr+p'r)+b  (mr+p'r)  *+2iripr  (mr+p'r)  _  Q~^f  (2pV-«'> 

2P     r 
where 

Pr=^€+Qr,      Pr=^€+Qr, 

so  that 

2p/=2e'  +  2Q/=2e'  +  %'. 
Thus  we  have 

S-  (MJ,  g,)  ^  (u2,  qj  %  (u3,  q3)  ^  (w4,  q4) 

'^ 


This  very  general  formula  obviously  includes  the  formula  of  Ex.  xi.,  §  286, 
Chap.  XV.  It  is  clear  moreover  that  a  similar  investigation  can  be  made  for 
the  product  of  any  number,  k,  of  theta-functions,  provided  only  we  know  of  a 
matrix  J,  of  k  rows  and  columns,  which  will  transform  the  exponent  of  the 
general  term  of  the  product  into  the  exponent  of  the  general  term  of  the  sum 
of  other  products. 

It  is  for  this  more  general  case  that  the  next  Article  is  elaborated. 
It  is  not  necessary  for  either  case  that  the  characteristics  q1}  q2,  ...  should 
consist  of  half-integers. 

Ex.  i.     If  q  be  a  half-  integer  characteristic,  =  Q,  say,  and  we  use  the  abbreviation 

0(M,  v,  w,  t\  Q)  =  $(u;  Q)3(v,  0)3(1*',  0)*(t>  Q}, 
we  have 

i 

(f)(u  +  a,  u-a,  v  +  b,  v-b,  Q)  =  ^  2  e~nife'  <f>[u  +  b,  u-b,  v  +  a,  v-a  ; 

•  f,f' 

where  the  summation  on  the  right  hand  extends  to  all  possible  22p  half-integer  character 
istics  £  r  J  ;  putting  Q  +  $(f\  =  R,  so  that  R  also  becomes  all  22^  half-integer  character 
istics,  this  is  the  same  as 


,  u-a,  v  +  b,  v-b;  Q)  =    >2e"ilQ'  Rl  +  wi  [Rl  <f>(u  +  b,  u-b,  v  +  a,  v-a;  R), 
where, 
if  <? 


293] 


GENERAL   CASE. 


477 


By  adding,  or  subtracting,  to  this  the  formula  derived  from  it  by  interchange  of  v  and 
a,  we  obtain  a  formula  in  which  only  even  or  odd  characteristics  R  occur  on  the  right  hand. 
Thus,  for  p  =  l,  we  derive  the  equation  of  three  terms. 

Ex.  ii.  If  a,  |3,  y,  8  be  integers  such  that  ay  is  positive  and  /38  is  negative,  p  =  a8-j3y, 
and  r  be  the  absolute  value  of  p,  prove  that 


ayr 


/38r 


e  - 


where  e  f  w  ;  r      J  denotes  the  theta  function  in  which  the  exponent  of  the  general  term  is 
2  iriu  (n  +  e')  +  iirr  (n  +  1  ')2  +  2irie  (n  +  e'), 

and  |t,  «*  are  row  letters  of  p  elements,  all  positive  (or  zero)  and  less  than  r,  subject  to  the 
condition  that  (8/x  -  /3i>)/p,  (av  —  y/i)/p  are  integral,  while  e,  /,  g,  h  are  row  letters  of  p 
elements  which  are  all  positive  (or  zero)  and  less  than  r. 

Ex.  iii.  Taking,  in  Ex.  ii.,  a,  @,  y,  8  respectively  equal  to  1,  1,  1,  -k,  we  find 
p  =  v<k+  1,  k  being  positive.  Hence,  taking  &  =  3,  prove  the  formula  (Konigsberger, 
Crelle,  LXIV.  (1865),  p.  24),  of  which  each  side  contains  2P  terms, 


26 


(u;  r\\S> 

V      It 


QU;  3r  I  f  $'- 

if 


's  9  /O;  r   °.}  Q  (lu;  3r  !  ?  V 

\     liv    V        If*/ 


s,  «'  being  rows  of  p  quantities  each  either  0  or  1. 

293.  We  proceed  now  to  obtain  a  formula*  for  the  product  of  any 
number,  k,  of  theta  functions. 

We  shall  be  concerned  with  two  matrices  X,  x,  each  of  p  rows  and  k 
columns  ;  the  original  matrix,  written  with  capital  letters,  is  to  be  trans 
formed  into  the  new  matrix  by  a  substitution  different  for  each  of  the 
p  rows  ;  for  the  j-th  row  this  substitution  is  of  the  form 

(Xij,  X2j,  ...,  Xrj,  ...,  Xktj)=-  a>j(xliit  asaj,  ...,  xrj,  ...,  ocktj); 

rj 

herein  TJ  is  a  positive  integer;  to,-  is  a  matrix  of  k  rows  and  columns, 
consisting  of  integers  ;  the  determinant  formed  by  the  elements  of  this 
matrix  is  supposed  other  than  zero,  and  denoted  by  /^;  bearing  in  rnind 
that  throughout  this  Article  the  values  of  r  are  1,  2,  ...,  k  and  the  values  of^' 
are  1,  2,  .  .  .  ,  p,  we  may  write  the  substitution  in  the  form 


The  substitution  formed  with  the  first  minors  of  the  determinant  of  etj  will 
be  denoted  by  ft,-;  that  formed  from  flj  by  a  transposition  of  its  rows  and 

columns  will  be  denoted  by  IL.     Then  the  substitution  inverse  to  -  «,  is 

ri 

£fy'}  denoting  the  former  substitution  by  X,-,  the  latter  is  X/-1. 

Prym  und  Krazer,  Neue  Grundlagen...der  allgemeinen  thetafunctionen,  Leipzig,  1892. 


478  INVESTIGATION   OF   A  GENERAL   FORMULA  [293 

If  for  any  value  of  j  a  set  of  k  integers,  Prj,  be  known  such  that  the  k 
quantities 


are  integers,  then  it  is  clear  that  an  infinite  number  of  such  sets  can  be 
derived;  we  have  only  to  increase  the  integers  Prj  by  integral  multiples  of 
jj,j.  But  the  number  of  such  sets  in  which  each  of  Prj  is  positive  (including 
zero)  and  less  than  the  absolute  value  of  ft  is  clearly  finite,  since  each 
element  has  only  a  finite  number  of  possible  values.  We  shall  denote  this 
number  by  Sj  and  call  it  the  number  of  normal  solutions  of  the  conditions 

A*.         _ 

—  flj  (Pr,j)  =  integral  ; 
ft 

it  is  the  same  as  the  number  of  sets  of  k  integers,  positive  (or  zero)  and  less 
than  the  absolute  value  of  ft,  which  can  be  represented  in  the  form  ^j(pr,j), 
for  integral  values  of  the  elements  prj. 

The  k  theta  functions  to  be  multiplied  together  are  at  first  taken  to  be 
those  given  by 

®r  =  2e2  W+^W  (r  =  1  ,...,&), 


wherein  Br  is  such  a  symmetrical  matrix  that,  for  real  values  of  the  p 
quantities  X,  the  real  part  of  the  quadratic  form  denoted  (§  174,  Chap.  X.)  by 
BrX2  is  negative.  The  p  elements  of  the  row-letters  Vr,  Nr  are  denoted  by 
Vrj,  Nr>j(j  =  1,  ...,p).  The  substitutions  Xj  are  supposed  to  be  such  that 

k 

the   equations   (Xr>  j)  =  *hy(ar,j)   transform   the   sum    2  BrXr2  into   a    sum 


r=l 

t 


S  brXr*>  in  which  the  matrices  br  are  symmetrical  and  have  the  property  that 

r=l 

for  real  xr  the  real  part  of  byX?  is  negative. 

Taking  now  quantities  mrj,  vrj  determined  by 

(mr,  j)  =  X,--1  (Nr>  j)  =  p  n,-  (Nr>  j),     (vr,  j)  =  \j  (  Vr>  j)  =  -  &j  (  Vr,  j), 
/*;  rj 

k  k  k 

the  expressions    X  BrNrz,    S  NrVr  are  respectively  transformed  to    2  brmt? 

r=l  r=l  r=l 

and 

p  P  — 

2,  \j  (mr>  j)  (  Vr>  j)  =  S  Xj  (  Vr>  j)  (mr,  j)  =  2  vrmr  ; 

j=l  j=l  r=l 

hence  the  product   II  ®r  is  transformed  into        1      e%"rWr  ,  rmr  t  where  the 

r=l  N,  .....  Nk 

quantities  mrj  have  every  set  of  values  such  that  the  quantities  \j(mrj)  take 
all  the  integral  values,  Nrj,  of  the  original  product. 


293]  FOR   THE    PRODUCT   OF   THETA    FUNCTIONS.  479 

As  in  the  two  cases  previously  considered  in  this  chapter,  we  seek  now  to 
associate  integers  with  the  quantities  mrj.  Let  (Pr,j)  be  any  normal  solution 
of  the  conditions 

^  tij  (Prj)  =  integral,  =  (pr<  j),  say ; 
Pt 

put,  for  every  value  of  j, 

(Nrj)-(Prj)  =  Hj(Mrtj)  +  (E'rJ\  (r  =  l,  ...,  k) 

wherein  (Mrj}  consists  of  integers,  and  (E'r,j)  consists  of  positive  integers 
(including  zero),  of  which  each  is  less  than  the  absolute  value  of  /j,j.  For  an 
assigned  set  (Pr>  j)  this  is  possible  in  one  way ;  then 

(mr,  j)  =  2  Qj(Nrti)  =  (pflj)  +  rjQj  (MrJ)  +  ^  ^(E'r>j} 
Pi  Pi 

=  (nr,j)+  -;(e'r,j),  say, 
where 

(«r,j)  =  (Pr.j)  +  rjflj  (MrJ),       (e'r>j)  =  Tj&j  (E'rj)  ' 

by  this  means  there  is  associated  with  (Nrj),  corresponding  to  an  assigned 
set  (Pr,j),  a  definite  set  of  integers  (nrj),  and  a  definite  set  (E'rj).  We  do 
not  thus  obtain  every  possible  set  of  integers  for  (nrj),  for  we  have 

~  «/  K,  j)  =  £  «j  (Pr,  j)  +  ft  (Mr,  j)  =  (Pr,  j)  +  HJ  (Mr>  j), 
Tj  Tj 

so  that  the  values  of  nr>  j  which  arise  are  such  that  Xj  (wr>  j)  are  integers. 

Conversely  let  (nr.  j)  be  any  assigned  integers  such  that  \j(nrj)  are 
integers  ;  put 

\j(nr>j)  =  (PrJ)  +  ftj(Mr!J), 

wherein  the  quantities  Mrj  are  integers,  and  the  quantities  Prj  are  positive 
integers  (or  zero),  which  are  all  less  than  the  absolute  value  of  /^-;  this  is 
possible  in  one  way ;  then  taking  any  set  of  assigned  integers  (E'r,  j),  which 
are  all  positive  (or  zero)  and  less  than  the  absolute  value  of  fij,  we  can  define 
a  set  of  integers  Nr<  j  by  the  equations,  wherein  \f~l  (Pr>  j)  =  integral, 

(Nrtj)  =  (E'rJ)  +  (PrJ)  +  pj  (MrJ)  -  (E'r>j)  +  X,.  (nrj). 

Thus,  from  any  set  of  integers  (Nrj),  arising  with  a  term  e*(Z  rNr+SrNr*)  of 

I 
the  product    II  ®r,  we  can,  by  association  with  a  definite  normal  solution 

r=l 

(Pr,j)  of  the  conditions  \f*  (Prj)  =  integral,  obtain  a  definite  set  (E'rij),  and 
a  definite  set  (nr,j)  such  that  \j(nrj)  are  integers.  And  conversely,  from  any 
set  of  integers  (wr,j)  which  are  such  that  \j(nfij)  are  integral,  we  can,  by 
association  with  a  definite  set  (E'r>j),  obtain  a  definite  normal  solution  (Pr,j) 
and  a  definite  set  (Nrj). 


480  INVESTIGATION   OF   A   GENERAL   FORMULA  [293 

It  follows  therefore  that  if  the  product  H  ®r  be  written  down  ^ . . .  sp  times, 


r=l 


a  term  er  being  associated  in  turn  with  every  one  of  the  Si  ...sp 

normal  solutions  of  the  p  conditions  X/"1  (Pj)  =  integral,  then  there  will  arise, 
once  with  every  assigned  set  (E'Tj  j),  every  possible  set  (nr>  j)  for  which  Xj  (nr<  j) 
are  integers. 

We  introduce  now  a  factor  which  has  the  value  1  or  0  according  as  the 
integers  (nTi  j)  satisfy  the  conditions  X,-  (nri  j)  =  integral,  or  not.  Take  k  in 
tegers  (Erj),  which  are  positive  (or  zero),  and  less  than  r,-;  put 

then 

.  j_  !?jj  ]  =  22  —  e,  ,-  mr  4  =  2X9-  (Er  ,•)  (mr  ,-)  =  2X,-  (mr  ,•)  (Er  ,-) 
>j  I  „-_  ' i j     'ij       .   j  \    >tj/  \    M^/       .   j  \     <j'  »     'j' 


j 

and  this  is  integral  when  Nr  is  integral,  that  is,  for  all  the  values  (nrj)  which 
actually  occur  ;  in  fact  the  quantities  Nr>  j  denned  by 

1  /  '        \  ~\ 

(Nr>j)  =  \j(mrt})  =  -  ^(%^-t-^)  =  -  «!/  («r,  j)  +  (E'rj)  =  ^  Kj)  +  (E'rJ) 
rj     \  n  '      'i 

are  integral  or  not  according  as  Xj  (nfj  j)  are  integers  or  not. 
Hence,  for  a  given  set  nrjy  and  a  given  set  E'rj,  the  sum 


wherein  the  summation  extends  to  all  positive  (and  zero)  integer  values  of 
(Erj)  less  than  TJ,  is  equal  to  r^  ...  r^j  when  (Nrj)  are  all  integral,  and  other 
wise  contains  a  factor  of  the  form 


which  is  zero  because  TJ  (Nr,j)  is  certainly  integral.     Hence  if  we  denote 

22  -  erj  (nri  j  +  e^}  by  S  I  er  f  n,  +  ^)  , 
j  r  r,-     3  V  /A?  /          r  ^      V          /*  / 

J^  having  the  values  r^  ...,  rp,  then  we  can  write 

1  v    ZTriZ^er  (nr+-\         n  n 

,  -  ^2e    r«    \      ft/  =  l,  or  0, 
(n  .  .  .  r^f  .E 

according  as  X^  (?ir>  j)  are  all  integers  or  not. 

If  then  every  term  of  the  transformed  series,  in  which,  so  far,  only  those 
values  of  nrj  arise  for  which  \j(nrj)  are  integers,  be  multiplied  by  this  factor, 


293]  FOR  THE    PRODUCT   OF   THETA   FUNCTIONS.  481 

and  the  transformed  series  be  completed  by  the  introduction  of  terms  of  the 
same  general  form  as  those  which  naturally  arise  in  this  way,  so  that  now  all 
possible  integer  values  of  (nr>j)  are  taken  in,  the  value  of  the  transformed 
series  will  be  unaltered.  In  other  words  we  have 


n,E,E  r 

wherein  all  possible  integer  values  of  (nrj)  arise  on  the  right  ;  thus  the  right- 
hand  side  is  equal  to 


E\  E  r 

and  this  is  the  desired  form  of  the  transformed  product.  For  con 
venience  we  recapitulate  the  notations;  Er',  Er  each  denote  a  column  of 
p  integers,  positive  or  zero,  such  that  E'r>j  <  ^  ,  ErJ  <  r,-  ;  (Yr,j)  =  rjfy  (E'ft})\ 
(er>j)  =  ajj(E,.j);  Sj  is  the  number  of  sets  of  integral  solutions,  positive  or 
zero,  each  less  than  ^  ,  of  the  conditions  ij.j~lrj£Lj(Prt  ,-)  =  integi-al  ; 
(vr,  j)  =  rj~l  6>j  (Vr>  j)  ;  the  function  ®,.  is  a  theta  function  in  which  the  ordinary 
matrices  a,  b,  h  (§  189)  are  respectively  0,  6,.,  1  ;  by  linear  transformation  of 
the  variables  of  the  form  Vr  =  hrWr,  and,  in  case  the  matrices  coj  be  suitable, 

•S.ArV^ 

multiplication  by  an  exponential  er  ,  these  particularities  in  the  form  of 
the  theta  functions  may  be  removed. 

The  number  of  sets  (Erj)  is  (^...rp)*;  the  number  of  sets  (E'rtj)  is 
l/Ltj*  ...  npk  ;  the  product  of  these  numbers  is  the  number  of  theta-products  on 
the  right-hand  side  of  the  equation. 

Ex.  i.     We  test  this  formula  by  applying  it  to  the  case  already  discussed  where  «,•  is 
an  orthogonal  substitution  given  by 


which  is  independent  ofj,  r,-=2,  6r  = 


=  4;  then  ^=  -  16,  -Er,j<2,  E'rJ<lG,  and 


thence  -j\(i,j-  ^f2,y=-^2,>~-^u  =  integral,  etc.,  so  that  the  fractional  part  of  j,tr,j  is  in 

dependent  of  r  :  similarly  the  fractional  part  of  -  (e'r>>)  is  independent  of  r  and  we  may 

write     (f'r.j)  =  (kf'j  +  I'i.j,  \t'j  +  L2<i,  ...,  ^t'j  +  L^)  wherein  2ZriJ-  +  e'y<16.     By  the  formula 

B.  31 


482  EXAMPLES   OF  THE   APPLICATION  [293 

=  eMq>ff  S(v,  q},  when  N  is  integral,  we  know  that  9,.  ( v,. ;    *][£]  is  independent 

\         fr/-*V 

of  the  integral  part  of  f'r/p.  Hence  the  (16)4»  =  216')  terms  on  the  right-hand  side  of  the 
general  formula,  which,  for  a  specified  value  of  £»  (Er>i\  correspond  to  all  the  values  of 
\a>(E'r,j\  reduce  to  2P  terms,  in  which,  since  (E'r,j)  =  i<» (a f'i  +  ^i,i >  •••>  ^6'j  +  A,j)>  *U 
values  of  e'(<2)  arise.  Hence  there  is  a  factor  216p  and  instead  of  the  summation  in 
regard  to  E,  E'  we  have  a  summation  in  regard  to  E,  e',  the  right  hand  being  in  fact 

(7.2«p  2  neftv,  f6' 

A',  e'  »•       \         |«  (,A 

and  containing  24j>  terms. 

Now  put  $(Ei,j+E2,i  +  E3,s  +  E4,J 

Mj  being  integral ;  then  the  factor  of  a  general  term  of  the  expanded  right-hand  product 
which  contains  the  quantities  %a>  (Eftj)  is 

ne2iriifcr  (»,.+*£') 
}• 
where 

kr,J  =  E1,j  +  E,,j  +  E3,j  +  Et,j-2Er,j  =  ( 

and 

farie"SJcr  — 11$™)'  (tej+SMj—Zej-lMj)  _  jj 
*  i  3  ' 

while 

22Trik,.tjnrtj  =  iri22fjnrj  (mod.  2),  =iric .  2»r, 

j  r  j  r  r 

so  that 

ne27riP,.(n,.+K)  _rne27r^€(nr+Je')-j  g-««'. 
,.  ,. 

therefore  the  right-hand  product  consists  only  of  terms  of  the  form    116  (v,.,  f  J    e~"M£. 

Hence  the  24^  terms  arising,  for  a  specified  value  of  e',  for  all  the  values  of  Erti)  reduce  to 
2p  terms,  and  there  is  a  further  factor  23j) — the  right  hand  being 


where 

C7-(ii...^)-1(rI...rf)-*-(ik-i)"1»"¥-»"*1"IPli 

To  determine  the  value  of  C  we  must  know  the  number  (s)  of  positive  integral 
solutions,  each  less  than  16,  of  the  conditions  £o>  (#)  =  integral,  =(y)  say,  namely  of  the 
conditions,  x1  +  x2  +  x^+xi  =  2(xr  +  i/r}.  Now  of  these  any  positive  values  of  x^  x^  xz,  x± 
(<16)  are  admissible  for  which  ^  +  ^2  +  ^3+^4  is  even.  They  must  therefore  either  be 
all  even,  possible  in  84  ways,  or  two  even,  possible  in  6  .  82  .  82  ways,  or  all  odd,  possible  in 

84  ways.     Hence  s  =  8  .  8^  =  2^.     Hence  <7=1/215"24P  =  1/219P  and  therefore  C.  ^8p  =  ^- 
Making  now  in  the  formula  thus  obtained,  which  is 


the    substitution     Vr  =  kUr,    we    have    vr  =  $(Vl  +  Vs+V3+  F4  -  2  T"r)  =  hur,    where 
Ur=%(U1+U2+U3+Ui-2Ur);  and  if  we  multiply  the  left  hand  },;} 
which  is  equal  to  e^+^+^+^\  we  obtain 


293]  OF    THE   GENERAL    FORMULA.  483 

Therefore  if  Qly  Q2,  Q3,  Q^  denote  any  characteristics,  and,  as  formerly,  QQ  denote  the 
period-part  corresponding  to  Qr,  we  have 


n3(Ur,  Qr)  =  ne-^ur>  ^»(Ur+QQ    o)=n<rA<^'  «-)  n*(Ur+aQ  ,  o), 


of  which  the  first  factor  is  easily  shewn  to  be  mT^'  *•>,  if  fa,  ?2,  ?3,  ?4)  =  ^w(<21,  &,  Q3,  Qt)  • 
thus 

,  Qr)=      e-™'ne-^<r>  *) 


which  is  exactly  the  formula  previously  obtained  (§  292). 

Ex.  ii.     More  generally  let  A  =  -<o,-   be   any  matrix  such   that  the   linear  equations 


wherein  m  is  independent  of  ^,  ...,  xk  ;  then,  since,  by  a  property  of  all  linear  substitutions, 
the  equations  (Yr)  =  \  (yr)  lead  to 

r    a  ^v    8  3  9 

Jla^  +  ......  +  F^ryi8^+  ......  +^9V 

we  have  also* 


Hence,  if  A  be  any  matrix  of  p  rows  and  columns  and 

(Xrti')  =  \(xrti\  O'=l,  ...,P), 


we  have 


^2^,.  Fr>  <  =  j»  2  ^i,^. 

r  i,jr 


where  Ar1}  a,\,  etc.  now  denote  rows  of  p  quantities. 

tution  furnishes  a 

,-  =  «,  n=  +r*,  ^r>y  <  r,  A"P>> 


Thus  any  orthogonal  substitution  furnishes  a  case  of  our  theorem.     Taking  a  case 
where 


we  have 


so  that  the  new  characteristics  will  be  r-th  parts  of  integers. 
Suppose  now,  in  particular,  that  the  substitution  is 


* 

2        2-/t...          2 


2 


*  Therefore  mxy  =  XY=\x  .  \y  =  \\xy,  so  that  \\=m ;  hence  the  determinant  formed  with  the 
elements  of  X  has  one  of  the  values  ^/m*. 

31—2 


484  EXAMPLES   OF   THE   APPLICATION  [293 

which  gives 


=  2  R  ;  Oi  +  .  .  .  +  #fc)  -  xr     =  k  ^ 


.  .  .  .  .  .  .  .  .  +  xk)'2  +  2A>2  -  ^  2^,.  (^  +  .  .  .  +  xk)  =  2  J?r8 

and 


A\  +  ......  +Xk  =  A\  +  ......  +  A'fc,     Ar1-Z2  =  ^2-^1,  etc. 

The  previous  example  is  a  particular  case,  namely  when  £  =  4.  In  what  follows  we 
may  suppose  k  odd  so  that  r,-  =  &.  When  £  is  even  r,  may  be  taken  =  £&.  The  work  is 
arranged  to  apply  to  either  case. 

The  fractional  parts  of  -  («',.,  y)  being  independent  of  the  suffix  r  —  because 
e\,j--<'-2,J  =  -E'>t,J-E'i,i>  etc-> 


—we  may  put  -(?',-,  j)  =  (-,«/+  A,  >>  •••>  -  fj'  +  ^k,j]  >  aild  may  therefore  write 
ne  f  *v  'r!£\  in  the  form  ne  (v,.,  '  JV)  . 

r       \        frltij  r       \        frl^-J 

The  equation 


shews  that  all  values  of  -  e/  (<  1)  do  arise.     Hence  for  a  given  value  of  (Efti)  there  are, 

instead  of   1^1^  =  ?-^'  terms  given  by  the  general  formula,  only  r'\  and  the  factor  H*'2"1^ 
divides  out. 

The  values  of  —(*,-,,•)  given  by  the  general  formula  are  in  number  r  **>,  corresponding 

to  all  the  values  of  (Er>j).   As  before  the  fractional  part  of  -    («,.,  ,-)  is  independent  of  r.   Let 


where  T<!  ;  then 

K 


,.,  . 

The  factor  in  the  general  term  of  the  expanded  product  on  the  right  hand  which 
contains  cr>j  is 


Now 

1 

2ri  /   77f        \  
—  €,.  ,-  =  2  (Jiir  j)  =< 

r  1'  r 

therefore,  as  r  is  k  or  a  factor  of  k, 

Zm  —  e     •  — e'        Znite  +  IcM •)  ei         Ztri'j^i- 

Ile     r'rj=e       }       }   r  —e       f 

r 

and 


=  2  ft  +  2  J/,-  -  /?r ,  f]  nr , ,-  =  -k  ^fjnr , ,.  (mod.  1 ). 


293] 


OF   THE   GENERAL   FORMULA. 


485 


Hence  the  factor  above  is 

r  2e  /          e\~\  te'  «' 

T-         ^  2lrl'T  ("   +  -)        -Jrt—       2ni  — 
K=\l\.e       k   \    r    r/  \e          >•     e       r  , 
Lr 

and  the  general  term  of  the  right  hand  is 

[••(*•  £)>•"*• 

1  /2f,  \ 

06  7?(fr>*'     I  ir+^J^  —  ETti  ]  we  may  suppose  all  values  of  tj<*  to  arise.     Hence 
\  K  j 

instead  of  I*P  we  have  k*>  and  a  factor  i*i>\ki>  divides  out. 


To  evaluate  the  factor  (^  ...  rp}-1  (sl  ...s]t)-k,  =C,  say,  we  must  enquire  how  many 
positive  solutions  exist  of  the  conditions 

-#,.  =  integral, 


£  (#1  +  ...... 

namely,  how  many  solutions  of  the  conditions 

2 


T  (-^i  4- +%k)  =  integral, 

exist,  for  which  each  of  .rt,  ...,  xk<rk ;  let  s  be  this  number  ;  then  C=s-Pr~kJ),  and 

ne(Vr,0)  =  ^~^-      5 


where  «'<r,  e  <  ^r,  the  number  of  terms  on  the  right  being  (rky.     For  values  of  f>  -  we 
may  utilise  the  equation  3(v,  q  +  N)  =  e~niNq'  3  (v,  q).     For  example,  when  *  =  r  =  3  there 

are  3*  terms,  corresponding  to  characteristics  (*/?  )  .     When  k  =  4,  r=2,  the  character- 

2e       e 
istics  -£  =  -  will,  effectively,  repeat  themselves.     We  can  reduce  the  number  of  terms  from 


8»  or  23P  to  W.     We  shall  thus  get  factors 
that  already  found. 


=  l  and  so  the  formula  reduces  to 


Ex.  \\i.     Apply  the  formula  of  the  last  example  to  the  orthogonal  case  given  by  «,  =  w, 

(A',   Y,  Z,  T,  U,   K)  =  £«(#,  y,  z,  t,  u,  v), 
<•>  =  (        1       1      0      0      1  -1  ),     «-i  =  < 
1       1       00-1       1 
0      0 
0      0 


1-1       1       1 
-1111 
001-111 
00-1       1       1       1 
which  lead  to     =  64  and 


1  1  1-1  0  0  ), 
1  1-1  1  00 
001  1  1-1 
0011-11 
1-1  00  1  1 
-110011 


A'  +  r  +Z  +T  +  U  +  V  =.v  +y  +z  +t  +u 
Z-T=x-y,     U-V=z-t,     X-Y=u-v, 


[294 


CHAPTER   XVII. 

THETA  RELATIONS  ASSOCIATED  WITH  CERTAIN  GROUPS  OF  CHARACTERISTICS. 

294.  FOR  the  theta  relations  now  to  be  considered*,  the  theory  of  the 
groups  of  characteristics  upon  which  they  are  founded,  is  a  necessary 
preliminary.  This  theory  is  therefore  developed  at  some  length.  When  the 
contrary  is  not  expressly  stated  the  characteristics  considered  in  this 
chapter  are  half-integer  characteristics  f  ;  a  characteristic 


i 

Wi,  q-2,  -..,  qp 

is  denoted  by  a  single  capital  letter,  say  Q.  The  characteristic  of  which  all 
the  elements  are  zero  is  denoted  simply  by  0.  If  R  denote  another  charac 
teristic  of  half-integers,  the  symbol  Q  +  R  denotes  the  characteristic,  8  =  |s, 

*  The  present  chapter  follows  the  papers  of  Frobenius,  Crelle,  LXXXIX.  (1880),  p.  185,  Crelle, 
xcvi.  (1884),  p.  81.  The  case  of  characteristics  consisting  of  rt-th  parts  of  integers  is  considered 
by  Braunmiihl,  Math.  Annal.  xxxvn.  (1890),  p.  61  (and  Math.  Annal.  xxxn.  (1888),  where  the 
case  ?i  =  3  is  under  consideration). 

To  the  literature  dealing  with  theta  relations  the  following  references  may  be  given  :  Prym, 
Untersuchungen  iiber  die  Riemanri'sche  Thetaformel  (Leipzig,  1882)  ;  Prym  u.  Krazer,  Acta  Math. 
in.  (1883)  ;  Krazer,  Math.  Annal.  xxn.  (1883)  ;  Prym  u.  Krazer,  Neue  Grundlagen  einer  Theorie 
der  allgemeinen  Thetafunctionen  (Leipzig,  1892),  where  the  method,  explained  in  the  previous 
chapter,  of  multiplying  together  the  theta  series,  is  fundamental  :  Noether,  Math.  Annal.  xiv. 
(1879),  xvi.  (1880),  where  groups  of  half-integer  characteristics  are  considered,  the  former  paper 
dealing  with  the  case  p  =  i,  the  latter  with  any  value  of  p;  Caspary,  Crelle,  xciv.  (1883),  xcvi. 
(1884),  xcvii.  (1884)  ;  Stahl,  Crelle,  LXXXVIII.  (1879)  ;  Poincare",  Liouville,  1895;  beside  the  books 
of  Weber  and  Schottky,  for  the  case  p  =  3,  already  referred  to  (§§  247,  199),  and  the  book  of 
Krause  for  the  case  p  =  2,  referred  to  §  199,  to  which  a  bibliography  is  appended.  References  to 
the  literature  of  the  theory  of  the  transformation  of  theta  functions  are  given  in  chapter  XX. 
In  the  papers  of  Schottky,  in  Crelle,  en.  and  onwards,  and  the  papers  of  Frobenius,  in 
Crelle,  xcvn.  and  onwards,  and  in  Humbert  and  Wirtinger  (loc.  cit.  Ex.  iv.  p.  340),  will  be  found 
many  results  of  interest,  directed  to  much  larger  generalizations  ;  the  reader  may  consult  Weier- 
strass,  Berlin.  Monatsber.,  Dec.  1869,  and  Crelle,  LXXXIX.  (1880),  and  subsequent  chapters  of  the 
present  volume. 

t  References  are  given  throughout,  in  footnotes,  to  the  case  where  the  characteristics  are  n-th 
parts  of  integers.  In  these  footnotes  a  capital  letter,  Q,  denotes  a  characteristic  whose  elements 
are  of  the  form  q'Jn,  or  of  the  form  qjn,  qt'  ,  q^  being  integers,  which  in  the  '  reduced  '  case  are 
positive  (or  zero)  and  less  than  n.  The  abbreviations  of  the  text  are  then  immediately  extended 
to  this  case,  n  replacing  2. 


295]  DEFINITIONS   OF   SOME   SYMBOLS.  487 


whose  elements  si,  st  are  given  by  S{  =  q{  -I-  r/,  Si  =  qi  +  Ti.  The  charac 
teristic,  \t,  wherein  £/=  s/,  ti  =  S{  (mod.  2)  and  each  of  £/,  ...,tp  is  either 
0  or  1,  is  denoted  by  QR.  Unless  the  contrary  is  stated  it  is  intended  in 
any  characteristic,  $q,  that  each  of  the  elements  qj,  qi  is  either  0  or  1.  If 
^q,  ^r,  ^k  be  any  characteristics,  we  use  the  following  abbreviations 

p 
Q\=-.qq'  =  q1q1'+  ......  +qpqp',     i  Q,  R    =  qr'  -  q'r  =  2  (g<r<  -  ft'r<), 

t=i 

|Q,  R,K\  =  \R,  K  +  K,  Q   +   Q,  R  ,     (  ®]  =  e^r  =  e^'r>+  -  +M  • 

\-ft/ 

further  we  say  that  two  characteristics  are  congruent  when  their  elements 
differ  only  by  integers,  and  use  for  this  relation  the  sign  =.  In  this  sense 
the  sum  of  two  characteristics  is  congruent  to  their  difference.  And  we 
say  that  two  characteristics  Q,  R  are  syzygetic  or  azygetic  according  as 
|  Q,  .R  =  0  or  =  1  (mod.  2),  and  that  three  characteristics  P,  Q,  R  are 
syzygetic  or  azygetic  according  as  P,  Q,  R  =  0  or  =  1  (mod.  2). 

Ex.  Prove  that  the  2/>  +  l  characteristics  arising  in  §  202  associated  with  the  half 
periods  ua'  °\  ua'  a>,  ua'  c%  ...,  u°"  aP,  ua>  c  are  azygetic  in  pairs.  Further  that  if  any  four  of 
these  characteristics,  A,  B,  C,  D,  be  replaced  by  the  four,  BCD,  CAD,  ABD,  ABC,  the 
statement  remains  true;  and  deduce  that  every  two  of  the  characteristics  1,  2,  ...,  7  of 
§  205  are  azygetic. 

295.  A  preliminary  lemma  of  which  frequent  application  will  be  made 
may  be  given  at  once.  Let  a,,  ,,  ...,  a,,  „,  ...,  ar>  ,,  ...,  ar>n  be  integers,  such 
that  the  r  linear  forms 

Ui  =  aitlxl  +  ......  +  ais  nxn,  (i  =  1,  2,  .  .  .  ,  r), 

are  linearly  independent  (mod.  2)  for  indeterminate  values  of  xlt  ...,#„; 
then  if  Oi,  ...,  ar  be  arbitrary  integers,  the  r  congruences 

f/i  =  «!  ,  .  .  .  ,  Ur  =  ar  ,  (mod.  2), 

have  2n~r  sets  of  solutions*  in  which  each  of  xlt  ...,  xn  is  either  0  or  1.  For 
consider  the  sum 

2      [i  +  e^tf.-a.)]  ...  [1  +  e^Wr-  "'•>]. 

*    *i,  .-.,  xn 

wherein  the  2n  terms  are  obtained  by  ascribing  to  xl,  ...,  xn  every  one  of  the 
possible  sets  of  values  in  which  each  of  #,,  ...,  xn  is  either  0  or  1.  A  term  in 
which  xl}  ...,  xn  have  a  set  of  values  which  constitutes  a  solution  of  the 
proposed  congruences,  has  the  value  unity.  A  term  in  which  xly  ...,  xn  do 
not  constitute  such  a  solution  will  vanish  ;  for  one  at  least  of  its  factors  will 
vanish.  Hence  the  sum  of  this  series  gives  the  desired  number  of  sets  of 

*  When  the  forms  C/j  ,  .  .  .  ,  Ur  are  linearly  independent  mod.  m,  the  number  of  incongruent 

2irr 

sets  of  solutions  is  mn~r.  In  working  with  modulus  m  we  use  u  =  e  m  ,  instead  of  eiw  ;  and  instead 
of  a  factor  i  +  e™(u<-«^  we  U8e  a  factor  1  +  M  +  ^  +-  ...  +/j.n~\  where  n  =  t»Ul~n>. 


488  PROOF    OF   A   LEMMA.  [295 

solutions  of  the  congruences.     Now  the  general  term  of  the  series  is  typified 
by  such  a  term  as 


where  /*  may  be  0,  or  1,  or  .  .  .  ,  or  p  ;  and  this  is  equal  to 


where 

and,  therefore,  equal  to 


now,  when  //,  >  0,  one  at  least  of  the  quantities  clt  ...,cn  must  be  =  1  (mod.  2), 
since  otherwise  the  sum  of  the  forms  Ult  ...,  U^  is  =  0  (mod.  2),  contrary  to 
the  hypothesis  that  the  r  forms  Ult  ...,  Ur  are  independent  (mod.  2);  hence 
the  only  terms  of  the  summations  which  do  not  vanish  are  those  arising  for 
fj,  =  0,  and  the  sum  of  the  series  is 

Is  i 

Or  > 

*    x 

or  2n~r. 

Ex.  i.  If,  of  all  22P  half-integer  characteristics,  %q,  the  number  of  even  characteristics 
be  denoted  by  g,  and  h  be  the  number  of  odd  characteristics,  prove  by  the  method  here 
followed  that  g-h,  which  is  equal  to  Se™?9',  is  equal  to  2".  This  equation,  with  g  +  h  =  2*>, 
determine  the  known  numbers*  g  =  ^-\  (2*>  +  l),  h  =  <2P~l  (2"-  1). 

Ex.  ii.  If  \a  denote  any  half-integer  characteristic  other  than  zero,  and  %q  become  in 
turn  all  the  2*>  characteristics,  the  sum  Se7™'1  ^'  Ql  =  2e™  ^-a'^  vanishes.  For  it  is  equal  to 


and  if  \a  be  other  than  zero,  one  at  least  of  these  factors  vanishes.     On  the  other  hand  it 
is  obvious  that  2e™  '  °-  Q  '  =  22P. 

We  may  deduce  the  result  from  the  lemma  of  the  text.  For  by  what  is  there  proved 
there  are  22*-1  characteristics  for  which  \A,  Q\  =  0  (mod.  2)  and  an  equal  number  for 
which  |  A,  §|  =  1. 

296.     We  proceed  now  to  obtain  a  group  of  characteristics  which  are 
such  that  every  two  are  syzygetic. 

Let  P!  be  any  characteristic  other  than  zero  ;  it  can  be  taken  in  22^  —  1 
ways. 

Let  P2  be  any  characteristic  other  than  zero  and  other  than  Pj  ,  such  that 

P1}P2    =0(mod.  2); 

*  Among  the  n2?  incongruent  characteristics  which  are  7i-th  parts  of  integers,  there  are 
,,P-I  (wp  +  r?  -  1)  for  which  Q  \  =  0  (mod.  n),  and  n?-1  (n?  -  1)  for  which  |  Q  =  r  (mod.  n),  when  r 
is  not  divisible  by  n. 


296] 


GOPEL   GROUP    OF   CHARACTERISTICS. 


489 


by  the  previous  lemma  (§  295),  P2  can  be  taken  in  2'*"1  —  2  ways  ;  also  by 
the  definition,  if  P1P.1  be  the  reduced  sum*  of  P,,  P2, 

P^PJP.H    P^P,    +    P,,  P,|  =  0(mod.  2). 

Let  P3  be  any  characteristic,  other  than  one  of  the  four  0,  PI,  P2,  PiP2, 
such  that  the  two  congruences  are  satisfied 

|  P3,  P!    =  0,  |  P,,  P2    =  0,  (mod.  2)  ; 

then  P3  can  be  chosen  in  22*~2  —  22  ways  ;  also,  by  the  definition, 
|  P3,  P,P,  |  =    P,,  P,    +    P,,  P2    =  0,  (mod.  2), 

|  P,,  P,P,  |  =  0,  etc. 
Let  P4  be  any  characteristic,  other  than  the  23  characteristics 

0,  Plf  P2,  P,,  P.P,,  P2P3,  P.P,,  P.P.P3, 
which  is  such  that 

|  P4,  A    =  0,     P4,  P2    =  0,     P4,  P3    =  0,  (mod.  2)  ; 


and 


then  P4  can  be  chosen  in  2^~3  -  2s  ways,  and  we  have 


and 


P2P3,  P4  =  P2,  P4  +  P3,  P4  !  =  0,  (mod.  2),  etc., 


P,P,P,,  P4  1  =  Plf  P4 


,  P4  =  0,  (mod.  2). 


P     P  I 
*ti  ft  \  • 

Proceeding  thus  we  shall  obtain  a  group  of  2r  characteristics, 

0     P,       Po  P    Po  PPP 

v>   •*•   1)    •*•    2 1    "••?    •*•    I*    2?    •  •  •  >    -*•    1  -*•    2-*    3j    •  •  *  > 

formed  by  the  sums  of  r  fundamental  characteristics,  and  such  that  every 
two  are  syzygetic.  The  r-th  of  the  fundamental  characteristics  can  be 
chosen  in  22?-r+1  -  2r~1  =  2r~l  (2*p-*-+*  -  1)  ways;  thus  we  may  suppose  r  as 
great  as  p,  but  not  greater.  Such  a  group  will  be  denoted  by  a  single 
letter,  (P) ;  the  r  fundamental  characteristics,  P1}  P2,  P3,  ...,  may  be  called 
the  basis  of  the  group.  We  have  shewn  that  they  can  be  chosen  in 

or 

/  ff>*>Jl  1    \    /£V>»1 — O  1    \     /  C*O*i 1  1    \  /flOl) ftf-L.it  t    \    Cl*  I'/'f       -i  \  f  I 

I     1  I       '"P       -'I*    __      I     \      J^'  \*  — *•)  j  \f* 


ways.  But  all  these  ways  will  not  give  a  different  group ;  any  r  linearly 
independent  characteristics  of  the  group  may  be  regarded  as  forming  a  basis 
of  the  group.  For  instance  instead  of  the  basis 


we  may  take,  as  basis, 


P     P  P 

j.  i,  J.  2,  •  •• ,  ±  r 

PPP  P 

*  I-1-  2>  -*•  2)   •••  t  *  r> 

wherein  PiP2  is  taken  instead  of  P, ;  then  Pl  will  arise  by  the  combination 
*  So  that  the  elements  of  PjPo  are  each  either  0  or  £. 


490  GOPEL    SYSTEMS  [296 

of  PjP2  and  P2.  Hence,  the  number  of  ways  in  which,  for  a  given  group,  a 
basis  of  r  characteristics,  P/,  ...,  P/,  may  be  selected  is 

(2*1  -  1)  (2r  -  2)  .  .  .  (2*-  -  2'-1)/|r, 

for  the  first  of  them,  P/,  may  be  chosen,  other  than  0,  in  2r  —  1  ways  ;  then 
P2',  other  than  0  and  P/,  in  2r  —  2  ways  ;  then  P/  may  be  chosen,  other  than 
0,  P/,  P/,  P/Pa',  in  2r  —  22  ways,  and  so  on,  and  the  order  in  which  they  are 
selected  is  immaterial. 

Hence  on  the  whole  the  number  of  different  groups,  of  the  form 
0   p     p  p  p  P  P  P 

Vj   -L   i)    J-    21    •••)    -L    I-1-   2>    •••>   *    I-4   I*    3>    ••• 

of  2r  characteristics,  in  which  every  two  characteristics  of  the  group  are 
syzygetic*,  is 

(2^  —  1)  (22^-2  —  1)  ......  (%ip-vr+2  —  1) 

~  ~ 


Such  a  group  may  be  called  a  Gopel  group  of  2r  characteristics.  The 
name  is  often  limited  to  the  case  when  r=p,  such  groups  having  been 
considered  by  Gopel  for  the  case  p  =  2  (cf.  §  221,  Ex.  i.). 

297.  We  now  form  a  set  of  2r  characteristics  by  adding  an  arbitrary 
characteristic  A  to  each  of  the  characteristics  of  the  group  (P)  just  obtained  ; 
let  P,  Q,  R  be  three  characteristics  of  the  group,  and  A',  A",  A'",  the  three 
corresponding  characteristics  of  the  resulting  set  ;  then 

\A',A",A'"  =  \AP,AQ,AR\  =  \P,Q,R  =   Q,  R  +   R,P  +  P,Q  ,  (mod.  2), 

as  is  immediately  verifiable  from  the  definition  of  the  symbols  ;  thus  the 
resulting  set  is  such  that  every  three  of  its  characteristics  are  syzygetic,  that 
is,  satisfy  the  condition 

|  A',  A",  A'"   =  0,  (mod.  2)  ; 

this  set  is  not  a  group,  in  the  sense  so  far  employed  ;  we  may  choose  r  +  1 
fundamental  characteristics  A,  Al}  ...,  Ar,  respectively  equal  to  A,  APl} 
J.P2,  ...,  APr>  and  these  will  be  said  to  constitute  the  basis  of  the  system; 
but  the  2r  characteristics  of  the  system  are  formed  from  them  by  taking  only 
combinations  which  involve  an  odd  number  of  the  characteristics  of  the  basis. 
The  characteristics  of  the  basis  are  not  necessarily  independent  ;  there  may, 
for  instance,  exist  the  relation  A  +  AP1  =  AP2,  or  A  ^P^.  But  there  can 
be  no  relation  connecting  an  even  number  of  the  characteristics  of  the  basis  ; 
for  such  a  relation  would  involve  a  relation  connecting  the  set,  Pl}  P2,  .  ..,  Pr, 
of  the  group  before  considered,  and  such  a  relation  was  expressly  excluded. 
Hence  it  follows  that  there  is  at  most  one  relation  connecting  an  odd  number 

*  When  the  characteristics  are  n-th  parts  of  integers,  the  number  of  such  syzygetic  groups  is 
(n2"-!)  ...  (n2P-2r+2-l)  divided  by  (nr-l)  ...  (n-  1). 


297]  OF   CHARACTERISTICS.  491 

of  the  characteristics  of  the  basis  ;  for  two  such  relations  added  together 
would  give  a  relation  connecting  an  even  number. 

Conversely  if  A,  Aly  ...,  Ar  be  any  r+l  characteristics,  whereof  no 
even  number  are  connected  by  a  relation,  such  that  every  three  of  them 
satisfy  the  relation 

A',  A",  A'"   =  0,  (mod.  2), 

we  can,  taking  Pa  =  AaLA,  obtain  r  independent  characteristics  P1(  ...,  Pr>  of 
which  every  two  are  syzygetic,  and  hence,  can  form  such  a  group  (P)  of  2r 
pairwise  syzygetic  characteristics  as  previously  discussed.  The  aggregate  of 
the  combinations  of  an  odd  number  of  the  characteristics  A,  Alt  ...,  Ar  may 
be  called  a  Gopel  system*  of  characteristics.  It  is  such  that  there  exists  no 
relation  connecting  an  even  number  of  the  characteristics  which  compose  the 
system,  and  every  three  of  the  2r  characteristics  of  the  system  satisfy  the 
conditions 

|  A',  A",  A'"   =  0,  (mod.  2). 

We  shall  denote  the  Gopel  system  by  (AP). 

To  pass  from  a  definite  group,  (P),  of  2r  pairwise  syzygetic  characteristics 
to  a  Gopel  system,  the  characteristic  A  may  be  taken  to  be  any  one  of  the 
2^  characteristics.  But  if  it  be  taken  to  be  any  one  of  the  characteristics  of 
the  group  (P),  we  shall  obtain,  for  the  Gopel  system,  only  the  group  (P)  ;  and 
more  generally,  if  P  denote  in  turn  every  one  of  the  characteristics  of  the 
group  (P),  and  A  be  any  assigned  characteristic,  each  of  the  2r  characteristics 
AP  leads,  from  the  group  (P),  to  the  same  Gopel  system.  Hence,  from  a 
given  group  (P)  we  obtain  only  2'*~r  Gopel  systems.  Hence  the  number  of 
Gopel  systems  is  equal  to 

(2*  -1)  (£*"  -1)...  (2*-*+'  -1) 


We  shall  say  that  two  characteristics,  whose  difference  is  a  characteristic  of 
the  group  (P).  are  congruent,  mod.  (P).  Thus  there  exist  only  2P>-r 
characteristics  which  are  incongruent  to  one  another,  mod.  (P). 

It  is  to  be  noticed  that  the  22^~r  Gopel  systems  derived  from  a  given 
group  (P)  have  no  characteristic  in  common;  for  if  P1}  P2  denote  character 
istics  of  the  group,  and  A1}  Az  denote  two  values  of  the  characteristic  A,  a 
congruence  A^  =  A2P2  would  give  A^A^P^^,  which  is  contrary  to  the 
hypothesis  that  Al  and  A2  are  incongruent,  mod.  (P).  Thus  the  Gopel 
systems  derivable  from  a  given  group  (P)  constitute  a  division  of  the  2=* 
possible  characteristics  into  2^~r  systems,  each  of  2r  characteristics.  We  can 
however  divide  the  2^  characteristics  into  2^-r  systems  based  upon  any 
group  (Q)  of  2r  characteristics  ;  it  is  not  necessary  that  the  characteristics  of 
the  group  (Q)  be  syzygetic  in  pairs. 

By  Frobenius,  the  name  Gopel  system  is  limited  to  the  case  when  r  =  p. 


492 


GOPEL   SYSTEMS    CONSISTING   WHOLLY 


[297 


Ex.  For  £>  =  2,  r  =  2,  the  number  of  groups  (P)  given  by  the  formula  is  15.  And  the 
number  of  Gopel  systems  derivable  from  each  is  4.  We  have  shewn  in  Example  iv., 
§  289,  Chap.  XV.,  how  to  form  the  15  groups,  and  shewn  how  to  form  the  systems 
belonging  to  each  one.  The  condition  that  two  characteristics  P,  Q  be  syzygetic  is  equiva 
lent  to  |  PQ  |  =  P  |  + 1  Q  |  (mod.  2),  or  in  words,  two  characteristics  are  syzygetio  when  their 
sum  is  even  or  odd  according  as  they  themselves  are  of  the  same  or  of  different  character. 
It  is  immediately  seen  that  the  15  groups  given  in  §  289,  Ex.  iv.,  satisfy  this  condition. 
The  four  systems  derivable  from  any  group  were  stated  to  consist  of  one  system  in  which 
all  the  characteristics  are  even  and  of  three  systems  in  which  two  are  even  and  two  odd. 
We  proceed  to  a  generalization  of  this  result. 

298.  Of  the  22*'~r  Gopel  systems  derivable  from  one  group  (P),  there  is  a 
certain  definite  number  of  systems  consisting  wholly  of  odd  characteristics, 
and  a  certain  number  consisting  wholly  of  even  characteristics*.  We  shall 
prove  in  fact  that  when  p>r  there  are  20""1  (2°"  +  1)  of  the  systems  which 
consist  wholly  of  even  characteristics,  o-  being  p  —  r ;  these  may  then  be 
described  as  even  systems ;  and  there  are  2<r~1  (2°"  —  1)  systems  which  may  be 
described  as  odd  systems,  consisting  wholly  of  odd  characteristics.  When  p  =  r, 
there  is  one  even  system,  and  no  odd  system.  In  every  one  of  the  22cr(2r  —  1) 
Gopel  systems  in  which  all  the  characteristics  are  not  of  the  same  character, 
there  are  as  many  odd  characteristics  as  even  characteristics. 

For,  if  Pj,  ...,  Pr  be  the  basis  of  the  group  (P),  a  characteristic  A  which 
is  such  that  the  characteristics  A,  APl}  ...,  APr  are  all  either  even  or  odd, 
must  satisfy  the  congruences 

\XP,\=    XP2   = =    X  ,  (mod.  2) 

which  are  equivalent  to 

Y  P-  =\  P-  a  —  i  9       T\ 

•<*->   -L    I      —  \  -L   I     >  \fc  ~    1>    6}    •••>'}} 

as  is  immediately  obvious.     Since,  when    X,  Pl  \  =  j  7^  ,  and    X,  P2 1  =   P 


X,  P, 


X,P.2\+ 

=  I  Pj  I  +    P2    +  I  PI,  P2  I  =  ! 


etc.,  it  follows  that  these  r  congruences  are  sufficient,  as  well  as  necessary. 
These  congruences  have  (§  295)  22^~r  solutions.  If  A  be  any  solution,  each 
of  the  2r  characteristics  forming  the  Gopel  system  (AP)  is  also  a  solution ; 
for  it  follows  immediately  from  the  definition,  if  P,  Q  denote  any  two 
characteristics  of  the  group,  that 

\APQ\  =  \A   +  P\+  Q  +  A,  p  +\A,Q  +  P,  Q 
=  \A\  +  2\P  +2JQ  +  P,Q\ 
=  \A  , 
because    P,  Q.\  =  0.     Hence  the  2'*~r  solutions  of  the  congruences  consist  of 


*  This  result  holds  for  characteristics  which  are  -;t-th  parts  of  integers,  provided  the  group  (P) 
consist  of  characteristics  in  which  either  the  upper  line,  or  the  lower  line,  of  elements,  are  zeros. 


299]  OF   ODD   OR   OF    EVEN    CHARACTERISTICS.  493 

2w-'-f2r  =  <2?p-'»-  characteristics  A,  and  the  characteristics  derivable  therefrom 
by  addition  of  the  characteristics,  other  than  0,  of  the  group  (P)  ;  namely 
they  consist  of  the  characteristics  constituting  22^~2r  Gopel  systems,  these 
systems  being  all  derived  from  the  group  (P).  In  a  notation  already 
introduced,  the  congruences  have  2^~2''  solutions  which  are  incongruent 
(mod.  (P)). 

Ex.  If  S  be  any  characteristic  which  is  syzygetic  with  every  characteristic  of  the 
group  (P),  without  necessarily  belonging  to  that  group,  prove  that  the  22P~2r  characteristics 
SA  are  incongruent  (mod.  P),  and  constitute  a  set  precisely  like  the  set  formed  by  the 
characteristics  A. 

299.  Put  now  a  =  p  —  r,  and  consider,  of  the  22<r  Gopel  systems  just 
derived,  each  consisting  wholly  either  of  odd  or  of  even  characteristics, 
how  many  there  are  which  consist  wholly  of  odd  characteristics  and  how 
many  which  consist  wholly  of  even  characteristics.  Let  h  be  the  number  of 
odd  systems,  and  g  the  number  of  even  systems.  Then  we  have,  beside  the 
equation 

g  +  h  =  22-, 
also 

g  —  k  =  2~-'"S,e'"'ilRl  [  I+^^^.-P.I-^I^I]  ...  [i  +  e*i\it,pr\—*i\prn 

wherein  Plt  ...,  Pr  are  the  basis  of  the  group  (P),  and  R  is  in  turn  every  one 
of  the  22^  possible  characteristics.  For,  noticing  that  the  congruence 
|  RP  =  .ft  |  is  the  same  as  |  R,  P  \  =  \  P  |,  it  is  evident  that  the  element  of 
the  summation  on  the  right-hand  side  has  a  zero  factor  when  R  is  a 
characteristic  for  which  all  of  R,  RPlt  ...,  RPr  are  not  of  the  same 
character,  either  even  or  odd,  and  that  it  is  equal  to  2~renilRl  when 
these  characteristics  are  all  of  the  same  character;  while,  corresponding 
to  any  value  of  R,  say  R  =  A,  for  which  all  of  R,  RP1}  ...,  .RPr  are  of 
the  same  character,  there  arise,  on  the  right  hand,  2r  values  of  R,  the 
elements  of  the  Gopel  set  (AP),  for  which  the  same  is  true. 

Now  if  we  multiply  out  the  right-hand  side  we  obtain 


wherein^   2     denotes   a   summation   extending   to    every  set  of  /j,  of  the 
/"i,  PI,  ... 

characteristics  P1(  ...,  PM,  and  /a  is  to  have  every  value  from  1   to  ?•;  but 
we  have,  since  P,,  P.2,  ...  ,  are  syzygetic  in  pairs, 


and  therefore 


where  S,  =  RP1  ...  P^,  will,  as  R  becomes  all   2^   characteristics   in    turn, 


494  DETERMINATION    OF    GOPEL    SYSTEMS  [299 

also  become  all  characteristics  in  turn;  also  ^eniljl]  =  ^ewils^  is  immediately 

R  s 

seen  to  be  2^  ;  it  is  in  fact  the  difference  between  the  whole  number  of  even 
and  odd  characteristics  contained  in  the  22p  characteristics.     Hence 


and  therefore  g-h  =  %>-r  =  2". 

This  equation,  with  g  +  h  =  22<r,  when  cr  >  0,  determines  g  =  Z*~l  (2°"  +  1) 
and  h  =  20""1  (2CT  —  1),  and  when  cr  =  0  determines  g  =  1,  h  =  0. 

These  results  will  be  compared  with  the  numbers  %>-1  (2^  +  1),  2p~l  (2p  -  1), 
of  the  even  and  odd  characteristics,  which  make  up  the  22p  possible  character 
istics. 

If  Pi  denote  every  characteristic  of  the  group  (P)  in  turn,  and  Pm  denote 
one  characteristic  of  the  bases  P},  ...,  Pr,  and  R  be  such  a  characteristic  that 
the  2r  characteristics  RPi  are  not  all  of  the  same  character,  at  least  one  of 
the  r  quantities  R,  Pm  \  +  \  Pm  |  is  =  1  (mod.  2),  and  therefore  the  product 

r 

IJ     H    +  0iri\Pm\+iri\R,Pm\\ 

m=l 

is  zero.     But,  in  virtue  of  the  congruences, 

I   p.p.  I  —  I    P.  I  _l_  I  P.  I        17?    P.  I  4.     7?     P.    =17?    P.P.  I 
I  ***J  I  =  I  •*  i  \   '    I  *}  I  '       I  •"'»  -*i  I    '      -**t  *i    =  I  •"')  ***  J  I  ' 

this  product  is  equal  to 

2r  2r 

^    girilPil  +ni\R,  Pi  I      Qr    g-Tril^l    ^    gTril/JPil  _ 


Now  e™  '  fip'  '  is  1  or  —  1  according  as  RPi  is  an  even  or  odd  characteristic. 
Hence  the  system  of  2r  characteristics  RPi  contains  as  many  odd  as  even 
characteristics,  and  therefore  2r~l  of  each,  unless  all  its  characteristics  be  of 
the  same  character. 

300.  The  22<r  Gb'pel  systems  thus  obtained,  each  of  which  consists  wholly 
of  characteristics  having  the  same  character,  either  even  or  odd,  have  a 
further  analogy  with  the  22p  single  characteristics.  We  have  shewn  (§  202, 
Chap.  XL)  that  the  2^  characteristics  can  all  be  formed  as  sums  of  not  more 
than  p  of  2p  +  1  fundamental  characteristics,  whose  sum  is  the  zero  character 
istic;  we  proceed  to  shew  that  from  the  22cr  Gopel  systems  we  can  choose 
2cr  +  1  fundamental  systems  having  a  similar  property  for  these  22<r  systems. 

Let  the  s  =  22<r  Gopel  systems  be  represented  by 

(^P),  ...,(2L.P), 

the  first  of  them,  in  a  previous  notation,  consisting  of  Al  and  all  characteristics 
which  are  congruent  to  A±  for  the  modulus  (P),  and  similarly  with  the  others. 
Then  we  prove  that  it  is  possible,  from  A1}  ...,  As  to  choose  2<r  +  1  character- 


300] 


WHEREOF    EVERY    THREE    ARE   AZYGETIC. 


495 


istics,  which  we  may  denote  by  Alt  ...,  A2^+1,  such  that  every  three  of  them, 
say  A',  A",  A"',  satisfy  the  condition 

j  A',  A",  A'"  |  =  1,  (mod.  2) ; 
but  it  is  necessary  to  notice  that,  if  P  be  any  characteristic  of  the  group  (P), 

I  A'P,  A",  A'"  ,  =  \A',  A",  A'"  +  |  P,  A"   +   P,  A'" 


is  = 


A',A",A'"\;  for  |  P, 


P  ,  is  also  =  P,  A'"  ;  hence,  if  B',  B",  B'" 
be  any  three  characteristics  chosen  respectively  from  the  systems  (A'P), 
(A"P),  (A'"P),  the  condition  |  A',  A",  A'"  \  =  1  will  involve  also  Bf,  B",  B'"  =  I  ; 
hence  we  may  state  our  theorem  by  saying  that  it  is  possible,  from  the 
22<r  Gopel  systems,  to  choose  2<r  -f  1  systems,  whereof  every  three  are  azygetic. 

Before  proving  the  theorem  it  is  convenient  to  prove  a  lemma  ;  if  B  be 
any  characteristic  not  contained  in  the  group  (P),  in  other  words  not 
=  0  (mod.  (P)),  and  R  become  in  turn  all  the  22<r  characteristics  A1}  ...,  A8, 

then* 

•£e™  i  R,  B  i  _  o. 

R 

For  let  a  characteristic  be  chosen  to  satisfy  the  r  +  1  congruences 
X,  B   =1,    X,  P!   =  0,  ...,|Z,  Pr   =0,  (mod.  2), 

and,  corresponding  to  any  characteristic  R  which  is  one  of  Alt  ...,  As,  and 
therefore  satisfies  the  r  congruences  |  R,  P;  |  =  P  J  ,  take  a  characteristic 
S  =  RX;  then 

\8,B\-  R,B  =  \X,B  EEl.and   S,Pt\=  RX,Pi\  =  \R,Pi\  +  \X,Pi  =  P<|, 

because  |  X,  Pi  =  0  ;  hence  the  characteristics  Alt  ...,  As  can  be  divided  into 
pairs,  such  as  R  and  S,  which  satisfy  the  equation  eni  '  s>  B  '  =  —  evi  '  R>  B  '.  This 
provesf  that  ^e^R>  B{  =  0. 

R 

We  now  prove  the  theorem  enunciated.  Let  the  characteristic  Al  be 
chosen  arbitrarily  from  the  s  characteristics  Alt  ...,  As\  this  is  possible  in 
22<r  ways.  Let  A2  be  chosen,  also  from  among  A1}  ...,AS,  other  than  Al  ; 
this  is  possible  in  22<r  —  1  ways.  Then  A3  must  be  one  of  the  characteristics 
A-i,  ...,AS>  other  than  Alt  A2,  andj  must  satisfy  the  congruence  |  Al)Az,  X  \  =1. 
The  number  of  characteristics  satisfying  these  conditions  is  equal  to 


*  We  have  proved  an  analogous  particular  proposition,  that  if  B  be  not  the  zero  characteristic, 
and  R  be  in  turn  all  the  2-'*>  characteristics,  Se™  '  R'  B  '  =  0  (§  295,  Ex.  ii.). 

R 

t  If  R  be  all  the  2*P  characteristics  in  turn,  Se1"  '  0>  R  '  =  2^.     If  P  be  one  of  the  group  (P), 

and  tf  be  one  of  Alt  ...  ,  A,,  so  that  |  R,  P  \  =  \  P  |,  we  have  Se7"*'1  A  *  l  =  ewi  '  P  '  22". 

• 

t  We  do  not  exclude  the  possibility  ^as^^jj.      Since  l^,^,,,  ^^,,1  =  1  Al,  A.2  \,  it  is  a 
possibility  only  if  |^lt  A^\  =  l. 


496 


DETERMINATION    OF   GOPEL   SYSTEMS 


[300 


wherein  R  is  in  turn  equal  to  all  the  characteristics  Alt  ...,  As.     For  a  term 
of  this  series,  in  which  R  satisfies  the  conditions  for  A3,  is  equal  to  unity*, 
while   for   other  values  of  R  the  terms  vanish.     Now,  since    A1}  A2,  R 
R,  A1A2  \  +  |  A1}  A2  ,  the  series  is  equal  to 


the  characteristic  A1A2  cannot  be  one  of  the  group  (P),  for  if  A1A2  =  P,  then 
A2  =  A1P>  which  is  contrary  to  the  hypothesis  that  Alt  ...,  As  are  incon- 
gruent  for  the  modulus  (P);  hence  by  the  lemma  just  proved  the  sum  of  the 
series  is  2'2<r~1,  and  A3  can  be  chosen  in  220""1  ways. 

We  consider  next  in  how  many  ways  A4  can  be  chosen  ;  it  must  be  one  of 
A1}  ...,  As  other  than  Alt  A2,  A3  and  must  satisfy  the  congruences 

i  A1}  A2,  X  I  =  1,  |  Ait  A3,  X  =  1, 
which,  in  virtue  of  the  congruence    A1}  A2,  A3   =  1,  and  the  identity 


A2,  A3)  X 


,  Alt  X 


,  X 


ly  A2,  A3 


involve  also  j  A2,  As,  X   =  1.     The  number  of  characteristics  which  satisfy 
these  conditions  is  equal  to 


or 


2,  R\_      -2 


where  R  is  in  turn  equal  to  every  one  of  A1}  ...,  As;  hence,  in  virtue  of  the 
lemma  proved,  using  the  equations, 


A1} 


2,  R 


AltA2 


R, 


j,  A3  +   A2AS,  R 


the  number  of  solutions  obtained  is  22a~2.     But  we  have 


\A1A2A3,A1,A2 


A1A.2A3,A1A 


so  that  AiA^Az  also  satisfies  the  conditions. 

Now  it  is  to  be  noticed  that,  for  an  odd  number  of  characteristics 
Blt  ...,  -B^+1,  the  condition  that  every  three  be  azygetic  excludes  the 
possibility  of  the  existence  of  any  relation  connecting  an  even  number  of 
these  characteristics,  and  for  an  even  number  of  characteristics  B1}  ...,5^, 
the  condition  that  every  three  be  azygetic  excludes  the  possibility  of  the 
existence  of  any  relation  connecting  an  even  number  except  the  relation 
B1B2 . . .  B^  =  0.  For,  B  being  any  one  of  Blt  ...,  -5o*+i  other  than  Blt  ...,  B2m, 
we  have,  as  is  easy  to  verify, 


B1B2  .  .  . 


•\BltBtm,B\-^B9tBm,tB 

It  is  immediately  seen  that    A,  B,  B  \  =  0. 


,  B 


300] 


WHEREOF   EVERY   THREE   ARE   AZYGETIC. 


497 


so  that  the  left  hand  is  =  1  ;  therefore,  as  B2m,  B2m,  B  =  0,  we  cannot  have 
B2m  =  B1B2  ...  #>,„_!•  This  holds  for  all  values  of  m  not  greater  than  k,  and 
proves  the  statement. 

Hence,  2o-+  1  being  greater  than  4,  we  cannot  have  A4  =  A1A2A3,  for  we 
are  determining  an  odd  number,  2cr  +  l,  of  characteristics.  On  the  whole, 
then,  A  4  can  be  chosen  in  22<7~2  —  1  ways. 

To  find  the  number  of  ways  in  which  A5  can  be  chosen  we  consider  the 
congruences 


I,  A2,  .A.     =1,     AI,  A3,  JL     =  1, 


,  2L  \  =  1, 


which  include  such  congruences  as  A2,  A3,  X  \  =  1,  A2,  A±,  X\  =  1,  etc. 
The  characteristic  A5  must  be  one  of  Alt  ...,  As,  other  than  Al}  A2,  A3,  At\ 
the  condition  that  A5  be  not  the  sum  of  any  three  of  AI,  A2>  A3,  A4  is 
included  in  these  conditions.  The  number  of  ways  in  which  As  can  be 
chosen  is  therefore 


where  R  is  in  turn  equal  to  every  one  of  Alt  ...,  As;  making  use  of  the  fact 
that  A1A2A3A4  is  not  =  0,  we  find  the  number  of  ways  to  be  22<r~3. 

Proceeding  in  this  way,  we  find  that  a  characteristic  A2m+1  can  be  chosen 
in  a  number  of  ways  equal  to  the  sum  of  a  series  of  the  form 

2~  (zrn-i)  2  ("l  —  e1"!-4!'  ^2'  ^H  [1  —  e1™!-4!'  •4»«-Ri"|  ...  fl  —  e1"!-4!'  Azm>  R\~\ 

R 

and  therefore  in  22(7~<2m~1)  ways,  and  that  a  characteristic  A^  can  be  chosen 
in  22<r-<2m-2)  —  1  ways,  the  value  Azm  =  A1  A2  ...  A2m^  being  excluded.  In 
particular  A^  can  be  chosen  in  22  —  1  ways,  and  -42<r+i  in  2  ways. 

To  the  2<r+l  characteristics  thus  determined  it  is  convenient*  to  add 
the  characteristic  A2<r+2  =  A1A2  .  .  .  A2(r+1  ;  if  Ai}  Aj  be  any  two  of  Al}  ...,  A2ff+l 
we  have 

A2<r+2t  A{,  Aj   =  I  A{,  Aj,  AI  |  +  ......  +  |  A{,  Aj,  A2a-+i  \  =  1, 

the  expressions  Ai}  Aj,  At  \,  \  Ait  Aj,  Aj  \  being  both  zero.  We  have  then 
the  result  :  From  the  2'2<r  characteristics  Al}  ...,  As  it  is  possible  to  choose  a 
set  AI,  ...,  -42<H-2>  such  thut  every  three  of  them  satisfy  the  condition 

\A',A",A'"  =1, 
in 

1  (22ff~2  -  1)  ...  (22-  1)  2     2*r+ff8  (2ar-  1)  (22ff~2  -  1)  ...  (22-  1) 


ways ;  there  exists  no  relation  connecting  an  even  number  of  the  characteristics 
Al}  ...,  -A2<r+2  except  the  prescribed  condition  that  their  sum  is  zei*o ;  since  the 
sum  of  two  relations  each  connecting  an  odd  number  is  a  relation  connecting 

*  In  the  particular  case  of  §  202,  Chap.  XI.,  A2tT+2  is  zero. 
B.  32 


498  ROOT   SETS.  [300 

an  even  number,  there  can  be  at  most*  only  one  independent  relation  con 
necting  an  odd  number  of  the  characteristics  A!,  ...,  -42<7+2.  And,  as  before 
remarked,  to  every  one  of  the  characteristics  Al}  ...,  -42<r+2  is  associated  a 
Gopel  system  of  2r  characteristics. 

301.  The  22or  systems.  (A1P),  ...,  (ASP),  which  have  been  considered, 
were  obtained  by  limiting  our  attention  to  one  group  (P)  of  2r  pairvvise 
syzygetic  characteristics.  We  are  now  to  limit  our  attention  still  further  to 
the  sets  Alt  ...,  -A2<r+o  just  obtained  satisfying  the  condition  that  every  three 
are  azygetic. 

If  to  any  one  of  the  characteristics  Al}  ...,  A2<T+2,  say  A^,  we  add  the 
characteristic  X,  the  conditions  that  the  resulting  characteristic  may  still 
be  a  characteristic  of  the  set  Alt  ...,  As,  are  (§  298)  the  r  congruences 
XAk,  Pi  |  =  j  Pi  \,  in  which  i=  1,  ...,  r ;  in  virtue  of  the  conditions  |  A^,  Pi  \ 
=  |  Pi  ,  these  are  equivalent  to  the  r  congruences  \X,  Pi  \  =  0,  which  are 
independent  of  k;  these  latter  congruences  have  2^~r  solutions,  but  from 
any  solution  we  can  obtain  2r  others  by  adding  to  it  all  the  characteristics  of 
the  group  (P).  There  are  therefore  22p~2r  =  22<T  congruences  X,  incongruent 
with  respect  to  the  modulus  (P),  each  of  which -f,  added  to  the  set  Alf . . . ,  A2(r+z, 
will  give  rise  to  a  set  AS,  ...,  A'2(T+2,  also  belonging  to  Alt  ...,  As.  Further 
|  Ai,  A/,  Ajc'  \  =  XAi,  XAj,  XAk  \  =  Ai}  Aj,  Ak  =  1  ;  and  any  relation  con 
necting  an  even  number  of  the  characteristics  J./>  ...,  A'2lT+2  gives  a  relation 
connecting  the  corresponding  characteristics  of  Alf  ...,  A^+2.  Thus  the 
22<r  sets  derivable  from  A1}  ...,  A^+2  have  the  same  properties  as  the  set 
A  A 

XI  i,     ...  ,    ,TL2o.-|_2. 

Hence  all  the  sets  Alt  ...,  AZtT+2  can  be  derived  from 


root  sets  by  adding  any  one  of  the  22<r  characteristics  X  to  each  characteristic 
of  the  root  set. 

302.  Fixing  attention  upon  one  of  these  root  sets,  and  selecting 
arbitrarily  2<7  + 1  of  its  characteristics,  which  shall  be  those  denoted  by 
Aly  ...,  A2(r+i,  we  proceed  to  shew  that  of  the  22<r  characteristics  X,  there  is 
just  one  such  that  the  characteristics  XA1}  ...,  XA2<T+l,  derived  from 
Alf  ...,  A2tr+1,  have  all  the  same  character,  either  even  or  odd.  The 
conditions  for  this  are 

|  .A.n.1     =     XAf 


*  If  the  characteristic  of  which  all  the  elements,  except  the  z'-th  element  of  the  first  line,  are 
zero,  be  denoted  by  £/,  and  E^  denote  the  characteristic  in  which  all  the  elements  are  zero 
except  the  t-th  element  of  the  second  line,  every  possible  characteristic  is  clearly  a  linear  aggre 
gate  of  Ejf,  ... ,  Ep,  El,  ...,  Ep.  Thus  when  a  has  its  greatest  value,  =p,  there  is  certainly  one 
relation,  at  least,  connecting  any  2o-  + 1  characteristics. 

t  It  is  only  in  case  all  the  characteristics  of  the  group  (P)  are  even  that  the  values  of  A"  can 
be  the  characteristics  Al ,  ... ,  Ag. 


302]  FUNDAMENTAL   SETS   OF   THE   SAME   CHARACTER.  499 

which  are  equivalent  to  the  20-  congruences 

X.A.Ai  =   A^  +  lAil      (i=2,3,  ...,(2<r  +  l)); 

if  X  be  a  solution  of  these  congruences,  and  P  be  any  characteristic  of  the 
group  (P),  we  have 

XP,A,Ai\  =   X,AlAi\  +  \P,Al   +\P,At   =   A,   +   Ai\  +  2\P\, 

so  that  XP  is  also  a  solution;  since  the  other  congruences  satisfied  by  X 
were  in  number  r,  and  similarly,  associated  with  any  solution,  there  were  2r 
other  solutions  congruent  to  one  another  in  regard  to  the  group  (P),  it 
follows  that  the  total  number  of  .characteristics  X  satisfying  all  the 
conditions  is  %#-r-'**-r  =  l.  Thus,  as  stated,  from  any  2<7+  1  characteristics, 
AI,  ...,  -£0.7+1,  of  a  root  set,  we  can  derive  one  set  of  2<r  +  l  characteristics 
Aly  ...^A2<r+1,  which  are  all  of  the  same  character,  their  values  being  of  the 
form  Ai  =  XAi. 

Starting  from  the  same  root  set,  and  selecting,  in  place  of  Alt  ...,  Av+lt 
another  set  of  2<r+l  characteristics,  say  A^,  ...,  Av+z,  we  can  similarly 
derive  a  set  of  the  form 

X  A2,  ...,  X 4lsrffi 

consisting  of  2cr  + 1  characteristics  of  the  same  character.  The  question 
arises  whether  this  can  be  the  same  set  as  Alt  ...,  A.M+1.  The  answer  is  in 
the  negative.  For  if  the  set  X'Aa,  ...,  X'A2<r+2  be  in  some  order  the  same  as 
the  set  XAlt  ...,  XA2<r+l,  or  the  set  XX' A2,  ...,  XX'A2<r+2  the  same  as  the 
set  Alt ...,  A^+1,  it  follows  by  addition  that  XX' A^  =  A^+2  or  XX' =  A^A*^. 
Thence  the  set  A.A.A^,,  A.A-.A,^,  ...,  A^A^A^,  Al  is  the  same  as 
Alt  A.,,  ...,  A^+l,  or  we  have  2<7  equations  of  the  form  A^A^^^Aj,  in 
which  i  =  2,  ...,  2a+l,j  =  2,  ...,  2<r  +  l.  Since  there  is  no  relation  con 
necting  an  even  number  of  the  characteristics  Alt  ...,  A2<T+2  except  the  one 
expressing  that  their  sum  is  0,  these  equations  are  impossible*. 

Similarly  the  question  may  arise  whether  such  a  set  as  Alt  ...,  A»+l,  of 
2o-  +  l  characteristics  of  the  same  character,  azygetic  in  threes,  subject  to  no 
relation  connecting  an  even  number,  and  incongruent  for  modulus  (P),  can 
arise  from  two  different  root  sets.  The  answer  is  again  in  the  negative. 
For  if  A1}  ...,  A.&+1,  and  B1}  ...,  Bw+l  be  two  sets  taken  from  different  root 
sets,  the  2«r+l  conditions  XAi  =  X'Bi,  for  i  =  l,  ...,  2<r+l,  to  which  by 
addition  may  be  added  XA^^X'B^^,  shew  that  the  set  Blt  ...,  52<r+2  is 
derivable  from  the  set  A ,,...,  A2IT+2  by  addition  of  the  characteristic  XX'  to 
every  constituent.  This  is  contrary  to  the  definition  of  root  sets.  Conversely 
if  AI,  ...,  A'2a+»  be  any  one  of  the  2^  sets  which  are  derivable  from  the  root 
set  Alt  ...,  Av+a  by  equations  of  the  form  A-=ZAi,  the  set  of  2<r  +  l 

To  the  sets  Alt  ...,  A^^  and  X'A2,  ...,  X'A2<r+2  we  may  adjoin  respectively  their  respective 
sums.  The  two  sets  of  2ff  +  2  characteristics  thus  obtained  are  not  necessarily  the  same.  When 
ff  is  odd  they  cannot  be  the  same,  as  will  appear  below  (§  303). 

32—2 


500  UTILITY   OF   FUNDAMENTAL   SETS.  [302 

characteristics  of  the  same  character,  say  AI,  . ..,  A'2<r+l,  which  are  derivable 
from  AI,  ...,  -A'ar+i  by  equations  of  the  form  Ai  =  X'Al,  will  also  be  derived 
from  A1}  ...,  A2a+l  by  the  equations  AJ  =  XAi}  in  which  X  =  X'Z. 

On  the  whole  then  it  follows  that  there  are 


different  sets,  Aly  ...,A2<T+1,  of  2<r  +  l  characteristics  of  the  same  character, 
azygetic  in  threes,  subject  to  no  relation  connecting  an  even  number,  and 
incongruent  for  the  modulus  (P). 

Of  the  characteristics  A1}  ...,  A2<T+1  there  can  be  formed 

(2<r  +  1,  1)  +  (2<r+  1,  3)  +  ...  +  (2cr  +  1,  2(7  +  1)  =  22" 

combinations*,  each  consisting  of  an  odd  number  ;  and,  since  there  is  no 
relation  connecting  an  even  number  of  Al}  ...,  Aw+l,  no  two  of  these  com 
binations  can  be  equal.  These  combinations  all  belong  to  the  characteristics 
Alt  ...,  As,  satisfying  the  r  congruences  X,  Pf  =  |  Pt  \  ;  for 

I   ~A    ~A  ~A  PI—      T      P    I  _i_         _i_  I   /T  PI  —  IP 

|  -0.1-0.2  •••  •"•2fc—  1>   •*  i  \   —      •"•!>   ri  I  T   •••   T  I  •"•<&—  1>   *  <  I  =   I  J   t     • 

And  no  two  of  them  are  congruent  in  regard  to  the  modulus  (P)  ;  for  a 
relation  of  the  form 

AI  .  •  •  -a.2k—  i  —  •^•m-^-m+i  •  •  •  •"•m+2jA-*> 


wherein  P  is  a  characteristic  of  the  group  (P),  would  lead  to  a  relation  of  the 

form  A2p  =  A1A2...A2p_1P,  and  thence  give 

whereas 


P    A        A 

p—l-L    ,   -0.2p,    -tlj 


A1  ...  A2p_ly  A.2p,  A 


.2p,     2p+1 


T         T          ~A       7        i 

-"•i  •  ••  -"2p-i>  •/12p>  -"ap+i  | 

-"•!)   -"-2p>  -"2p+l     H~  •  •  •  +     -"-2p—  1  »  -"-2p, 


Thus  the  22(r  combinations,  each  consisting  of  an  odd  number  of  the 
characteristics  A1}  ...,  -4ar+i>  are  in  fact  the  characteristics  ^4a,  ...,  As.  We*f* 
call  the  set  A1}  ...,Aw+l  &  fundamental  set.  We  may  associate  therewith 
the  characteristic  -42<r+2  =  .41  ...  A2a+l,  which  is  azygetic  with  every  two  of  the 
set  A1}  ...,  Aw+l;  the  case  in  which  it  has  the  same  character  as  these  will 
appear  in  the  next  article.  And  it  should  be  remarked  that  the  argument 
establishes,  for  the  22<r  Gopel  systems  (A1P),  ...,  (ASP),  the  existence  of 
fundamental  sets,  (yljP),  ...,  (A2(r+lP),  which  are  Gopel  systems,  by  the  odd 
combinations  of  the  constituents  of  which,  the  constituents  of  the  systems 
(A-iP),  ...,  (ASP)  can  be  represented. 

*  Where  (n,  k)  denotes  n  (n-  l)...(?i-  k+  l)/k  I 

t  By  Frobenius  the  term  Fundamental  Set  is  applied  to  any  2o-  +  2  characteristics  (incon 
gruent  mod.  (P))  of  which  every  three  are  azygetic. 


303J  THEIR   CHARACTER.  501 

303.  The  characteristics  Aly  ...,  A.^+i  have  been  derived  to  have  the 
same  character.  We  proceed  to  shew  now,  in  conclusion,  that  this  character 
is  the  same  for  every  one  of  the  possible  fundamental  sets,  and  depends  only 

on  <r.     Let  (-7)  be  the  usual  sign  which  is  +1  or  —1  according  as  a-  is  a 
\4/ 

quadratic  residue  of  4  or  not,  in  other  words,  (-)  =  1   when  a-  is  =  1   or 

\4/ 

=  0  (mod.  4),  and  (  y  j  =  —  1  when  &  is  =  2  or  =  3  (mod.  4)  ;  then  the  character 

of  the  sets  Alt  ...,  Aw+l  is  |-J  ,  that  is,  A1}  ...,Aw+l  are  even  when  f-J  =  +  1 
and  are  otherwise  odd,  and  the  character  of  the  sum  A2<r+2  =  Al  ...  Ay,+\  is 
e™  I  -7  )  •  Or,  we  may  say 

when  er  =  1  (mod.  4),  Alt  .  ..,  A^+1  are  even,  A.2a+.2  is  odd  ; 

when  a  =  0,  Alt  ...,  A2a+l  are  even,  -4^+2  is  even, 
when  a  =  2  (mod.  4),  Alf  ...,  AZ<7+1  are  odd,  A2>,+<,  is  odd  ; 

when  a  =  3,  AI}  ...,  Aw+l  are  odd,  -4^+2  is  even. 
For  if  Aly  ...,  A2<T+l  be  all  of  character  e  we  have 

|  Al  A2  ...  A*+1  1  =  |  lj  |  +  ...  +  |  Z*+1  1  +  2  |  Ait  AJ  |, 
where  ^1^,  AJ  consist  of  every  pair  from  Aly  ...,  A^^  ;  also 


where  ^Ij,  4;,  -4/,  consist  of  every  triad  from  Alt  ...,  -4afc+il  hence,  since 
\Ai,  AJ,  Ah\  =  l,  and,  as  is  easily  seen,  n(n  —  \}(n—  2)/3  !  is  even  or  odd 
according  as  n  is  of  the  form  4m  +  1  or  4m  +  3,  it  follows  that  S  |  -4{,  -4j  |  is 
even  or  odd  according  as  2&  +  1  is  of  the  form  4>m  +  1  or  4m  +  3  ;  therefore 
A1AZ  ...  A&+1  has  the  character  e  or  —  e  according,  as  2k  +  1=1  or 
=  3  (mod.  4).  Thus  the  number  of  combinations  of  an  odd  number  from 
AI,  ...,  -4ar+i  which  have  the  character  e  is 

+  1,5)  +  (2o-+  1,9)  +  ... 
=  i  {(1  +  «)2<r+1  -  (1  -  «)2<r+1  +  1  (1  -  tV)2<r+1  -  i  (1  +  ^)2<7+1}a;=1 


=  22'-1  +  2*-*  sin  TT  ; 

4 

this  number  is  220""1  +  2"7"1  when  <r  =  0  or  a  =  1  (mod.  4)  ;  otherwise  it  is 
2'20""1  —  2"7"1  ;  now  we  have  shewn  (§  298)  that  the  characteristics  A1}  ...,  ^.g 
contain  respectively  22"7"1  +  20""1,  2'2"7"1  —  20""1  even  and  odd  characteristics,  and 
(§  302)  that  every  one  of  Alt  ...,  As  can  be  formed  as  an  odd  combina 
tion  from  Alt  ...,Ayr+l;  hence  e  =  +  l  when  a  =  0  or  o-  =  l  (mod.  4),  and 


502  SUMMARY    OF   RESULTS.  [303 

otherwise  e=— 1;  this  agrees  with  the  statement  made.  Further,  by  the  same 
argument  A^AZ  . . .  Aw+l  has  the  character  e  or  —  e  according  as  2o-  +  1  =  1 
or  =  3  (mod.  4) ;  and  this  leads  to  the  statement  made  for  A2^+2. 

The  reader  will  find  it  convenient  to  remember  that  the  combinations, 
from  the  fundamental  set  Al}  ...,  A.^+1)  consisting  of  1,  5,  9,  13,  ...  of  them, 
are  all  of  the  same  character,  and  the  combinations  consisting  of  3,  7,  11,  ... 
are  all  of  the  opposite  character. 

Ex.  If  Alt  ...,  ^42p  +  i  be  half-integer  characteristics  azygetic  in  pairs,  and  S  be  the 
sum  of  the  odd  ones  of  these,  prove  that  a  characteristic  formed  by  adding  S  to  a  sum  of 
any  p  +  r  characteristics  of  these  is  even  when  r=0  or  =1  (mod.  4),  and  odd  when  r=2  or 
=  3  (mod.  4).  (Stahl,  Crelle,  LXXXVIII.  (1879),  p.  273.) 

304.  It  is  desirable  now  to  frame  a  connected  statement  of  the  results 
thus  obtained.  It  is  possible,  in 

(2*?  -  1)  (22^-2  -  1)  ...  (2-^-2'-+2  -  l)/(2»>  -  1)  (2'-1  -  1)  ...  (2  -  1) 
ways,  to  form  a  group, 

0    p     p  p  p  P  P  P 

UJ   •*-   1»    -1-   2>    •••>   *!•*  iJ    •••»    •*,!•*  t-*»l    ••• 

of  2r  characteristics,  consisting  of  the  combinations  of  r  independent  charac 
teristics  Pa,  ...,  Pr,  such  that  every  two  characteristics  P,  P'  of  the  group 
are  syzygetic,  that  is,  satisfy  the  congruence  |  P,  P'  |  =  0,  (mod.  2).  Such  a 
group  is  denoted  by  (P),  and  two  characteristics  whose  difference  is  a 
characteristic  of  the  group  are  said  to  be  congruent  for  the  modulus  (P). 

From  such  a  group  (P),  by  adding  the  same  characteristic  A  to  each 
constituent,  we  form  a  system,  which  we  call  a  Gb'pel  system,  consisting  of 
the  combinations  of  an  odd  number  of  r+  1  characteristics  A,  AP1}  ...,  APr, 
among  an  even  number  of  which  there  exists  no  relation ;  this  system  is  such 
that  every  three  of  its  constituents,  say  L,  M,  N,  satisfy  the  congruence 
L,  M,  N  \  =  0,  or,  as  we  say,  are  syzygetic.  Such  a  Gb'pel  system  is 
represented  by  (AP). 

It  is  shewn  that  by  taking  22^~r  different  values  of  A  and  retaining  the 
same  group  (P),  we  can  thus  divide  the  22^  possible  characteristics  into 
<pp-r  Gopel  systems.  Among  these  %&-r  Gopel  systems  there  are  22P~2r 
systems  of  which  all  the  elements  have  the  same  character.  Putting 
2p  —  2r  =  2<r  we  shew  further  that  2°"~1  (2a  + 1)  of  these  Gopel  systems 
consist  wholly  of  even  characteristics,  and  that  2<r~1(2cr  — 1)  of  them  consist 
wholly  of  odd  characteristics.  Putting  s  =  22<r  we  denote  the  22<r  Gopel 
systems  which  have  a  distinct  character  by  (^iP),  ...,  (ASP);  and,  still 
retaining  the  same  group  (P),  we  proceed  to  consider  how  to  represent  these 
22<r  systems  by  means  of  2cr  -f  1  fundamental  systems. 

It  appears  then  that  from  the  characteristics  A1}  ...,  As  we  can  choose 
2o--l-l  characteristics  Alf  ...,  A2<T+1  in 

2 -  1)  ...  (22 - 


305]  EXAMPLES.  503 

ways,  such  that  every  three  of  them  are  azygetic,  and  all  have  the  same 
character;  this  character  is  not  at  our  disposal  but  is  that  of  (-  J  ;  the  sum 

\  T?  / 

of  Alt  ...,  A-a+i,  denoted  by  A2<r+2,  has  the  character  e™^).     Then  all  the 

\4v 

combinations  of  1,  5,  9,  ...  of  A1}  ...,  Aw^  have  the  character  f^j.  and  all 

\4/ 

the  combinations  of  3,  7,  11,  ...  have  the  opposite  character.  These  combi 
nations  in^  their  aggregate  are  the  characteristics  Alt  ...,  As.  The  charac 
teristics  Alt  ...,  A2(r+1  are,  like  A1}  ...,  At,  incongruent  for  the  modulus  (P). 
To  each  of  them,  say  Aiy  corresponds  a  Gopel  system  (AiP),  to  any  con 
stituent  of  which  statements  may  be  applied  analogous  to  those  made  for  Zf 
itself. 

The  characteristic  A^+.2  is  such  that  every  three  of  the  set  Alt  ...,  A^+.2 
are  azygetic.  This  set  is  in  fact  derived,  as  one  of  2cr  +  2  such,  from  a  set  of 
2<r  +  2  characteristics,  here  called  a  root  set,  which  satisfies  the  condition 
that  every  three  of  its  constituents  are  azygetic  without  satisfying  the 
condition  that  2<r  +  1  of  them  are  of  the  same  character.  There  are 


such  root  sets.     It  is  not  possible,  from  any  root  set,  to  obtain  another  by 
adding  the  same  characteristic  to  each  constituent  of  the  former  set. 

The  root  sets  are  not  the  most  general  possible  sets  of  2<r  +  2  charac 
teristics  of  which  every  three  are  azygetic.     Of  such  sets  there  are 

2«r«+,'a  (2*r  -  1)  .  .  .  (22  -  I)/  2CT  +  2, 


but  they  break  up  into  batches  of  22<r,  each  derivable  from  a  root  set  by  the 
addition  of  a  proper  characteristic  to  all  the  constituents  of  the  root  set. 

305.  As  examples  of  the  foregoing  theory  we  consider  now  the  cases  <r  =  0,  <r=  1,  o-  =  2, 
<r=p.  When  <r  =  0,  the  number  of  Gopel  groups  of  2"  pairwise  syzygetic  characteristics  is 

(2"+l)(2J>-i  +  l)  ......  (2  +  1); 

from  any  such  group  we  can,  by  the  addition  of  the  same  characteristic  to  each  of  its 
constituents  obtain  one  Gopel  system  consisting  wholly  of  characteristics  of  the  same  even 
character.  These  results  have  already  been  obtained  in  case  p  =  2  (§  289,  Ex.  iv.), 
and,  as  in  that  particular  case,  the  2f>-  1  other  systems  obtainable  from  the  Gopel  group 
by  the  addition  of  the  same  characteristic  to  each  constituent,  contain  as  many  odd 
characteristics  as  even  characteristics. 

When  o-=l,  we  can,  from  any  Gopel  group  of  2"-1  pairwise  syzygetic  characteristics, 
obtain  4  Gopel  systems,  three  of  them  consisting  of  2"-i  even  characteristics  and  one  of 
2*  -i  odd  characteristics.  The  characteristics  of  the  latter  (odd)  system  are  obtainable  as 
the  sums  of  three  characteristics  taken  one  from  each  of  the  three  even  systems. 

Whon  o-  =  2,  the  number  of  fundamental  sets  Alt  ...,  A&  is 


504  THE   CASE   WHEN   a   IS   3.  [305 

each  of  them  has  the  character  (jj,  or  is  odd,  and  their  sum,  A6,  is  odd.     Among  the 

22*=16  characteristics  A1,  ...,  As  there  are  ^2cr~1-2<r~1  or  6  odd  characteristics;  these 
clearly  consist  of  the  characteristics  Alf  ...,  A6  ;  the  six  fundamental  sets  are  obtained  by 
neglecting  each  of  Alt  ...,  A6  in  turn.  Among  the  characteristics  Alt  ...,  As  there  are  10 
even  characteristics,  obtainable  by  combining  A^  ...,  Ag  in  threes.  And,  to  each  of  the 
characteristics  Alt  ...,  Ag  corresponds  a  Gopel  system  of  2r=2P-<r  =  2^'~2  characteristics, 
for  the  constituents  of  which  similar  statements  may  be  made. 

Of  the  cases  for  which  a-  =  2,  the  case  p  =  2  is  the  simplest.  After  what  has  been  said 
in  Chap.  XL,  and  elsewhere,  we  can  leave  that  case  aside  here.  For  jo  =  3  the  Gopel 
systems  consist  of  two  characteristics  ;  adopting,  for  instance,  as  the  group  (P),  the  pair 

^  \OOOJ  '  ^  (loo)  '  ^G  conc^tion  for  the  characteristics  Al,  ...,  A^  namely  |  X,  Pl  =  P1\, 
reduces  to  the  condition  that  the  first  element  of  the  upper  row  of  the  characteristic 
symbol  of  X  shall  be  zero  ;  hence  the  16  characteristics  Alf  ...,  A,  may  be  taken  to  be 

i  (n    1     2  )  »  wnere  if1     2  )  represents  in  turn  all  the  characteristic  symbols  for  p  =  2. 
\0  QI   a2  /  •  \QI   a2  / 

Taking  next  the  case  o-  =  3,  there  are  s=22<r=64  Gopel  systems,  (AP),  each  consisting 
wholly  either  of  odd  characteristics  or  of  even  characteristics,  there  being  2"-1  (2*  -  1),  =  28, 
odd  systems,  and  36  even  systems.  From  the  representatives,  Alt  ...,  Ag,  of  these  systems, 
which  are  incongruent  mod.  (P),  we  can  choose  a  fundamental  set  of  7  characteristics 
Alt  ...,Af  in 

29  (26-1)  (2*-  1)  (22-1)     _ 

17  »   —zoo, 

ways;   Alt  ...,  Aj  will  be  odd,   and   their  sum,  J8,  will  be  even;   for  (?J  =  (£)=-!, 

6™  \4J  =  1'  ^e  set  ^n  '"'  ^7>  ^8  ^s>  ^n  accor(iance  witn  ^e  theory,  derived  from  one 
of  288/(2o-  +  2),  =36,  root  sets  A»_...,A%  (§  301),  by  equations  of  the  form  A^XAi,  in 
which  X  is  so  chosen  that  A1}  ...,  A7  are  of  the  same  character  ;  from  this  root  set  we  can 
similarly  derive  8  fundamental  sets  of  seven  odd  characteristics,  according  as  it  is  A6  or  is 
one  of  Alt  ...,  A7  which  is  left  aside.  Now  the  fact  is,  that,  in  whichever  of  the  eight 
ways  we  pass  from  the  root  set  to  the  seven  fundamental  odd  characteristics,  the  sum  of 
these  seven  fundamental  characteristics  is  the  same.  We  see  this  immediately  in  an 
indirect  way.  Let  A  lt  ...,  Aj  be  a  fundamental  set  of  odd  characteristics  derived  from  the 
root_set  Alt  ...,A8_by_  the  equations  A^XAi;  putting  A8  =  A1...  J7,  consider  the  set 
As,  A^A^A^  ...,  A^AVA^  Alt  derived  from  A1,  ...,  J8  by  adding  A^A^  to  each  ;  in  the  first 
place  it  consists  of  one  even  characteristic,  J8,  and  seven  odd  characteristics  ;  for 


i,  At\=  At,Ai,At\  =  l,  (mod.  2), 
because  Alt  ...,  A&  are  azygetic  in  threes  ;  in  the  next  place 

I  AS)  A1}  A^AiAi\m\  As,  AH  ^|  =  1, 

so  that^every  three  of  its  constituents  are  azygetic.  Hence  the  characteristics  As  A1A2, 
...,  A^Aj^Aj,  Aj,  which,  as  easy  to  see,  are  not  congruent  to  Alt  ...,  Aj  mod.  (P),  form, 
equally  with  Aly  ...,  A7,  a  fundamental  set,  whose  sum  is  likewise  As  ;  they  are  derived 
from  Alt  ...,  A8  by  adding  A^A-^X  to  each  of  these.  There  are  clearly  six  other  jsuch 
fundamental  sets,  derived  from  Aly  ...,  As  by  adding  respectively  ASA2X,  ...,  A8A^X. 
Hence  to  each  of  the  36  root  sets  there  corresponds  a  certain  even  characteristic  and  to 
each  of  these  even  characteristics  there  correspond  8  fundamental  sets.  We  can  now  shew 
further  that  the  even  characteristics,  thus  associated  each  with  one  of  the  36  root  sets,  are 


306]  APPLICATION    TO   THETA   FUNCTIONS.  505 

in  fact  the  36  possible*  even  characteristics  of  the  set  Jj,  ...,  As.  This  again  we  shew 
indirectly  by  shewing  how  to  form  the  remaining  7  .  36  fundamental  systems  from  the 
system  Alt  ...,  An.  The  seven  characteristics  AKAZA3,  ASA3A1,  A^Aj^A^,  At,  A^,  A6,  A7, 
are  in  fact  incongruent  mod.  (P),  they  are  all  odd,  have  for  sum  A1A2A3,  which  is  even, 
and  are  azygetic  in  threes  ;  for  ASA2A3  is  a  combination  of  five  of  A  l  ,  .  .  .  ,  A  7  ,  and 

14,  Z5|+|13,  I4,  16    =1,      |  Z4,  J6,  I6|  =  l, 


(the  modulus  in  each  case  being  2)  ;  hence  these  seven  characteristics  form  a  fundamental 
system.  There  are  35  sets  of  three  characteristics,  such  as  Alt  A2,  A3,  derivable  from  the 
seven  Alt  ...,  A7  ;  each  of  these  corresponds  to  such  a  fundamental  system  as  that  just 
explained  ;  and  each  of  these  fundamental  systems  is  associated  with  seven  other  funda 
mental  systems,  derived  from  it  by  the  process  whereby  the  set  A{,  Z<ZS14S,  ...,  AiAsA7 
is  derived  from  A^  ...,  A7. 

When  or  =/>,  a  Gopel  system  consists  of  one  characteristic  only  ;  we  can,  in 


/p\ 
ways,  determine  a  set  of  2/>  +  l  characteristics,  all  of  character  (  ^  J  ,  of  which  every  three 

/%)\ 
are  azygetic  ;  their  sum  will  be  of  character  e"ip  I  ^  )  >  a^  ^he  possible  2%'  characteristics 

can  be  represented  as  combinations  of  an  odd  number  of  these. 

306.  We  pass  now  to  some  applications  of  the  foregoing  theory  to  the 
theta  functions.  The  results  obtained  are  based  upon  the  consideration  of  the 
theta  function  of  the  second  order  defined  by 

</>  (M,  a  ;  %q)  =  ^  (u  +  a  ;  %q)  ^  (u  -  a  ;  %q), 

where  ^q  is  a  half-integer  characteristic;  as  theta  function  of  the  second 
order  this  function  has  zero  characteristic  ;  the  addition  of  any  integers  to 
the  elements  of  the  characteristic  ^q  does  not  affect  the  value  of  the  function. 
By  means  of  the  formulae  (§  190,  Chap.  X.), 


wherein  N  denotes  a  row  of  integers  and  X(?*;  s)  =  Hii(u  +  ^fls)  —  iriss,  we 
immediately  find 

>  a  ;  1  q)  =  ^  **>  <f>  (u,  a  ; 


where  %kq  denotes  the  sum  of  the  characteristics  %k,  ^q;  to  save  the  repeti 
tion  of  the  ^,  this  equation  will  in  future  be  written  in  the  form  (cf.  §  294) 

0  (u 

when  the  contrary  is  not  stated  capital  letters  will  denote  half-integer 
characteristics,  and  KQ  will  denote  the  reduced  sum  of  the  characteristics 
K,  Q,  having  for  each  of  its  elements  either  0  or  £. 

*  Thus,  when  p  =  3=ff,  the  result  quoted  in  §  205,  Chap.  XI.,  is  justified. 


506  A   THETA   FUNCTION   OF   THE   SECOND   ORDER  [306 

We  shall  be  concerned  with  groups  of  2''  pairwise  syzygetic  characteristics, 
such  as  have  been  called  Gopel  groups,  and  denoted  by  (P) ;  corresponding 
to  the  r  characteristics  P1(  ...,Pr  from  which  such  a  group  is  formed,  we 
introduce  r  fourth  roots  of  unity,  denoted  by  en  ...,  er,  which  are  such  that 

6  2  _  Qiri  I  P,  I  ?    _  ^2  _  ewi  I  Pf  I  . 

the  signs  of  these  symbols  are,  at  starting,  arbitrary,  but  are  to  be  the  same 
throughout  unless  the  contrary  be  stated.  Since  the  characteristics  of  the 
group  (P)  satisfy  the  conditions 

|  Pi,  Pj  \  =  0,  (mod.  2), 


we  may,  without  ambiguity,  associate  with  the  compound  characteristics  of 
the  group  the  2r  —  r  symbols  denned  by 

eo=l,     ei)j  =  ei 

i  Pi  \  /PA  /PA  /PA  /  P,-  \  /  P*  \ 

*,  ;,  *  =  *<?;,  k  (p  p  J  =  ef  6;  6A  I  I  1  (I  =  6J6*.  ;  [ppj  =  €*  €f,  j  (  p  p    I  , 

\fjfJt/  \-L  k/   V*  »/  V-1-  j'  x-4  ik-^  t'  v*  t-1  7' 


. 

and  ej  =  et-f  ^  «=  e^e^  I    p      ,  etc. 

V  *< 

Consider  now  the  function*  denned  by 


where  A  is  an  arbitrary  half-integer  characteristic,  and  Pi  denotes  in  turn  all 
the  2r  characteristics  of  the  group  (P).  Adding  to  u  a  half-period  Qpk, 
corresponding  to  a  characteristic  Pk  of  the  group  (P),  we  obtain 

<t>  (u  4-  nPjfc,  a;  A)  — 
if  then  P^  =  PiP*,  or  P{  =  PhPk,  we  have 

P\      /       P,      \  /Pi\      /P,  \     /P,  \      /P,\      /P,\  /P.. 

i\  I    *  1    \  I  •rh\  I  J-  k\  I  *  k\  (fm\  f  •*  il  I  r  h  ,    .  „ 

—  fcfcc 

now,  as  Pi  becomes  in  turn  all  the  characteristics  of  the  group  (P),  Ph,  =  PiPk, 
also  becomes  all  the  characteristics  of  the  group,  in  general  in  a  different 
order ;  thus  we  have 

>,«;  A), 


*  If  preferred  the  sign  (      )  ,  whose  value  is  ±  1,  may  be  absorbed  in  ej .     But  there  is  a 
tain  convenience  in  writing  it  explicitly. 


307]  WITH    A    GOI'EL   SYSTEM   AS   PERIODS.  507 

If  2fl3[  be  any  period,  we  immediately  find 

4>  (w  +  2&M,  a  I  -4)  =  e2A(W;  m  <&  (u,  a  ;  A). 

Thus,  X(w;  P*)  being  a  linear  function  of  the  arguments  %,  ...,  up,  the 
function  <3>  (w,  a;  -4)  is  a  theta  function  of  the  second  order  with  zero 
characteristic,  having  the  additional  property  that  all  the  partial  differential 
coefficients  of  its  logarithm,  of  the  second  order,  have  the  2r  sets  of  simul 
taneous  periods  denoted  by  the  symbols  ^ipk- 

Ex.  i.     If  S  be  a  half-integer  characteristic  which  in  syzygetic  with  every  characteristic 
of  the  group  (/*),  prove  that 

*  (u  +  Q,,  a  ;  A)  =  e*(u< 


and 

jfilt1.  ii.     If  Pj;  be  any  characteristic  of  the  group  (1*),  prove  that 
4>  (u,  a  •  Al\}  =  (        «-i  *  («,  a  ;  ^1). 


j&a;.  iii.     When,  as  in  Ex.  i.,  S  is  syzygetic  with  every  characteristic  of  the  group  (P), 
shew  that 

e-'IS'V  *  («,  a  ;  APk)  *  (•»,  Z>  ;  APt)  =  e*i{s*  *(M,  a  ;  J)  *  (»,  6  ;  ^1). 

Conversely  it  can  be  shewn  that  if  a  theta  function  of  the  second  order 
with  zero  characteristic,  H  (w),  which,  therefore,  satisfies  the  equation 

II(tt+fl,»)  =  e2A'»<M)  n(«), 

for  integral  m,  be  further  such  that  for  each  of  the  two  half-periods  associated 
with  the  characteristics  \m  =  P,  ^m  =  Q,  there  exists  an  equation  of  the  form 

n  (u  +  %tim)  =  e^+"1«i+-+"/.«;.  n  (u), 

where  p,  vl}  ...,  vp  are  independent  of  u,  then  the  characteristics  P,  Q  must 
be  syzygetic.     Putting  vii  =  v1n1+  ......  +  vpup,  we  infer  from  the  equation 

just  written  that 

n  (u  +  nm)  =  ^+-(«+i«m)  n  (u  +  ^nw)  =  &+*™+wm  n  (M)  ; 

comparing  this  with  the  equation 

n  (u  +  n,a)  =  e2A'»(M)  n  (M)  =  e*u™<H+*a>»>-*rimm'  n  (%) 

we  infer  that  v  =  Hm,  p  =  kiri  +  ^HmQm  —  'iriiniri,  where  k  is  integral,  and 
hence 

n  (u  +  |nm)  =  +  e-i-*»M»'+2A<us  J?w)  n  ^w^ 

307.     In  accordance  with  these  indications,  let  Q(u)  denote  an  analytical 
integral  function  of  the  arguments  w1}  ...,  up  which  satisfies  the  equations 

Q(u  +  nm)  =  ^"'^'  Q(u);     Q(w  +  ftPjfc)  =  efce«i^i+^«5^>  Q(M), 
for  every  integral  m  and  every  half-integer  characteristic  P^  of  the  group  (P). 


508  GENERAL   EXPRESSION    OF    SUCH   A    FUNCTION.  [307 

We  may  regard  the  group  (P)  as  consisting  of  part  of  a  group  of  2^ 
painvise  syzygetic  characteristics  formed  by  all  the  combinations  of  the 
constituents  of  the  group  (P)  with  the  constituents  of  another  pairwise 
syzygetic  group  (R)  of  %P~r  characteristics.  Then  the  2?  characteristics  of 
the  compound  group  are  obtainable  in  the  form  PiRj,  wherein  P{  has  the  2r 
values  of  the  group  (P),  and  Rj  has  the  2^~r  values  of  the  group  (R).  Since 
every  2^+1  theta  functions  of  the  second  order  and  the  same  characteristic 
are  connected  by  a  linear  equation,  we  have 

CQ(u)=2Ci>j<f>(u,a; 


where  C,  Gitj  are  independent  of  u  and  are  not  all  zero*.     Hence,  adding  to 
u  the  half-period  Qpk,  we  have 


*j  Q  (u)  =  2  Citj  e^->  ^  ^  LJ  4>  (u,  a  ;  P{PkRj), 

and  therefore,  as  q,^*'p*J  =  e"1, 

/  p    \ 
CQ  (u)  =  2  Cij  (p  »- J  e*</>  (w,  a ;  PiPkRj) ; 

forming  this  equation  for  each  of  the  2r  values  of  Pk,  and  adding  the  results, 
we  have 


herein  put  Ph  =  PiPk,  so  that  as,  for  any  value  of  i,  Pk  becomes  in  turn  all 
the  characteristics  of  the  group  (P),  the  characteristic  P^  also  becomes  all  the 
characteristics  in  turn,  in  general  in  a  different  order  ;  then 

Ph\  /PhPi\  /Ph\  /P 

m   =  €h€i 

and,  therefore, 

u)  =  2  2  eh 

j    h 


where 

* 


and  thus 


Now  the  2^~r  functions  <E>  (tt,  a  ;  Rj)  are  not  in  general  connected  by  any 
linear  relation  with  coefficients  independent  of  u  ;  for  such  a  relation  would 
be  of  the  form 


*  It  is  proved  below  (§  308)  that  the  functions  <f>  (u,  a  ;  P{Rj)  are  linearly  independent,  so 
that,  in  fact,  C  is  not  zero. 


308]  THE  GENERAL  THEOREM.  509 

wherein  Hi  is  independent  of  u,  and  Qi  becomes,  in  turn,  all  the  constituents 
of  a  group  (Q)  of  2^  pairwise  syzygetic  characteristics,  and  we  shall  prove  (in 
§  308)  that  such  a  relation  is  impossible  for  general  values  of  the  arguments 
a.  Hence,  all  theta  functions  of  the  second  order,  with,  zero  characteristic, 
which  satisfy  the  equation 

Q(u  +  flPjfc)  =  ete«'ip*i+2A<«s  *V  Q  (u) 

for  every  half-integer  characteristic  Pk  of  the  group  (P),  are  representable 
linearly  by  2^"*",  =  2",  of  them,  with  coefficients  independent  of  u.  We  have 
shewn  that  the  functions  <I>  (u,  a;  A),  defined  by  the  equation 

u-a;  APt), 

where  the  summation  includes  2r  terms,  are  a  particular  case  of  such  theta 
functions. 

308.     Suppose  there  exists  a  relation  of  the  form 


where  the  summation  extends  to  all  the  2?)  characteristics  Q{  of  a  Gopel  group  (Q),  and  Hi 
is  independent  of  u.  Putting  for  u,  it  +  QQa,  where  Qa  is  a  characteristic  of  the  group  (Q), 
we  obtain 


hence,  if  tlt  ...,  ep  are  fourth  roots  of  unity  associated  with  a  basis  Qlt  ...,  Qp  of  the  group 
(Q),  as  before,  and  this  equation  be  multiplied  by  fa,  and  the  equations  of  this  form 
obtained  by  taking  Qa  to  be,  in  turn,  all  the  2p  characteristics  of  the  group  (Q),  be  added 
together,  we  have 


now  let  Qj-=QaQi}  then  for  any  value  of  i,  as  Qa  becomes  all  the  characteristics  of  the 
group  (Q),  Qj  will  become  all  those  characteristics  ;  therefore,  substituting 


we  have 


hence  one  at  least  of  the  expressions 

2f>3  (u  +  a;  A  Qj)  9(u  +  b 

J  i 

must  vanish. 

Here  €15  e2,  ...  have  any  one  of  2"  possible  sets  of  values.    The  expression  S/^ef1  cannot 

i 

vanish  for  every  one  of  these  sets  ;  for,  multiplying  by  e/1,  we  have  then 


where  fiti,  like  e^,  becomes  in  turn  the  symbol  associated  with  every  characteristic  of  the 
group,  and  there  are  2*>  equations  of  this  form;  adding  these  equations  we  infer  #,  =  0, 
and,  therefore,  as^'  is  arbitrary,  we  infer  that  all  the  coefficients  are  zero. 


510  FIRST   APPLICATION  [308 

Hence  it  follows  that  there  is  at  least  one  of  the  '2p  sets  of  values  for  e1}  «„,  ...,  for 
which 

2cy  .9  (u  +  a;  A  Q-)  3  (u  +  b  ;  A  Qj)  =  0. 

./ 

When  the  arguments  u  +  a,  u  +  b  are  independent,  this  is  impossible;  for  putting 
u  +  a=U,  n  +  b—V,  this  is  an  equation  connecting  the  2"  functions  3(U;  AQj)  in  which 
the  coefficients  are  independent  of  £7(cf.  §§  282,  283,  Chap.  XV.). 


When  the  arguments  u  +  a,  u  +  b  are  not  independent,  this  equation  is  not  impossible. 
For  instance,  if  flc=  -e*1™1  &l,  it  is  easy  to  verify  that 


;  Qh)3(u;  Qh) 

and  hence  the  equation  does  hold  when  A  =  0,  a  =  QQ  ,  6  =  0,  ek=  —  e*1™'^*  •',  for  all 
the  values  of  e1,  ...,  *,._,,  (k  +  l,  ...,  fp.  For  any  values  of  the  arguments  u  +  a,  u  +  b 
we  infer  from  the  reasoning  here  given  that  if  the  functions  9  (u  +  a  ;  AQ^S^  +  b;  AQt) 
are  connected  by  a  linear  equation  with  coefficients,  H^  independent  of  u,  then  (i)  they 
are  connected  by  at  least  one  equation 


for  one  of  the  2"  sets  of  values  of  the  quantities  fl,  f2,  ...,  and  (ii)  similarly,  since  the  2* 
functions  3  (u  +  a;  AQi)9(u  +  b;  AQ-)  do  not  all  vanish  identically,  that  the  coefficients 
are  connected  by  at  least  one  equation 


309.  The  result  of  §  307  is  of  great  generality;  we  proceed  to  give 
examples  of  its  application  (§§  309  —  313).  The  simplest,  as  well  as  the  most 
important,  case  is  that  in  which  cr  =  0,  r=p,  and  to  that  we  give  most 
attention  (§§  309—311). 

When  <r  =  0,  any  two  of  the  functions  <£(>,  a;  A)  are  connected  by  a 
linear  equation,  in  which  the  coefficients  are  independent  of  u.  If  v,  a,  b  be 
any  arguments,  and  A,  B  any  half-integer  characteristics,  introducing  the 
symbol  e  to  put  in  evidence  the  fact  that  3>(u,  a;  A)  is  formed  with  one 
of  2^  possible  selections  for  the  symbols  e1,...,€p,  and  so  writing  <I>  (u,  a;  A,e) 
for  4>(w,  a;  A),  we  therefore  have  the  fundamental  equation 

3>(u  v  A   c^^(u>b;B,e)^(a,v-A,e) 


By  adding  the  2?  equations  of  this  form*  which  arise  by  giving  all  the 
possible  sets  of  values  to  the  fourth  roots  of  unity  e^  ...,  e^,  bearing  in  mind 
that  every  symbol  e{,  except  e0,  =  1,  occurs  as  often  with  the  positive  as  with 
the  negative  sign,  we  obtain 


(a,v,  A,  e) 


,3>(a,b;B,  e) 

*  Wherein  it  is  assumed  that  a,  b  have  not  such  special  values  that  any  one  of  the  2?  quanti 
ties  *  (a,  6  ;  B,  e)  vanishes.     Of.  §  308. 


309]  OF  THE  GENERAL  THEOREM.  511 

whereby  the  function  <f>  (u,  v  ;  A)  is  expressed  in  terms  of  2^  functions 

<I>  (u,  b  ;  B,  e). 
By  taking,  in  the  formula 

3>  (u,  v;  A,  e)  <&  (a,  b  ;  B,  e)  =  ^  (u,  b;  B,  e)  <£  (a,  v  ;  4,  e), 


or 


A       E 

j     X-'1  /   \-O 

=  2  2  6,6; <*> (»*,  6 ;  BPt)  ^(a,v;  APj). 


all  the  2^  possible  sets  of  values  for  elt  ...,  ep,  and  adding  the  results,  we 
obtain 


increasing  a  and  b  each  by  the  half-period  H^,  we  have 

t;  ;  ^^Pf)  </>  (a,  b  ;  5JKP,-) 

«iWf«**«l.#<«tfci  BPi)<f>(a)v; 


taking  R  to  be  all  the  possible  2^  half-integer  characteristics  in  turn,  and 
adding  the  resulting  equations  we  deduce*,  putting  C  =  AB, 

,  b;  AC)(j)(a,v;  A) 

e«  i  ^  i  <f>  (u,  v  •  RAPt)  <t>(a,b;  RA  P£) 


i   R   \    ^     J 

?(AS\  nilASl.,          ^  ..     ,     Q~ 
=  Zi  I    ~    I  e •    '    "  i  <p  (ii,  v  ',  £>)  <p  (a,  o ;  £>0), 
s  V  t/  / 

where  -4,  (7  are  arbitrary  half-integer  characteristics,  and  S  becomes  all  2^ 

possible  half-integer  characteristics  in  turn  ;  for  (Ex.  ii.  §  295),  Se7"1-^  ^1  =  2^ 

it 

when  P;  =  0,  and  is  otherwise  zero,  while,  for  any  definite  characteristic  APit 
as  R  becomes  all  possible  characteristics,  so  does  RAP{.  The  formula  can  be 
simplified  by  adding  the  half-period  £lc  to  the  argument  b;  the  result  is 
obtainable  directly  by  taking  C=  0  in  the  formula  written. 

This  agrees  with  a  result  previously  obtained  (§  292,  Chap.  XVI.) ;  for  a 
generalisation  of  it,  see  below,  §  314. 

*  This  equation  has  been  called  the  Riemann  theta  formula.     Cf.  Prym,  Untersuchmifien  Hber 
(lit-  Riemaim'telu  Thftnfarmcl,  Leipzig,  1882. 


512  INDICATION   OF  [310 

310.  The  formula  just  obtained  may  be  regarded  as  a  particular  case  of  another  which 
is  immediately  deducible  therefrom.  Let  (K )  be  a  group  of  2M  characteristics  formed  by 
taking  all  the  combinations  of  p.  independent  characteristics  Klt  ...,  K^;  if  A  be  any 
characteristic  whatever,  we  have 


according  as  \A,  _ffj|==0  (for  i  =  l,  ...,  /*),  or  not;  hence,  putting  (7=0  in  the  formula 
of  §  309,  and  replacing  the  A  of  that  formula  by  Kit  we  deduce 

2^  ^        •        JT  •     IT  O 

2^-M2e"|ji^l^(M,  6;  Ki)(f>(a,v,  Ari)  =  2-'A  2  e"14^1  Se^1^81^  (w,  v;  S)<j)(a,b;  S), 
where  £  becomes  all  22*>  characteristics, 
=  2   ^2  e7™  2  c          '    *  <p  (u,  V ',  S}  <f>  (a,  b ;  >S) 

,S'  i=l 

/  2^      •  \ 

n  ~u  Tri  I  j4 1  «    iri    ^4-R     /    «     Trt  72,  Ay    \     .    /  A  r>\     i    /         T          ,*  />\ 

=:  2      e  2e  (2e  /V  (%>  ^ !  •"  ^/  0  \^*>  ^  >  •"  v> 

J{  \i=l  / 

where  R  becomes  all  22p  characteristics, 

(a,b;  AR\ 


it 


where  R  extends  to  all  the  22p~'A  characteristics  for  which  |  R,  Ki\  =  0,  ...,  \  R, 
Putting  w  +  Ojg,  a  +  QB  for  u,  a  respectively,  and  replacing  AB  by  C,  we  obtain 


~  , 

**  1  BCL;  I    •  / 

e    '        J  $  (M,  v 
j=i 

here  (A")  is  any  group  of  2^  characteristics,  (Z)  is  an  adjoint  group  of  22p~'4  characteristics 
defined  by  the  conditions  \L,  K\  =  Q  (mod.  2),  and  B,  C  are  arbitrary  half-integer 
characteristics.  The  formula  of  the  previous  Article  is  obtained  by  taking  /x  =  0.  The 
formula  of  the  present  Article  may  be  regarded  as  a  particular  case  of  that  given  below 
in  §  315. 

311.  The  function  <j)(u,  v;  A)  is  unaffected  by  the  addition  of  integers 
to  the  half-integer  characteristic  A  ;  we  may  therefore  suppose  that  in  the 
functions  <£  (u,  v,  APi)  which  have  frequently  occurred  in  the  preceding 
Articles,  the  characteristic  APi  is  reduced,  all  its  elements  being  either  0  or  \. 
In  the  applications  which  now  immediately  follow  (§  311)  it  is  convenient,  to 
avoid  the  explicit  appearance  of  certain  fourth  roots  of  unity  (cf.  Ex.  vii., 
p.  469),  not  to  use  reduced  characteristics.  Two,  or  more,  characteristics 
which  are  to  be  added  without  reduction  will  be  placed  with  a  comma  between 
them  ;  thus  A,  Pi  denotes  A  +  Pt.  The  characteristics  Pt-  are  still  supposed 
reduced. 

Taking  the  formula  (§  309) 

^  3>  (u,  b  ;  A',  e)  <£  (a,  v;  A,  e) 

- 


311]  COROLLARIES.  513 

where  A'  replaces  the  B  of  §  309,  suppose  a  =  b,  and  put,  for 

u  -  b,     a  +  v,     a-v,     u  +  v,     u-v,     a  +  b,     a  -  b,     u  +  b, 
respectively, 

U,     V,     W,     U+V,     U+W,     V+W,    0,     U+V+W; 
then  we  obtain 

;  A)*(U+W;  A) 


!  C')e**(F+  w  ;  A'> 

adding  to  V  and  W  respectively  the  half-periods  flB,  flc,  this  becomes 
**\U,  F;  A,B][U,  W-  A,C] 

2  2  vMttjW  V,  W;  A',  B,  C,  PJ  [U;  A',  P{]  [V;A,B,  Pj]  [  W;  A,  C,  Pj] 


=  2 


1    3 


2vk8t[V,  W;  A'.B,  C,Pk][0-  A',Pk] 

k 

wherein  [U,V;A,B]  denotes  ^  [U+V-  A+B],  etc.,  ^=  f        6,,  ^  =  €it 

\^L  /  V^l  / 

/  /Q'\  /    f\  /     '\ 

etc.,  and,  if  £  =  £       )  ,  C'  =  i(^  )  ,  P,  =  i(^'  )  ,  then  ^^  sfc  are  fourth  roots  of 

\P  '  \V/  V^r/ 

unity  given  by  ^^-  =  e-J»»(^'-h'')(?l.+g(.))  5jfc  =  e-JiriO'+y')9Jfct 

In  connexion  with  this  formula  several  results  may  be  deduced. 

(a)     Putting  W  =  -  V,  A  +  B  =  K,  A  +  G  =  D,  A'  =  D,  the  formula  gives 
an  expression  of  *[U+  V;  K]*[U-V;  D]  in  terms  of  the  quantities 

*  [V;  KP<],  *[U-t  DP,],  ^[V-  DP,],  *[0;  KP,], 


the  expre-ssion  contains  in  the  denominator  only  the  constants  ^  [0  ;  KPt], 
[0;  DP{];  it  has  been  shewn  (§  299)  that  not  all  the  characteristics  KP-, 
i  can  be  odd. 


Putting    further   K  =  Q,    we    obtain    an    expression    of    ^IU+V-    01 
*[U-V-,  D]  in  terms  of 


-,  Pt],    *[V-  P.;],    *[U;  DP,],    ^[F;  DP,],    ^[0;  P,], 


Dividing  the  former  result  by  the  latter  we  obtain  an  expression  for 
U+  V-  K]/*[U+  V-  0]  in  terms  of  theta  functions  of  U  &nd  Fwith  the 
characteristics  DPt,  KP,,  P{,  the  coefficients  being  combinations  of  &  [0  ;  PJ, 
^[0;  DP,],  ^[0;  KP{]  with  numerical  quantities.  In  this  expression  the 
characteristic  D  is  arbitrary  ;  it  may  for  instance  be  taken  to  be  zero. 


33 


514  INDICATION    OF  [311 

The  formulae  are  very  remarkable  ;  replacing,  on  the  right  hand,  et-ewil^'  'V 
by  €i,  as  is  clearly  allowable,  and  taking  .0  =  0,  they  are  both  included  in  the 
following  formula  (cf.  Ex.  viii.  §  317) 

-v;  0] 


;  P0) 

ik'\  !Q  '\ 

where  K  =  4    7  )  ,  Pa  =  i          ,  and  the  summation  in  regard  to  a  extends  to 
2W  2Vga/ 

all  the  2?  characteristics,  Pa,  of  the  group  (P). 

It  is  assumed  that  the  characteristic  K  is  such  that  the  denominator  on 
the  right  hand  does  not  vanish  for  any  one  of  the  2?  sets  of  values  for  the 
quantities  ea  .  For  instance  the  case  when  K  is  one  of  the  characteristics  of 
the  group  (P),  other  than  zero,  is  excluded  (cf.  §  308). 

Ex.  i.     For  p  =  l,  if  P  denote  any  one  of  the  half-integer  characteristics  other  than 
zero, 

[3*  (u)  32  (v)  +  3*p  (u)  4  („)]  52  (0)  -  [32  (u)  4  (v)  +e™  I  p  1  ^  (it)  32  (*)]  4  (0) 


where  5  (w),  ^P(w)  denote  3  (u;  0),  5  (u;  P),  etc. 
.£&.  ii.     By  putting,  in  case  p  =  2, 


deduce  from  the  formula  of  the  text  that 
4^2  (0)  $01  (°)  502  ("  +  «')  ^5  (v  ~u')=   2 

^1  >  ^2 

wherein  £,=  +1,  f2=  +1,  and 


A',  B',  C",  I?  denoting  the  same  functions  of  the  arguments  u'. 

Hence  obtain  the  formula  given  at  the  bottom  of  page  457  of  this  volume. 

08)     Putting  B=  C,  V=W=0,A'  =  A,  we  obtain 

tij  [U;  A,  B,  B,  P{][U;  AP<]  [0  ;  A,  B, 


o;  A,B,B,Pk][0;  A,  Pk] 

k 

which  shews  that  the  square  of  any  theta  function  is  expressible  as  a  linear 
function  of  the  squares  of  the  theta  functions  with  the  characteristics  forming 
the  Gopel  system  (^1P).  We  omit  the  proof  that  these  2?  squares, 
^(U;  APi),  are  not  in  general  connected*  by  any  linear  relation  in  which 
the  coefficients  are  independent  of  U. 

*  Cf.  the  concluding  remark  of  §  308,  §  291,  Ex.  iv.  and  §  283. 


311]  COROLLARIES.  515 

Ex.     For  p  =  2  obtain  the  formula 


where  52  =  52  (0),  etc. 

(7)     There  is  however  a  biquadratic  relation  connecting  the  functions 
£  (u  ;  APi)  provided  p  be  greater  than  1.     In  the  formula  (§  309) 

(a-b;  A,  Pt) 

(a-v;  A,  1\\ 

supposing  the  characteristic  A  to  be  chosen  so  that  all  the  characteristics 
APt  are  even,  as  is  possible  (§  299)  by  taking  A  suitably,  substitute  for 

u  +  v,     u-v,     a  +  b,     a  —  b,     u  +  b,     u—b,     a  +  v,     a—v 
respectively 

u  +  v  +  w,     u-v,     a  +  b  +  w,     a-b,     u  +  b  +  w,     u  -  b,     a  +  v+w,     a  -  v; 
then,  putting  a  =  b  =  0,  we  have 

n-v-  A,  Pi)*(u  +  v  +  w  ;  A,  P<) 

(v  +  w;  A,  P,); 

herein  put  w  =  nPi,  v  =  u  +  £LPn,  where  P,,  P2  are  two  of  the  characteristics 
belonging  to  the  basis  Plt  ...,  Pp  of  the  group  (P)  ;  then  we  obtain 

/PP 


l)r<iJM»<tii  4,  Pf)*(«;  ^,  P,,  PW*;  ^^2>  A-)^(«;  A,  plt  p.,  PA 

t   / 

Now  every  characteristic  of  the  group  (P)  can  be  given  in  one  of  the  forms 
Qg,  Q*Pi,  QsPz,  Q«PiP2,  where  Qs  becomes  in  turn  all  the  characteristics  of 
a  group  (Q)  of  2^~2  characteristics  ;  putting 


we  immediately  find 

*  («  ;  Q.)  =  *  («  ;  Q.,  P,)  =  *(*;&.  A)  =  ^  (*«  ;  Q-,  A,  P9)  ; 

hence  the  equation  just  obtained  can  be  written 


u 


where  Rm  has  the  four  values  0,  P,,  P,,,  P,  +  P.,. 
Again,  if  in  the  formula  (§  309) 


33—2 


516  COROLLARIES.  [311 

we  add  to  u  the  half  period  Op  ,  we  obtain,  after  putting  u  =  v,  a  =  b  =  0,  the 
result 


,0;  A,e)' 
where 


By  substitution  of  the  value  of  ^  (2u  ;  A,  Pk)  given  by  this  formula,  in 
the  formula  above,  there  results  the  biquadratic  relation*  connecting  the 
functions  ^  ('ii  ;  A  PI). 

(8)  As  an  indication  of  another  set  of  formulae,  which  are  interesting  as 
direct  generalizations  of  the  formulae  for  the  elliptic  function  $(u),  the 
following  may  also  be  given.  Let 

a  a 

o  —  A,j  ~       r  •  •  •  ~r  A^  ,5      , 

dvl  r  ovp 

where  \,  ...,\p  are  undetermined  quantities,  SS-  (v)  =  &  (v*),  8*$  (v)  =  W  (v), 
and  let 


+W(v;  A)- 

then,  differentiating  the  formula 

(u,  b;  A,  e)  3>  (a,  v  ;  A,  e) 
' 


twice  in  regard  to  v,  and  afterwards  putting  v  =  0  and  b  =  0,  we  obtain 


wherein 


(*j  APk) 


the  2^  quantities  Ct  being  independent  of  M  and  of  a.  By  this  formula  the 
function  %>(u',  A)  is  expressed  linearly  by  the  squares  of  2P  theta  quotients 
(cf.  Chap.  XI.  §  217). 

*  Frobenius,  Crelle,  LXXXIX.  (1880),  p.  204.  The  general  Gopel  biquadratic  relation  has  also 
been  obtained  algebraically  (for  Riemann  theta  functions)  by  Brioschi,  Annal.  d.  Mat.,  2a  Ser. , 
t.  x.  (1880—1882). 


312]         SECOND  APPLICATION  OF  THE  GENERAL  THEOREM.         517 

312.  These  propositions  (§§  309 — 311)  are  corollaries  from  the  fact  that 
the  functions  Q(u,  a;  A,  e)  are  linearly  expressible  by  2*'~r  of  them;  we 
have  considered  the  case  r=pa,t  great  length,  on  account  of  its  importance. 

Passing  now  to  the  case  r  =  p  —  1,  there  is  a  linear  relation  connecting 
any  three  of  the  functions 

<f> (u,  a ;  A,  e)  =  2S    (Pf]  ei* (u  +  a-  AP{) *(u-a;  APt). 

i  =  l     \-™- / 

There  is  one  case  in  which  we  can  immediately  determine  the  coefficients  in 
this  relation ;  we  have  <r  =  p  -r=l,  22(T  =  4 ;  there  are  thus  four  character 
istics  A,  whereof  three  are  even  and  one  odd,  which  are  such  that  all  the 
2P-1  characteristics  (AP)  are  of  the  same  character.  Taking  the  single  case 
in  which  these  are  all  odd,  we  have 

4>(M,  a;  A,  e)  =  -<£(«,  u;  A,  e),     and     $>  (a,  a;  A,  e)  =  0; 
hence,  if,  in  the  existing  relation 

X4>  (u,  a;  A,e)  +  n$>(u,b;  A,  e)  +  i/<X>  (u,  c;  A,e)  =  0, 
wherein  X,,  p,  v  are  independent  of  u,  we  put  u  =  a,  we  infer 

yu  :  v  =  <5>  (c,  a  ;  A,  e)  :  <b  (a,  b  ;  A,  e)  ; 
thus  the  relation  is 

,  c-  A,€)®(u,a;  A,  e)  +  3>  (c,  a ;  A,€)®(u,b;  A,  e) 

+  4>  (a,  6;  A,  e)  <!>(«,  c;  A,e)  =  0, 


or 


2P-1 
V 


where 


-c-,  AP}) 
-a;  AP,) 


Adding  together  all  the  equations  thus  obtainable,  by  taking  all  the 
possible  sets  of  values  for  the  fourth  roots  of  unity  ely  ...,  ep-lt  we  obtain 


For  instance,  when  />  =  !,  this  is  the  so-called  equation  of  three  terms,  from  which  all 
relations  connecting  the  elliptic  functions  can  be  derived.  When  p  =  2,  it  is  an  equation 
of  six  terms  and  there  are  fifteen  such  equations,  all  expressed  by 

'•;A)$(b-c',A) 


A  and  B  being  any  two  odd  characteristics*. 

*  Cf.  Frobenius,  Crelle,  xcvi.  (1884),  p.  107. 


518  THIRD    APPLICATION    OF   THE    GENEKAL   THEOREM.  [313 

313.  Taking  next  the  case  r=p  —  2,  every  22  +  1,  or  5,  functions 
<£>  (w,  a;  .4,  e)  are  connected  by  a  linear  relation.  In  this  case  there  are 
sixteen  characteristics  A  such  that  all  the  2p~2  characteristics  (AP)  are  of 
the  same  character,  six  of  them  being  odd.  Denoting  the  six  odd  character 
istics  in  any  order  by  A1}  ...,  As,  and  an  even  characteristic  by  A,  there  is  an 
equation  of  the  form 

\^  (u,  a;  Alte)  +  X23>  (u,  a  ;  A2,  e)  +  \3<&  (u,  a;  A3,  e) 

=  4>  (u,  a  ;  J.4,  e)  +  X3>  (w,  a  ;  A,  e)  ; 

putting  herein  u  =  a,  this  equation  reduces  to  \<I>(a,  a;  J.,  e)  =  0,  so  that 
A,  =  0.  The  other  coefficients  can  also  be  determined  ;  for,  if  C  =  A2A3,  we 
have  (§  306,  Ex.  i.), 

4>  (M  +  flc,  a  ;  A,  e)  =  e*(«-.  O  (^a/3)  <X>  (ti,  a  ;  44.A,,  e)  ; 


putting  therefore  for  u,  in  the  equation  above,  the  value  a  +  Hc,  where 
C=  A2A3,  and  recalling  (§  303)  that  A^A^As,  A4A2A3  are  even  characteristics, 
we  infer 


X,  *   <S>  (a,  a  •  A,A2AS,  e)  =       **   4>  (a,  a  ;  A,A,A3,  e). 


Proceeding  similarly  with  the  characteristics  A3Alf  AjA2  in  turn,  instead  of 
A2A3,  we  finally  obtain 


3>  (a,  a  ;  AtAM  <$>  (u,  a-  A,)  +      •*   3>  (a,  a  ;  A4A3A,)  &  (u,  a  ;  A,) 

\-d.2-^4' 

>  (a,  a;  A.A.A,)  $>  (u,  a  ;.  A3)  =  $>(a,a;  A.A^A,)  <&  (u,  a  ;  At), 


where,  for  greater  brevity,  the  e  is  omitted  in  the  sign  of  the  function  3> 
(cf.  Ex.  viii.,  §  289). 

Ex.     For  p  =  2,  deduce  the  result 
*MSM  (2-t;)  502  (u  +  v)  \,  (u-v)-  403303  (2  v)  $u  (u  +  v)9M(u-v)  +  523^23  (Zv)^(u+  v}  S0i  (u-v) 


where  ^34  =  ^34(0),  etc.     When  v  =  Q  this  is  an  equation  connecting  the  squares  of  302(«), 

3-24  (tt),  ^04  (»),  ^1  («)- 

314.  The  results  of  §§  309,  310  are  capable  of  a  generalization,  obtainable  by  a  repeti 
tion  of  the  argument  there  employed. 

A  group  of  2fc  pairwise  syzygetic  characteristics  may  be  considered  as  arising  by  the 
composition  of  two  such  groups.  Take  k,  =  r  +  s,  characteristics  Ply  ...,  Pr,  Qi,  •••>  Qs, 
every  two  of  which  are  syzygetic  ;  form  the  groups 

(P)  =  0,  /j,  ...,  Pr,  PI"Z,  '•',  «j«»*n  ••• 


respectively  of  2>-  and  2s  characteristics  ;  the  2>-  +  8  combinations  Riyj  =  PiQj  form  a  group 
(/£)  of  2r  +  *  pairwise  syzygetic  characteristics;  for  distinctness  the  fourth  roots  of  unity 


314]  DEDUCTION   OF   A    FURTHER   RESULT.  519 

associated  respectively  with  1\,  ...,  Pr,  Qlt  ...,  Qt,  may  be  denoted  by  *j,  ...,  fr,  f,,  ...,  („  ; 
then  with  /W,  Qj,jlt  Ri,j  will  be  associated  the  respective  quantities 

(Pi\  ,,   (Qt\      „ 

«<.<,  =  «««,  (pj  ,    &,*  =  &<*  (QJ  ,    ««-« 

thus  if  J  be  any  characteristic 


-  .  . 

A    "\  A     «  Q,  -    ;   •        * 

Therefore,  using  the  symbol  ¥  for  a  sum  extending  to  the  whole  group  (PQ\ 


*  (u,  a  ;  A,  E)=  2        '     E{  f  $  (u  +  a  ;  AR^)  3(u-a;  ARU] 

;  AQJPi)9(u-a;  AQ.P,) 


where  *  denotes  a  sum  extending  to  the  2r  terms  corresponding  to  the  characteristics  of 
the  group  (7*). 

By  the  theorem  of  §  307  the  functions  obtainable  from  *•  (?*,  a  ;  A,  E)  by  taking 
different  values  of  a  and  A,  and  the  same  group  (PQ),  are  linearly  expressible  by 
2P-r-«=2<r-«  Of  them,  if  v=p  —  r,  with  coefficients  independent  of  u.  The  2s  functions 
*  (u,  a  ;  AQjy  e),  obtained  by  varying  a  and  Qit  are  themselves  expressible  by  2°"  of  them. 

Thus,  taking  r+s=p,  or  s  =  cr,  we  have 

*  (M,  w  ;  J,  J£)  *  (a,  6  ;  ^1,  ^)  =*  (u,  b  ;  4,  #)  V  (a,  v;  A,  E) 
or 

.2  (^ 

=  s 

taking  for  £\,  ...,  f,  all  the  possible  2*  values,  and  adding  the  2*  equations  of  this  form, 
we  obtain 

2e"lfcl*(M,  v;  4Q,,f)*(a,6;  4^,  «)=2  «H|*'#(%6j  .!§>,  e)  *  (a,  »  ;  4&,  e). 

J=i  j=i 

Suppose  now  that  A1,...,A^  are  the  2217  characteristics  satisfying  the  r  relations 
|  X,  Pi  |  =  |  PJ  |,  (mod.  2),  and  let  (7m=^1^4m  ;  then  |  Cm)  Pi  |  =  0  ;  hence,  by  the  formulae  of 
§  306,  Ex.  i.,  adding  the  half  period  QCm  to  u  and  6,  and  dividing  by  the  factor  e77*1*7""  Al, 
we  have 


taking,  here,  all  the  22<r  values  of  (7m  in  turn,  and  adding  the  equations,  noticing  that 


is  zero  because  Qj  is  not  a  characteristic  of  the  group  (/'),  except  for  the  special  value 
Qj=0,  when  its  value  is  22<r  (§  300),  we  derive  the  formula 

2*r  *  (M,  i  ;  J,  0  *  («,  »  ;  '1,0=2     S  c'f  ic»«°>  '  «  (M,  v  ;  .IC',,,^,  f)  *  («,  b  ;  .K',,,^,  e)  ; 

J-=l  m=l 


520  DEDUCTION    OF    A    FURTHER   RESULT.  [314 

now,  as  already  remarked  (§  298,  Ex.),  if  a  characteristic  S  which  is  syzygetic  with 
every  characteristic  of  the  group  (P)  be  added  to  each  of  the  22<7  characteristics  Alt  ...,  Ak 
the  result  is  another  set  of  22a  characteristics  satisfying  the  same  congruences,  |  X,  I\  =  \  1\\  , 
as  the  set  A1}  ...,  A^,  and  incongruent  mod.  (P)  ;  thus,  taking  a  fixed  value  of  j,  we  have 
CmQj=CnPi,  where,  as  C,n  takes  its  22<T  values,  Cn  also  takes  the  same  values  in  another 
order,  and  Pi  varies  with  m.  Hence  (Ex.  iii.  §  306)  we  have 

^KW  *(w,t,;  ACmQJt  e)*  (0,6;  ACmQj,  f)  =  enilc*pi  l  *  (u,  v-  ACnPiti)  *  (a,  b;  ACnPit  «), 

=  e^c«<*(u,v;  ACn,()*(a,b;  ACn,t), 
and 


and  therefore,  finally,  dividing  by  a  factor  2'  (there  being  2<r  characteristics  in  ($)),  we 
have 

2'2<T 

2**  (w,6;  A,  «)*(«,  v;  ^,0=  2  e*1^*  '*(*,«;  4J^m,  e)*(a,  6;  ^J^m,  e). 

m=l 

When   0-=^,   this    becomes    the  formula  of    §   309.     We  infer   that  the  functions 
<J>(M,  a;  -4,  e)   are  connected   by  the    same    relations    as    the    functions    of   the    form 
;  A)  3  (u-a;  A]  when  the  number  of  variables  (in  the  latter  functions)  is  <r. 

Ex.     Prove  that,  with  the  notation  of  the  text, 


f  *(a,b;A,E) 

315.     The  formula  of  the  last  Article  is  capable  of  a  further  generalization.    Let  (R)  be 
a  group  of  2^  characteristics,  formed  with  Jtlt  ...,  R^  as  basis,  which  satisfy  the  conditions 

R    P     =0  /f    P   \  =  0 

Jt,    1  j     —  V,    .  . .  ,       ./»,,    1  ,.  |  —  U. 

Thus  (P)  is  a  sub-group  of  (R)  ;  the  group  (If)  consists  of  (P),  together  with  groups  (RP), 
whereof  the  characteristics  R  form  a  group  of  2*~r  characteristics,  whose  constituents  are 
incongruent  for  the  modulus  (P).  The  basis  of  this  sub-group  of  2^~J'  characteristics  will 
be  denoted  by  R1,  ...,  R,j._r.  The  total  number  of  characteristics  satisfying  the  prescribed 
conditions  is  22p~r;  thus  p^2p  —  r,  and,  when  /z<2jo-r  the  given  conditions  are  not 
enough  to  ensure  that  a  characteristic  belongs  to  the  group  (R). 

Then,  if  F,  G  be  arbitrary  characteristics,  and  Rt  become  in  turn  all  the  characteristics 
of  a  group  of  2A*~r  characteristics  of  the  group  (R)  which  are  incongruent  mod.  (P),  we 

have 

I 
*  («,  6;  GF&i,  t)  *  (a,  v ;  GRt,  e) 

SJM-r 


where  (7m  =  A^Am.  Since  |  ^,  P  =0,  the  constituents  of  the  set  RiCm,  where  /?» is  a  fixed 
characteristic  and  m=l,  2,  ...,  22(T,  are  in  some  order  congruent  (mod.  (P))  to  the  con 
stituents  of  the  set  Cm ;  hence  (§  306,  Ex.  iii.)  the  series  is  equal  to 

M,  v ;  6'<7m,  e)  *  (a,  b ;  (70^,  c), 

*ilj  $  (M)  v;  (yc^,  e)  *  (a,  6;  (?(7m,  e) ; 


316]  A   GENERAL   ADDITION    FORMULA.  521 

<jy-r 

now   2   enl     '    *    is  zero,  \mless  \L,  lii\=0  (mod.  2)  for  every  characteristic  Ii^  in  which 

i=l 

case  its  value  is  2'4~r ;  thus  the  series  is  equal  to 


where  Sm  satisfies  the  conditions  involved  in  |  Sm,  Rf  =0,  FGCm=Smj  namely  the  con 
ditions 

\Sm,  R,  =0,  ...,  \Sm,  ^_r|sO,    FGSm,  Pl  =0,  ...,  \FGSm,  Pr\  =  0 ', 

the  number  of  characteristics  satisfying  these  /*  conditions  is  22^~^;  the  number  of  these 
which  are  incongruent  for  the  modulus  (P)  is  22P~'*~r=22o'+r~''i. 

Suppose  now  that  \FG,  Pj  =0,  ...,  |  FG,  Pr  |  =  0 ;  then  the  characteristics  Sm  con 
stitute  a  group  satisfying  the  conditions  |  Sm,  R  =0,  where  R  becomes  in  turn  all  the  2^ 
characteristics  of  the  group  (R).  The  group  (S)  of  the  characteristics  Sm  may  be  obtained 
by  combining  the  characteristics  of  the  group  (P)  with  the  characteristics  of  a  group  of 
2  f-f.  r  characteristics  which  also  satisfy  these  conditions  and  are  incongruent  for  the 
modulus  (P) ;  putting  fj.  =  r  +  p,  we  have  therefore* 

•i,  0 

»'*(«,*;  FSm,t)*(a,b;  FSm,  e). 

In  this  equation  each  of  Rit  Sm  represents  the  characteristics,  respectively  of  the 
groups  (R),  (S),  which  are  incongruent  mod.  (P).  But  it  is  easy  to  see  (§  306,  Ex.  iii.) 
that  we  may  also  regard  Rt,  Sm  as  becoming  equal  to  all  the  characteristics,  respectively, 
of  the  groups  (R),  (S}. 

316.  We  have  shewn  in  Chap.  XV.  (§  286,  Ex.  i.)  that  a  certain  addition 
formula  can  be  obtained  for  the  cases  p=  1,  2,  3  by  the  application  of  one 
rule.  We  give  now  a  generalization  of  that  rule,  which  furnishes  results  for 
any  value  of  p. 

Suppose  that  among  the  22<r  characteristics  Alt  A2,  ...,  A^  which,  for  any 
Gopel  system  (P)  of  2r  characteristics,  satisfy  the  conditions 


we  have  k  +  1  =  2-+  1  characteristics  B,,  ...,Bk,  B,  of  which  B  is  even,  which 
are  such  that,  when  i  is  not  equal  to  j,  BBiBj  is  an  odd  characteristic ;  as 
follows  from  §  302  of  this  chapter,  and  §  286,  Ex.  i.,  Chap.  XV.,  this  is 
certainly  possible  when  o-  =  1,  or  2,  or  3  ;  and,  since 

\BBiBj,P\=   B,P\  +  \Bi,P  +   ^,Pj  =  |P|, 

*  The  formula  is  given  by  Frobenius,  Crelle,  xcvi.  p.  95,  being  there  obtained  from  the 
formula  of  §  310,  which  is  a  particular  case  of  it.  The  formula  is  generalised  by  Brauninuhl  to 
tlieta  functions  whose  characteristics  are  n-th  parts  of  integers  in  Math.  Annal.  xxxvn.  (1890), 
p.  98.  The  formula  includes  previous  formulae  of  this  chapter. 


522  A    GENERAL   ADDITION    FORMULA.  [316 


the  characteristics  BBiBj  will  be  among  the  set  A1}  ...,  A^,  so  that  all 
characteristics  congruent  to  BBiBj  (mod.  (P))  are  also  odd.  Then  by  §  307 
there  exists  an  equation  of  the  form* 


k 

,  c;  B,e)  =  2  \m$>(u,  a;  Bm,  e), 

m=l 


wherein  the  coefficients  \,  \lt  ...,  \k,  are  independent  of  u.     Put  in  this 
equation  u  =  a  +  O,BB.  ;  then  we  infer  (§  306,  Ex.  i.) 

X<J>  (a,  c  ;  BI,  e)  =  X;<£  (a,  a  ;  -B,  e)  ; 


hence  we  have 

k 

$>(a,a;  B,  e)  3>  (M,  c  ;  B,  e)  =   2   e^\^Bm\  <|>  (a>  c  -  sm,  e)  <l>  (M,  a  ;  Bm,  e), 

m=l 

which  is  the  formula  in  question  f. 

Adding  the  2r  equations  obtainable   from   this  formula   by  taking    the 
different  sets  of  values  for  the  fourth  roots  of  unity  els  ...,  er,  there  results 

2  e-f  I  ^  l^-o  (#?<)=   2    2  e-l 

i=l  m=l  i=l 

where 


=  *  (0  ;  BPi)  *  (2o  ;  &P<)  ^  (u  +  c  ;  JBP*)  ^  (u  -  c  ; 
=  *  (a  +  c  ;  BJPi)  *  (a  -  c  ;  5^)  ^  (u  +  a  ;  5w 
Herein  we  may  replace  the  arguments 

2a,     u  +  c,     u  —  c,     a  +  c,     a  —  c,     u  +  a,     u  —  a 
respectively  by 
U,  V,  W,  i(U+  V-  W\  ±(U-  V+  W),  ±(U+  V+  W),  i(-  U+  V+  W), 

and  thence,  in  case  p  =  2,  or  p  =  3,  obtain  the  formula  of  Ex.  xi.,  §  286, 
Chap.  XV. 

Or  we  may  put  a  —  0,  and  so  obtain 

2r 

2e«lpil^(0;  BPi)*(u  +  c;  BPi)*(u-c;  BP{} 
1=1 

=    £     |    e«i\Bm,BPi\^(u.    ^p.)^^.    Bmp.}. 
m=\  i=\ 

Other  developments  are  clearly  possible,  as  in  §  286,  Chap.  XV. 

Ex.  When  ar=l  there  are  three  even  Gopel  systems,  and  one  odd;  let  (BP\  (B^P), 
(B2P)  be  the  three  even  Gopel  systems;  then  we  have 

*  (a,  a  ;  B,  c)  *  (u,  c;  B,  e) 

=  e*i|M''*(a,  c;  B,,  «)  *  (a,  a;  Blt  f}  +  eni\BB*\  *  (a,  c;  52,  c)  *  (M,  a;  £2,  e), 

*  We  may,  if  we  wish,  take,  instead  of  the  characteristic  B  on  the  left  hand,  any  characteristic 
A  such  that  |  A,  Pf  \  =  \  P(  |  ,  (i  =  1,  ...  ,  2''). 

t  For  similar  results,  cf.  Frobenius,  Crelle,  LXXXIX.  (1880),  pp.  219,  220,  and  Noether,  Math. 
Annal.  xvi.  (1880),  p.  327. 


317]  EXAMPLES.  523 

where  *  («,  a ;  B,  t)  consists  of  2""1  terms ;  for  instance  when  p=  1  we  obtain 
3(0;  B)3(2a;  B)3(u  +  c;  B)9(u-e;  B) 

r,  Bl)3(a-c;  Bl)9(u  +  a;  B1)3(u-a;  Bj) 
B2)3(u-a;  B2). 


317.     Ex.   i.     If   P    be    a    fixed    characteristic    and  <1f(u;  A)  denote   the  function 
3(u;  A)3(u;  A  +  P),  prove  that 


>ty(ii-    A\ 
-  .  *  \  «•  >  -" ;, 

and 


'•,  B+Q). 

Hence,  if  B^  ...,  Bk,  Bbe  ^  +  1=2P-1  +  1  characteristics  each  satisfying  the  condition 
I  JT,  P\=  |  P\,  such  that,  when  i  is  not  equal  to  j,  BB^B,  is  odd,  we  have  (§  307)  an 
equation 

2P-1 
A¥(«;  .4)=    2  \mV(u;  Bm), 

where  ^1  is  any  other  even  characteristic  such  that  |  A,  P\  =  \  P  | ;  putting  u  =  QB  +  a#.,  we 
obtain 


therefore 


fia-.  ii.  Obtain  applications  of  the  formula  of  Ex.  i.  when  p  =  2,  3,  4;  'in  these  cases 
"•»  =P-1>  =1»  2>  3  respectively,  so  that  we  know  how  to  choose  the  characteristics 
B11...tBk,B  (Ex.  i.,  §  286,  Chap.  XV.,  and  §  302  of  this  Chap.). 

Ex.  iii.     From  the  formula  (§  309) 
5(M  +  6;  A)3(u-b;  A)$(a  +  v;  A)3(a-v;  A) 

=  -2e*i\AR\9(u  +  v,  R)B(u-v;  R)9(a  +  b;  Ji)S(a-b;  R), 
by  putting  a  +  QP  for  a,  and  b  =  v=0,  we  deduce 

52  (tt;  A)  3*  (a;  JP)  =  2^2  e^1^'  f  /'  }  3*  (u-  R)9*(a-,  PR), 
it  \aLK/ 

where  A,  I1  are  any  half-integer  characteristics  and  R  becomes  all  the  22"  half-integer 
characteristics  in  turn  ;  putting  RP  for  R  we  also  have,  from  this  equation, 


;  If); 
therefore 

;  AP) 


The  values  of  R  may  be  divided  into  two  sets,  according  as  \R,P\  +  \P\  =  l  (mod.  2), 
or  =0;  for  the  values  of  the  former  set  the  corresponding  terms  vanish;  the  values  of  R 
for  which  \R,P\  +  \P\  =  Q  (mod.  2)  may  be  either  odd  or  even;  for  the  odd  values  the 
zero  values  of  the  corresponding  theta  functions  are  zero  ;  there  remain  then  (§  299)  only 
2.  2"  -2(2"-'  +  1)  terms  on  the  right  hand  corresponding  to  values  of  R  which  satisfy  the 


524  EXAMPLES.  [317 

conditions  |  R  \  =  \  RP  \  =  0   (mod.    2)  ;    these  values  are  divisible  into  pairs  denoted  by 
R  =  E,  R  =  EP;  for  such  values  \  +  e^R'  p  l+"lpl  =  2,  and 


i\AE\(  f\,eni\AEP\(    1"    \ 

\AE)+          \AEP) 


,*i\AE\  (  P  \  r-i.jd\AB,P\-in\AJB\(  P      r,   ,    ri\A, 

=<          AE  L 


P\  r,   ,    ri\ 

AE)  L 

thiis,  provided  |  A,  P  \  +  1  P  \  =  0  (mod.  2), 

(;  EP),  (i), 


wherein  32(;  -4)  denotes  32(0;  J),  etc.,  and,  on  the  right  hand  there  are  2"~2  (2P~ 
terms  corresponding  to  values  of  E  for  which  |  E\  =  \  EP  |  =  0  (mod.  2),  only  one  of  the  two 
values,  E,  EP,  satisfying  these  conditions  being  taken. 

Putting  P=0,  u  =  a,  in  the  second  equation  of  this  example,  we  deduce  in  order 

S*(M;  A)  =  Z-^e'^AR^*(u',  R);  3*(u;  AP}  =  Z~^e^APR\  &  (u;  R); 

R  R 

so  that,  by  addition, 

$*(u;  A)  +  eiri\A'Pl3i(u;  ^P)=2-"S«"<l^Jl|[H-eir*|p|+iri|Ji"p|]5*(«;  R); 

R 

thus,  as  before, 

;  EP)},     (ii). 


Ex.  iv.  Taking  p  =  2,  let  (P)  =  0,  Px,  P2,  P^P-,,  be  a  Gopel  group  of  even  charac 
teristics*;  let  Bl,  S2,  B^BI  be  such  characteristics  (§  297)  that  the  Gopel  systems 
(P),  (B1P\  (BZP},  (J31B2f}  constitute  all  the  sixteen  characteristics;  each  of  the  systems 
(B^P),  (B2P),  (BlBi>P)  contains  two  odd  characteristics  and  two  even  characteristics. 
Then,  in  the  formulae  (i),  (ii)  of  Ex.  iii.,  if  P  denote  any  one  of  the  three  characteristics 
P15  P2J  PlP2t  the  conditions  for  the  characteristics  E  are  E,  P\=  P|  =  0,  1^1  =  0;  the 
2.  2^~2(2p~1  +  l),  =6,  solutions  of  these  conditions  must  consist  of  0,  Q,  B  and  P,  QP,  BP, 
where  Q  is  defined  by  the  condition  that  the  characteristics  0,  Q,  P,  QP  constitute  the 
group  (P),  and  B  is  a  certain  even  characteristic  chosen  from  one  of  the  systems  (Bl  P), 
(B2P),  (B1B2P).  Hence,  when  P=Pi,  we  may,  without  loss  of  generality,  take  for  the 
2P-2  (2p~1  +  l)  =  3  values  of  E  which  give  rise  to  different  terms  in  the  series  (i),  (ii),  the 
values  0,  P2,  Bl;  similarly,  when  P=P2>  we  have,  for  the  values  of  E,  E=0,  P1?  B2;  and 
when  P=P1P2,  E=0,  P15  B^;  taking  A  to  be  respectively  t  Bly  B2,  B^  in  these 
cases,  we  obtain  the  six  equations 


*  There  are  six  such  groups  (Ex.  iv.  §  289). 

f  We  easily  find   |  BlB%Pl  \  =  \  B^P*  =  -  |  BJt*  j  .     Thus   the   case   when  B^  is  odd  is 
included  by  writing  B1P1  in  place  of  2ix. 


317]  EXAMPLES.  525 


wherein  ^.^i»/  _  _  i.     These  formulae  express  the  zero  values  of 

all  the  even  theta  functions  in  terms  of  the  four£(;  0),  B(;  PJ,  $(;  Pz),  3(;  P^P^. 
Thus  for  instance  they  can  be  expressed  in  terms  of  ^5,^34,  S12,  $0;  the  equations  have 
been  given  in  Ex.  iii.,  §  289,  Chap.  XV. 

Ex.  v.     We  have  in  Chap.  XVI.  (§291)  obtained  the  formula 
S(u-v, 


where  t  represents  a  set  of  p  integers,  each  either  0  or  1,  and  has  therefore  2»  values. 

Suppose  now  that  q,  r  represent  the  same  half-integer  characteristic,  =i(     )  +|  (  /.   )  , 

\c  /         Vp«/ 
=  C+Ka,  say;  then  we  immediately  find 

*.[«'  *^£+o>[-'  *«3J#KT'  t'  y  •[-  *r|. 

where  t'c'  denotes  the  row  of  p  integers,  each  either  0  or  1,  which  are  given  by  (c'<f)i  =  fj+cj 
(mod.  2);  herein  the  factor  e"wc'  S^    •»  is  independent  of  ka.     For  Ka  we  take  now,  in 

turn,  the  constituents 

0,  Klt  A2,  ...,  Kp,  KlK.i,  ...,  K^K^K^  ... 

of  a  Go  pel  set  of  2p  characteristics,  in  which 

0,0,0,  ...\  1/0,0,0,..A  /O,  ...,0,0\ 

= 


then  denoting  $[u  +  v;  CKJ  $[u-v;  CKa]  by  [CKa],  we  obtain  2»  equations  which  are  all 
included  in  the  equation 


wherein  *=2P,  e/,  ...,  es'  represent  the  different  values  of  «',  and  ,/  is  a  matrix  wherein  the 
/3-th  element  of  the  a-th  row  is  ^  \u  ;  -f&C  \. 

The  2p  various  values  of  c'^c',  for  an  assigned  value  of  c',  are,  in  general  in  a  different 
order,  the  same  as  the  various  values  of  t'o  ;  we  may  suppose  the  order  of  the  columns  of 
t7  to  be  so  altered  that  the  various  values  of  e'^c'  become  the  values  of  e'«  in  an  assigned 

order,  the  order  of  the  elements  &™c'  ^  \v  ;  5  *  1     ,  .  .  .  ,  «"•'"«'  ^  \v  ;  ^  **     being  correspond 

ingly  altered.  When  this  is  done  the  matrix  J  is  independent  of  the  characteristic  C. 
Now  it  is  possible  to  choose  2"  characteristics  (7,  say  Clt  ...,  Cg  such  that  the  Gopel 
systems  (CtK)  give,  together,  all  the  2"  possible  characteristics  ;  then  the  2?  equations 
obtainable  from  that  just  written  by  replacing  C  in  turn  by  Clt  ...,  C,,  are  all  included, 
using  the  notation  of  matrices,  in  the  one  equation* 


wherein  £'a  denotes  a  row  of  jt?  integers,  each  either  0  or  1,  and  has  2"  values.     In  each 
matrix  the  element  written  down  is  the  ;3-th  element  of  the  a-th  row. 

*  We  can  obviously  obtain  a  more  general  equation  by  taking  22"  different  sets  of  arguments, 
the  general  element  of  the  matrix  on  the  left  hand  being  3-[>(a)  +v^}  ;  CaKfi]$[uw  -v®]  ;  CaKft]. 
Cf.  Chap.  XV.  §  291,  Ex.  v.,  and  Caspary,  Crelle,  xcvi.  (1884),  pp.  182,  324;  Frobenius,  Crelle, 
xcvi.  (1884),  p.  100.  Also  Weierstrass,  Sitzuni/abfi:  der  Ak.  <l.  Wins,  zn  Herlin,  1882,  i.—  xxvi 
p.  500. 


526  EXAMPLES.  [317 

Ex.  vi.     If  in  Ex.  v.,  jo  =  2,  and  the  group  (A')  consists  of  the  characteristics 


oi 


while  the  characteristics  C  consist  of 

/00\      ,  /10\ 

*  (oo) '  2  (oo) ' 

and  the  values  of  f  are,  in  order, 

(0,0),     (0,1),     (1,0),     (1,1), 
shew  that  the  sixteen  equations  expressed  by  the  final  equation  of  Ex.  v.  are  equivalent  to 

=  (       «4,        0.5,    —  a.2,        "i  )  (       ft?    —ft?        ft)        ft) 


oon      rion      ron 
iiJ'    [_ooj'    L10J' 


O 


n 


roii 

'  LHJ 


oi 


oi 


o1 


io 


00 


—  ao ,        a 


o ,        a4 ,        nj ,        a2 


a0,        a,,    —i 


«2>    -°1)        a4)        «3 


Q  C)                     Q  Q 

P-2»  P3'          ft>  "ft 

-ft)  ft)          ft)  ft 

ft)  ft)  "ft)  ft 


wherein,  on  the  left  hand,  denotes  S    u  +  v;  ?[-,-.}    ^    u-v;  |(n  J  L  etc.,  and 

the  right  hand, 

--*.[«!  *Q].  *-«.[»! 


/31?  /32,  ft,  ft  being  respectively  the  same  theta  functions  with  the  argument  v. 

Now  if  A,  B  denote  respectively  the  first  and  second  matrices  on  the  right  hand,  the 
linear  equations 

(#1.  ^2>  #3>    2/4)  =  ^  (#11  -^2>  '^3>  -r4)>    (-^I,  #2.  'r3>  ^4)  =  -B(«;l»  «2>  %»  ^4) 

are  immediately  seen  to  lead  to  the  results 


V+  V+V+  V=(ft2+ft2+ft2+ft2)  (V+^+V+O  ; 

hence  if  the^-th  element  of  the  j'-th  row  of  the  compound  matrix  J.B,  which  is  the  matrix 
on  the  left-hand  side  of  the  equation,  be  denoted  by  y?.  .  ,  we  have 

i1t«"i*l*»i^rn.'"^  (r**'  r'  *=1»  2'  3»  4)' 

and  these  equations  lead  to 

A<*-A*^A^'v^ 

Denoting  ,  ,  by  [a^g]  ,  [a^J  ,  etc.,  as  in  the  table  of  §  204,  and  inter 

changing  the  second  and  third  rows  of  the  matrix  on  the  left-hand  side,  we  may  express 
the  result  by  saying  that  the  matrix 

K^L       KcJi   -|>i<|  ,       [aj 


-[cc,]    ,    -[cc2]    ,    -[0^2],       [0] 
gives  an  orthogonal  linear  substitution  of  four  variables*. 

*  An  algebraic  proof  may  be  given  ;  cf.  Brioschi,  Ann.  d.  Mat.  xiv. 


317]  A   MULTIPLICATION   FORMULA.  527 

Ex.  vii.     Deduce  from  §  309  that 

AP^^(v;  Al>S\ 


—      -  , 

e  ifa  *    (,U  >    OJTf} 

a. 

where  /»<,  Pa  are  characteristics  of  a  Gopel  group  (P\  of  2»  characteristics.  Infer  that,  if 
n  be  any  positive  integer,  and  A  Pi  be  an  even  characteristic,  3(nv;  APj)  is  expressible  as  an 
integral  polynomial  of  order  n2  in  the  W  functions  9(v;  AP  ). 

Ex.  viii.     If  K  =  |  (     )  ,  P.  =  |  (q  a  )  ,  deduce  from  §  309,  putting 

W  \?a/ 

a  =  b  =  u-  U=v—  V=\Qk, 
that 


r,  -F), 
where 


x  (u,  v]  =  2fae~  "'»«  5  («  ;  /r+  P0)  3  (v  ; 


[318 


CHAPTER   XVIII. 

TRANSFORMATION  OF  PERIODS,  ESPECIALLY  LINEAR  TRANSFORMATION. 

318.  IN  the  foregoing  portion*  of  the  present  volume,  the  fundamental 
algebraic  equation  has  been  studied  with  the  help  of  a  Riemann  surface. 
Much  of  the  definiteness  of  the  theory  depends  upon  the  adoption  of  a 
specific  mode  of  dissecting  the  surface  by  means  of  period  loops ;  for  instance 
this  is  the  case  for  the  normal  integrals,  and  their  periods,  and  consequently 
also  for  the  theta  functions,  which  were  defined  in  terms  of  the  periods 
Tij  of  the  normal  integrals  of  the  first  kind;  it  is  also  the  case  for  the 
places  ml,...,mp  of  §  179  (Chap.  X.),  upon  which  the  theory  of  the 
vanishing  of  the  theta  functions  depends.  The  question  then  arises ;  if  we 
adopt  a  different  set  of  period  loops  as  fundamental,  how  is  the  theory 
modified,  and,  in  particular,  what  is  the  relation  between  the  new  theta 
functions  obtained,  and  the  original  functions  ?  We  have  given  a  geometrical 
method  (§  183,  Chap.  X.)  of  determining  the  places  ml,  ...,mp  from  the 
place  m,  from  which  it  appears  that  they  cannot  have  more  than  a  finite 
number  of  positions  when  m  is  given,  and  coresidual  places  are  reckoned 
equivalent;  the  enquiry  then  suggests  itself;  can  they  take  all  these  possible 
positions  by  a  suitable  choice  of  period  loops,  or  is  one  of  these  essentially 
different  from  the  others  ?  The  answers  to  such  questions  as  these  are  to  be 
sought  from  the  theory  of  the  present  chapter. 

There  is  another  enquiry,  not  directly  related  to  the  Riemann  surface, 
but  arising  in  connexion  with  the  analytical  theory  of  the  theta  functions. 
Taking  p  independent  variables  ul}  ...,  itp,  and  associating  with  them,  in 
accordance  with  the  suggestion  of  §§  138 — 140  (cf.  §  284),  the  matrices 
2&),  2&/,  2rj,  2?/,  we  are  thence  able,  with  the  help  of  the  resulting  equations 

2//W  =  TTI,    2ha>'  =  6,    i)  =  2a&>,    rf  =  2aa>'  —  h, 

to  formulate  a  theta  function.  But  it  is  manifest  that  this  procedure  makes 
an  unsymmetrical  use  of  the  columns  of  periods  arising  respectively  from 
the  matrices  co  and  o>' ;  and  it  becomes  a  problem  to  enquire  whether  this 

*  References  to  the  literature  dealing  with  transformation  are  given  at  the  beginning  of 
Chap.  XX. 


319]  THE  GENERAL  SYSTEM  OF  PERIOD  LOOPS.  529 

want  of  symmetry  can  be  removed ;  and  more  generally  to  enquire  what 
general  linear  functions  of  the  original  2p  columns  of  periods,  with  integral 
coefficients,  can  be  formed  to  replace  the  original  columns  of  periods;  and,  if 
theta  functions  be  formed  with  the  new  periods,  as  with  the  original  ones, 
to  investigate  the  expression  of  the  new  theta  functions  in  terms  of  the 
original  ones. 

So  far  as  the  theta  functions  are  concerned,  it  will  appear  that  the 
theory  of  the  transformation  of  periods,  and  of  characteristics,  includes  the 
consideration  of  the  effect  of  a  modification  of  the  period  loops  of  a  Riemann 
surface ;  for  that  reason  we  give  in  this  chapter  the  fundamental  equations 
for  the  transformation  of  the  periods  and  characteristic  of  a  theta  function, 
when  the  coefficients  of  transformation  are  integers ;  but  the  main  object 
of  this  chapter  is  to  deal  with  the  transformation  of  the  period  loops  on  a 
Riemann  surface.  The  analytical  theory  of  the  expression  of  the  transformed 
theta  functions  in  terms  of  the  original  functions  is  considered  in  the  two 
following  chapters. 

In  virtue  of  the  algebraical  representation  which  is  possible  for  quotients 
of  Riemann  theta  functions  (as  exemplified  in  Chap.  XI.),  the  theory  of 
the  expression  of  the  transformed  theta  functions  in  terms  of  the  original 
functions,  includes  a  theory  of  the  algebraical  transformation  of  the  funda 
mental  algebraical  equation  associated  with  a  Riemann  surface ;  it  is  known 
what  success  was  achieved  by  Jacobi,  from  this  point  of  view,  in  the  case  of 
elliptic  functions ;  and  some  of  the  earliest  contributions  to  the  general 
theory  of  transformation  of  theta  functions  approach  the  matter  from  that 
side*.  We  deal  briefly  with  particular  results  of  this  algebraical  theory  in 
Chap.  XXII. 

319.  Take  any  undissected  Riemann  surface  associated  with  a  funda 
mental  algebraic  equation  of  deficiency  p.  The  most  general  set  of  2p 
period  loops  may  be  constructed  as  follows  : 

Draw  on  the  surface  any  closed  curve  whatever,  not  intersecting  itself, 
which  is  such  that  if  the  surface  were  cut  along  this  curve  it  would  not  be 
divided  into  two  pieces ;  of  the  two  possible  directions  in  which  this  curve 
can  be  described,  choose  either,  and  call  it  the  positive  direction  ;  call  the 
side  of  the  curve  which  is  on  the  left  hand  when  the  curve  is  described 
positively,  the  left  side ;  this  curve  is  the  period  loop  (A^ ;  starting  now 
from  any  point  on  the  left  side  of  (A^,  a  curve  can  be  drawn  on  the  surface, 
which,  without  cutting  itself,  or  the  curve  (A^,  and  without  dividing  the 
surface,  ends  at  the  point  of  the  curve  (AJ  at  which  it  began,  but  on  the 
right  side  of  (AJ ;  this  is  the  loop  (BJ,  and  the  direction  in  which  it  has 

*  See,  in  particular,  Richelot,  Crelle,  xvi.  (1837),  De  transformatione...integralium  Abelian- 
orum  primi  ordinis  ;  in  the  papers  of  Konigsberger,  Crelle,  nx.iv.,  LXV.,  LXVII.,  some  of  the 
algebraical  results  of  Richelot  are  obtained  by  means  of  the  transformation  of  theta  functions. 

B.  34 


530  THE   GENERAL   SYSTEM   OF   PERIOD   LOOPS.  [319 

been  described  is  its  positive  direction  ;  its  left  side  is  that  on  the  left  hand 
in  the  positive  description  of  it.  The  period  associated  with  the  loop  (^i), 
of  any  Abelian  integral,  is  the  constant  whereby  the  value  of  the  integral 
on  the  left  side  of  (Aj)  exceeds  the  value  on  the  right  side,  and  is  equal  to 
the  value  obtained  by  taking  the  integral  along  the  loop  (B^  in  the  negative 
direction,  from  the  end  of  the  loop  (BJ  to  its  beginning.  The  period 
associated  with  the  loop  (BJ  is  similarly  the  excess  of  the  value  of  the 
integral  on  the  left  side  of  the  loop  (B^  over  its  value  on  the  right  side,  and 
may  be  obtained  by  taking  the  integral  round  the  loop  (A^)  in  the  positive 
direction,  from  the  right  side  of  the  loop  (BJ  to  the  left  side.  These  periods 
may  be  denoted  respectively  by  Ox  and  fl/. 

320.  It  is  useful  further  to  remark  that  there  is  no  essential  reason  why  what  we  have 
called  the  loops  (Aj),  (B^j  should  not  be  called  respectively  the  loops  [5J  and  [JJ.  If 
this  be  done,  and  the  positive  direction  of  the  (original)  loop  (Z?t)  be  preserved,  the 
convention  as  to  the  relation  of  the  directions  of  the  loops  [A{\,  [B^\  will  necessitate  a 
reversal  of  the  convention  as  to  the  positive  direction  of  the  (original)  loop  (Aj).  If  the 
periods  associated  with  the  (new)  loops  [A^,  [B^\  be  respectively  denoted  by  [Q]  and  [Q'], 
we  have,  therefore,  the  equations 


These  equations  represent  a  process  —  of  interchange  of  the  loops  (AJ,  (BJ,  with  retention 
of  the  direction  of  (BJ  —  which  may  be  repeated.  The  repetition  gives  equations  which  we 
may  denote  by 

{Q}  =  [O'J  =  -  O,     {&'}  =  -  [Q]  =  -  Q', 

and  the  two  processes  are  together  equivalent  to  reversing  the  direction  of  loop  (Aj)t  and 
(therefore)  of  the  loop  (Bj).  The  convention  that  the  loop  (BJ  shall  begin  from  the  left 
side  of  the  loop  (Aj)  is  not  necessary  for  the  purpose  of  the  dissection  of  the  surface  into  a 
simply  connected  surface  ;  but  it  affords  a  convenient  way  of  specifying  the  necessary 
condition  for  the  convergence  of  the  series  defining  the  theta  functions. 


321.  The  pair  of  loops  (AJ,  (Bj)  being  drawn,  the  successive  pairs 
(A2),  (.B2),  ...,  (Ap),  (Bp)  are  then  to  be  drawn  in  accordance  with  precisely 
similar  conventions  —  the  additional  convention  being  made  that  neither 
loop  of  any  pair  is  to  cross  any  one  of  the  previously  drawn  loops.  If 
the  Riemann  surface  be  cut  along  these  2p  loops  it  will  become  a  p-ply 
connected  surface,  with  p  closed  boundary  curves.  It  may  be  further 
dissected  into  a  simply  connected  surface  by  means  of  (p  —  1)  further  cuts 
((7j),  ...,  (C^-j),  taken  so  as  to  reduce  the  boundary  to  one  continuous  closed 
curve. 

Upon  the  p-p\y  connected  surface  formed  by  cutting  the  original  surface 
along  the  loops  (AJ,  (B^,  ...,  (Ap),  (Bp\  the  Riemann  integrals  of  the  first 
and  second  kind  are  single-  valued.  In  particular  if  Wl}  ...,  Wp  be  a  set  of 
linearly  independent  integrals  of  the  first  kind  defined  by  the  conditions 
that  the  periods  of  Wr  at  the  loops  (A^,  ...,  (Ap)  are  all  zero,  except  that  at 


322]  CHANGE  FROM  ONE  SYSTEM  TO  ANY  OTHER.  531 

(Ar\  which  is  1,  and  if  rr,g  be  the  period  of  Wr  at  the  loop  (Bs\  the  imaginary 
part  of  the  quadratic  form 

Tunj2  +  ......  +  2T12n1n2  +  ......  +  TpflPp 

is  necessarily  positive*  for  real  values  of  n1,  ...,  np.  This  statement  remains 
true  when,  for  each  of  the  p  pairs,  the  loops  (Ar),  (Br)  are  interchanged, 
with  e.g.  the  retention  of  the  direction  of  (Br)  and  a  consequent  change  in  the 
sign  of  the  period  associated  with  (Ar\  as  explained  above  (§  320)  ;  if  the 
loops  (Ar),  (Br)  be  interchanged  without  the  change  in  the  sign  of  the  period 
associated  with  (Ar),  the  imaginary  part  of  the  corresponding  quadratic 
form  is  negative*}-. 

322.  In  addition  now  to  such  a  general  system  of  period  loops  as  has 
been  described,  imagine  another  system  of  loops,  which  for  distinctness  we 
shall  call  the  original  system  ;  the  loops  of  the  original  system  may  be 
denoted  by  (ar),  (br)  and  the  periods  of  any  integral,  ui}  associated  therewith, 
by  2ft>;ir,  2(o'i>r;  the  general  system  of  period  loops  is  denoted  by  (Ar),  (Br), 
and  the  periods  associated  therewith  by  [2^  .,.],  [%w'it  r].  For  the  values  of 
the  integral  ui}  the  circuit  of  the  loop  (Br),  in  the  negative  direction,  from 
the  right  to  the  left  side  of  the  loop  (Af),  is  equivalent  to  a  certain  number, 
sayj  to  a.j>r>  of  circuits  of.  the  loop  (bj)  in  the  negative  direction,  together 
with  a  certain  number,  say  a  'j>  r,  of  circuits  of  the  loop  (a,-)  in  the  positive 
direction  (r,j=I,  2,  .  ..,  p}]  hence  we  have 

p 

[a>it  r]  =  2  (&>;,  j  «/,  r  +  G>\  j*'j,r\  (r  —  1  ,  2,  .  .  .  ,  p  )  ; 

j=i 

similarly  we  have  equations  which  we  write  in  the  form 

K  &  r  +  a>\  jfi'j,  ,),  (r  =  1,  2,  .  .  .  ,  p), 


the  interpretation  of  the  integers  /8j>r,  j3'jjr  being  similar  to  that  of  the 
integers  «,-_,.,  afj>r. 

Thus,  if  uly  ...,up  denote  p  linearly  independent  integrals  of  the  first 
kind,  and  the  matrices  of  their  periods  for  the  original  system  of  period 
loops  be  denoted  by  2&>,  2&>',  and  for  the  general  system  of  period  loops  by 
[2<a],  [2ft)'],  we  have 

[o>]  =  wo.  +  a/a',    [&>']  =  a>/3  +  &//3', 
where  a,  a',  ft,  @'  denote  matrices  whose  elements  are  integers. 

*  And  not  zero,  since  nlWl  +  ...  +  npWp  cannot  be  a  constant.  Cf.  for  instance,  Neumann, 
Riemann's  Theorie  der  AbeVschen  Integrate  (Leipzig,  1884),  p.  247,  or  Forsyth,  Theory  of 
Functions  (1893),  p.  447.  (Riemann,  Werke,  1876,  p.  124.) 

t  As  previously  remarked,  p.  247,  note. 

J  A  circuit  of  (&,•)  in  the  positive  direction  furnishing  a  contribution  of  -  1  to  a,-(,. 

34—2 


532  TRANSFORMATION   OF   PERIOD   LOOPS.  [322 

If  L1}  ...,  Lp  be  a  set  of  p  integrals  of  the  second  kind  associated  with 
ul}  ...,  up,  as  in  §  138,  Chap.  VII.,  and  satisfying,  therefore,  the  condition 


x,  a-.         r>        /          \  a2  t\    \  /          \  ®X 

i    ]  =  Dx  \(z,  x)  T  \-  Dz  \(x,  z)  -r    , 
L         atj          L         acJ 


and  the  period  matrices  of  Llt  ...,  Lp  at  the  original  and  general  period 
loops  be  denoted  respectively  by  -  2rj,  -  2?/  and  -  [2iy],  -  [2^'],  we  have, 
similarly,  for  the  same  values  of  a,  a',  /3,  /3', 

[?;]  =  7/-«  +  7?'a',      [r/]  =  ??/3  +  T//3'. 

We  have  used  the  notation  flp  for  the  row  of  P  quantities  2o>P  +  2&/P', 
where  P,  P'  each  denotes  a  row  of  p  quantities  ;  we  extend  this  notation  to 
the  matrix  2eoa  +  2a/a',  where  a,  a'  each  denotes  a  matrix  of  p  rows  and 
columns,  and  denote  this  matrix  by  Qa  ;  similarly  we  denote  the  matrix 
2r)d  +  2?/a'  by  Ha  ;  then  the  four  equations  just  obtained  may  be  written 
[2»]  =  n.f  [2a/]  =  fV  [27,]  =  #a,  [27/]  =  #0.  (I.) 

Noticing  now  that  the  matrices  [2<o],  [2o>'],  [2?;],  [2?/]  must  satisfy  the 
relations  obtained  in  §  140,  we  have 

iTrt  =  [ifl  [»']  -  [5]  [V]  = 


=  a 

=  (a/3'  -  a'/3)  ^wt, 

in  virtue  of  the  relations  satisfied  by  the  matrices  2<o,  2a/,  2i;,  2?/;  and 
similarly 

0  =  [fj]  [»]  -  [5]  [T/]  =  i  (^aOa  -  HaJffa)  =  (oV  -  a'a)  J^ri, 
and 

0  =  [5H  M  -  [«1  M  =  1  (Hefy  ~  n^)  =  (^/3'  -  /S'/S)  i^ri  ; 

thus  we  have 

off  -30  =  1  =&*-&*',    aa'-a'a  =  0,    /3/S'  -  /S'/3  =  0,          (II.) 

namely,  the  matrices  a,  /S,  of,  /3'  satisfy  relations  precisely  similar  to  those 
respectively  satisfied  by  the  matrices  to,  co',  77,  77  x,  the  ^-m'  which  occurs 
for  the  latter  case  being,  in  the  case  of  the  matrices  a,  /3,  a',  /3',  replaced 
by  —  1  ;  therefore  also,  as  in  §  141,  the  relations  satisfied  by  a,  /3,  a',  /S'  can  be 
given  in  the  form 

a/S'-/Sa/  =  l=/9/a-a//S,   a/S-/Sa=0,   a'/S'  -  /SV  =  0.          (III.) 
In  virtue  of  these  equations,  if 


denote  the  matrix  of  2p  rows  and  columns  formed  with  the  elements  of  the  matrices  a,  £, 

a',  £',  we  have  (cf.,  for  notation,  Appendix  ii.) 

a,/3W     ^',    -j8\       /a|8'-/3a',  /3a-aj8\/10\ 
a',  (87  V  -  5',        a^       \ftjf  -  jS'a',   /3*d  -  *W       \0   V  ' 


323]  TRANSFORMATION   OF   INTEGRALS.  533 

and  therefore 


and  the  original  periods  can  be  expressed  in  terms  of  the  general  periods  in  the  form 
w  =  [w]  /3'  —  [to']  a',     a)'  =  —  [w]  £  +  [to']  a, 


If  0  denote  the  matrix  of  jo  rows  and  columns  whereof  every  element  is  zero,  and 
1  denote  the  matrix  of  p  rows  and  columns  whereof  every  element  is  zero  except  those  in 
the  diagonal,  which  are  all  equal  to  1,  and  if  e  denote  the  matrix  of  2p  rows  and  columns 
given  by 


then  it  is  immediately  proved  that  the  relations  (II.),  (III.)  are  respectively  equivalent  to 
the  two  equations 

where 

•7"     /  o  ,    Q 
«/  =  (  -'    - 

\P>    P 

and  it  will  be  noticed  that  the  equations  (III.)  are  obtained  from  the  equations  (II.)  by 
changing  the  elements  of  J  into  the  corresponding  elements  of  J. 

It  follows*  from  the  equation  JfJ=e  that  the  determinant  of  the  matrix  J  is  equal  to 
+  1  or  to  - 1.     It  will  subsequently  (§  333)  appear  that  the  determinant  is  equal  to  +1. 

Ex.    Verify,  for  the  case  ^=2,  that  the  matrices 

_/     4,    -20\       fl/-29,       124\ 

,     /-3,       20\  /     22,   -124\ 

Q=V-8,     -7>     "=(     56,         43J 
satisfy  the  conditions  (III.)  (Weber,  CreUe,  LXXIV.  (1872),  p.  72). 

323.  It  is  often  convenient,  simultaneously  with  the  change  of  period 
loops  which  has  been  described,  to  make  a  linear  transformation  of  the 
fundamental  integrals  of  the  first  kind,  u^,  ...,up.  Suppose  that  we  intro 
duce,  in  place  of  ult  ...,  up,  other  p  integrals  w1}  ...,  wp,  such  that 


ui  =  Miilwl+ +Mi>pwp, 

or,  as  we  shall  write  it,  u  =  Mw,  M  being  a  matrix  whose  elements  are 
constants  and  of  which  the  determinant  is  not  zero.  We  enquire  then  what 
are  the  integrals  of  the  second  kind  associated  with  w1}  ...,  wp.  We  have 
(§  138)  denoted  Dui  by  /*;(#),  and  the  matrix  of  the  quantities  /*;(<?;)  by  p, ; 

*  For  another  proof  of  the  relations  (II.),  (HI.)  of  the  text,  the  reader  may  compare  Thomae, 
Crelle,  LXXV.  (1873),  p.  224.  A  proof  directly  on  the  lines  followed  here  may  of  course  be 
constructed  with  the  employment  only  of  Riemann's  normal  elementary  integrals  of  the  first 
and  second  kind.  Cf.  §  142. 


534  TRANSFORMATION   OF   PERIODS   AND  [323 

denote  now,  also,  Dwf  a  by  pt  (x),  and  the  matrix  of  the  quantities  pt  (GJ)  by  p  ; 
then  we  immediately  find  //.  =  pM,  and  the  equation  (§  138) 

Lx>  a  =  p-lHx>  a  -  2aux>  a 
gives 

ML*'  a  =  p~lHx'  a  -  2MaMwx>  a  ; 

thus  the  integrals  of  the  second  kind  associated  with  w1}  ...,wp  are  the  p 
integrals  given  by  MLx>a,  and,  corresponding  to  the  matrix  a  for  the 
integrals  L^  ,  ...,  Lp'  ,  we  have,  for  the  integrals  MLx'a,  the  matrix 
a  =  MaM.  If  2u,  2i/  denote  the  matrices  of  the  periods  of  the  integrals  w, 
and  —  2£,  —  2£"  denote  the  matrices  of  the  periods  of  the  integrals  MLx-a,  so 
that  (§  139) 


we  therefore  have  w  =  Mv,  w  =  Mv  and 

£  =  2MaMv  =  Mi),    Z'  =  2MaMv'-±MfJL-^  =  M'r)';  (IV.) 

it  is  immediately  apparent  from  these  equations  that  the  matrices  v,  v,  £  £" 
satisfy  the  equations  of  §  140, 

vv'  -  v'v  =  0,   £?  -  £'  ?  =  0,  v'l  -vl'  =  \  Tri  =  &'  -  ?v. 

324.  The  preceding  Articles  have  sufficiently  shewn  how  the  equations 
of  transformation  of  the  periods  arise  by  the  consideration  of  the  Abelian 
integrals.  It  is  of  importance  to  see  that  equations  of  the  same  character, 
but  of  more  general  significance,  arise  in  connexion  with  the  analytical 
theory  of  the  theta  functions. 

Let  <w,  &>',  77,  ?;'  be  any  four  matrices  of  p  rows  and  columns  satisfying 
the  conditions  (i)  that  the  determinant  of  &>  does  not  vanish,  (ii)  that  co~la)' 
is  a  symmetrical  matrix,  (iii)  that  the  quadratic  form  co^tw'w2  has  its 
imaginary  part  positive  when  nly  ...,np  are  real,  (iv)  that  r)a)~l  is  a  sym 
metrical  matrix,  (v)  that  rj  =  t]w~lo>'  —  ^Triw~l.  The  conditions  (i),  (ii),  (iv), 
(v)  are  equivalent  to  equations  of  the  form  of  (B)  and  (C),  §  140,  and, 
taking  matrices  a,  b,  h  such  that  a  =  ^t}(o~1)  h  =  ^7riw~l,  b  =  Triw^co',  or 
2hw  =  TTI,  Zha)'  =  b,  i]  =  2a&),  ?/  =  2aa>'  —  h,  the  condition  (iii)  ensures  the 
existence  of  the  function  defined  by 

^.  (u  .    <2'\  _  ^eo«2+2to(n+Q')+6(n+Q')2+2«Q(n+Q')) 

wherein  Q,  Q'  are  any  constants  (cf.  §  174). 

Introduce  now  two  other  matrices  [&>],  [&/],  also  of  p  rows  and  columns, 
defined  by  the  equations 

[&>]  =  cow  +  &)V,  =  ^Ha,  say,     [CD']  =  (u/3  +  &//3',  =  £00,  say, 
where  a,  a',  /3,  ft',  are  matrices  of  p  rows  and  columns  whose  elements  are 


824]  ARGUMENTS   OF   A   THETA   FUNCTION.  535 

integers*,  it  being  supposed  i"  that  the  determinant  of  the  matrix  [<w]  does 
not  vanish  ;  and  introduce  p  other  variables  wi}  ...,  wp  denned  by 

m=  Mif  !«/!  +  ......  +Miipwp,  (i=  1,  2,  ...,p) 

or  u  =  Mw,  where  M  is  a  matrix  of  constants,  whose  determinant  does  not 
vanish;  let  the  simultaneous  increments  of  wl}  ...,wp  when  ult  ...,up  are 
simultaneously  increased  by  the  constituents  of  the  j-th  column  of  [<w]  be 
denoted  by  vltj,  .  ..,  vpj,  and  the  simultaneous  increments  of  wl>  .  ..,  wp 
when  MJ,  ...,up  are  simultaneously  increased  by  the  elements  of  the  j-ih 
column  of  [«']  be  denoted  by  v'^j,  ...,V'PIJ\  then  we  have  the  equations 
2Mv  =  2  [CD]  =  fta,  2Mi/  =  2  [&>']  =  Hp,  where  u,  i/  denote  the  matrices  of 
which  respectively  the  (i,j)  elements  are  Vij  and  v'ij. 

The  function  S-(w;  ^)  is  a  function  of  w1;  ...,  wp;  we  proceed  now  to 
investigate  whether  it  is  possible  to  choose  the  matrices  a,  a.',  /3,  ft'  and  the 
matrix  M,  so  that  the  function  may  be  regarded  as  a  theta  function  in 
wlt  ...,wp  of  order  r  (cf.  Chap.  XV.  §  284). 

Let  the  arguments  wl}  ...,  wp  be  simultaneously  increased  by  the  con 
stituents  of  the  j-th  column  of  the  matrix  2t>;  thereby  u^,  .  ..,  up  will  be 
increased  by  the  constituents  of  the  j-ih  column  of  the  matrix  [2&>],  and, 
since  a,  a,  /3,  /3'  consist  of  integers,  the  function  S-  (u  ;  ^  )  will  (Chap.  X. 
§  190)  be  multiplied  by  a  factor  e^i  where 

Z,-  =  (#.)«>  [w  +  i(fla)tf>]-7rtt(«)(')  (a')(j)  +27rt'[(a)tf>  Q'-(O(j)  Q], 
(a)(^  denoting  the  row  of  ^  elements  forming  the  J-th  column  of  the  matrix 
a,  and  (na)(-",  (Ha}(h  denoting,  similarly,  the  j-ih  columns  of  the  matrices 
2<»a  +  2<a'a',  2?;a  +  277  V  respectively  ;  this  expression  Lj,  is  linear  in  w/u  .  .  .  ,  wp, 
and  can  be  put  into  the  form 


where  (wlt  ...,  wp)  denotes  the  row  letter  whose  elements  are  wlt  ...,  wp,  and 
similarly  (vltj,  ...,  vp>j)  is  the  row  letter  formed  by  the  elements  of  the  j-th 
column  of  the  matrix  v,  r  is  a  positive  integer  which  is  provisionally 
arbitrary,  Kj  and  2£1|j,  ...,  2%pj  are  properly  chosen  constants,  and 
(%£ij,  ...,  2^i?-)  is  the  row  letter  formed  of  the  last  of  these.  Similarly,  if 
the  arguments  w1}  ...,wp  be  simultaneously  increased  by  Zv'^j,  ...  ,  2v'pj,  the 
function  S-  (u  ;  ^  )  takes  a  factor  e^'i,  where 

Lf  =  (Hf)<*  [u  +  ±  (Q,)(J>]  -  m  (/3)0')  (/3')U>  +  2^  [(ft)*  Q  -  (P)&  Q], 
and,  with  the  same  value  of  r,  this  can  be  put  into  the  form 


*  The  case  when  a,  a',  j8,  /3'  are  not  integers  is  briefly  considered  in  chapter  XX. 
t  We  have  jn'ur1  [w]  =  iria  +  ba'  ;    we  suppose   that   the   determinant   of  via  +  ba'  does   not 
vanish. 


536  TRANSFORMATION   OF   PERIODS  AND  [324 

where  Kj,  £"1)7-,  ...,  £'pj  are  properly  chosen  constants.     In  these  equations 
we  suppose^  to  be  taken  in  turn  equal  to  1,  2,  .  ..,  p. 
Comparing  the  two  forms  of  Lj  we  have 


or 


so  that  the  (i,  j)th  element  of  the  matrix  MHa  is  2r£ij;  hence  if  f,  £'  denote 
respectively  the  matrices  of  the  quantities  ^j  and  %'ij,  we  have 

toa  =  2r£  MH?  =  2<  ;  (V.) 

from  these  we  deduce,  in  virtue  of  the  equations  *2Mv  =  £la,  2Mv  =  Zip, 


and  therefore,  in  particular,  comparing  the  (j,  j)ih  elements  on  the  two  sides 
of  these  equations, 


where,  as  before,  (t/)^  is  the  row  letter  formed  by  the  elements  of  the  j-th 
column  of  the  matrix  v,  etc.;  therefore  the  only  remaining  conditions 
necessary  for  the  identification  of  the  two  forms  of  Lj  and  L/,  are 


Kf  =  (a)0  Q'  -  (a')"'  Q  -  1  (a)U>  (a')'*,  -  Kj  =  (/3)(j)  Q'  -  (/3')(j)  Q  - 
and  the  j9  pairs  of  equations  of  this  form  are  included  in  the  two 

K'  =  «Q'  -a'Q-^d  (fia'),  -K  =  0Q-  0'Q  -  $d  (0/3'),          (VI) 

where  K',  K  are  row  letters  of  p  elements  and  d  (aaf),  d(ft/3')  are  respectively 
the  row  letters  of  p  elements  constituted  by  the  diagonal  elements  of  the 
matrices  aa',  y9/3'. 

The  equations  (VI.)  arise  by  identifying  the  two  forms  of  Lj  and  Z/;  it  is 
effectively  sufficient  to  identify  the  two  forms  of  eLJ  and  eLi'\  thus  it  is 
sufficient  to  regard  the  equations  (VI.)  as  congruences,  to  the  modulus  1. 

We  now  impose  upon  the  matrices  v,  v',  £,  £'  the  conditions 

f«,  -  X=  0  =  I  'v'  -  V?,    lv    -  V?  =  %7Ti,  (VII.) 

which,  as  will  be  proved  immediately,  are  equivalent  to  certain  conditions 
for  the  matrices  a,  /3,  'a.',  /3';  then,  denoting  *r(u;  J)  by  <f>(wly  ...,wp)  or 
<f>(w),  it  can  be  verified*  that  the  2p  equations 

<t>(...,Wr  +  2vrJ,...)  =  eL><l>(w\  $(...,  wr  +  2v\.>i,...)  =  eL>'<t>(w),(j  =  l,...,p\ 
where  Lj,  L/  have  the  specified  forms,  lead  to  the  equation 

<j>  (w  +  %vm  -f  2l»'m')  =  er^m+2£  m'>  (w+vm+v'm1)—  rmmm'+2Tri(mK'-m'K)  A  /^,\ 

wherein  m,  m'  are  row  letters  consisting  of  any  p  integers  ;  and  this  is  the 
*  The  verification  is  included  in  a  more  general  piece  of  work  which  occurs  in  Chap.  XIX. 


324]  ARGUMENTS   OF   A  THETA   FUNCTION.  537 

characteristic  equation  for  a  theta  function  of  order  r  with  the  associated 
constants  2u,  2i/,  2£  2£'  (§  284,  p.  448). 

The  equations  (VII.)  are  equivalent  to  conditions  for  the  matrices  v,  v\ 
£,  £',  entirely  analogous  to  the  conditions  (ii),  (iv),  (v)  of  §  324  for  the 
matrices  w,  &>',  77,  77'.  The  condition  analogous  to  (i)  of  §  324,  namely  that  the 
determinant  of  the  matrix  v  do  not  vanish,  is  involved  in  the  hypothesis 
that  the  determinant  of  Trio.  +  ba.'  do  not  vanish.  It  will  be  proved  below 
(§  325)  that  the  remaining  condition  involved  in  the  definition  of  a  theta 
function,  viz.  that  the  quadratic  form  v~lv'n*  has  its  imaginary  part  positive 
for  real  values  of  nlt  ...,  np>  is  a  consequence  of  the  corresponding  condition 
for  the  matrices  &>,  &>'.  We  consider  first  the  conditions  for  the  equations 
(VII). 

In  virtue  of  equations  (V.),  the  equations  (VII.)  require 


=  4r  ($/  -  v?)  = 

and,  similarly, 

HaCla  -  iiJJ.  =  0,  Hftflft  -  npHft  =  0  ; 

but 

')  (&>/3  +  o'/S')  -  (aa>  +  oV)  (77/3  +  T//3'), 
j3'  +  a  (rf(*>  -  0/77)  /3  +  a'  (tfw  -  wrf}  $', 
and  this,  by  the  equations  (B),  §  140,  is  equal  to 

i7n'(a/3'-a'/3); 
thus 

a/3'  -  a'/3  =  yg'a  -  yga'  =  r,  (  VIII.) 

and,  similarly, 

aa'-o'a  =  0,   /9/g'  -  J3'/3  =  0  ; 

and  as  before  (§  322)  these  three  equations  can  be  replaced  by  the  three 

ay8  =  /Sa,    of  ft'  =  /Pa',    *$'  -  $*'  =  r  =  jS'a-  *'$,  (IX.) 

the  relations  satisfied  by  the  matrices  a,  /9,  a',  £'  respectively  being  similar  to 
those  satisfied  by  o>,  o>',  77,  77',  with  the  change  of  the  ^-rri,  which  occurs  in  the 
latter  case,  into  —  r. 

The  number  r  which  occurs  in  these  equations  is  called  the  order  of  the 
transformation;  when  it  is  equal  to  1  the  transformation  is  called  a  linear 
transformation. 

Ex.  i.     Prove  that,  with  matrices  of  2p  rows  and  2p  columns, 
«    0W     ?    -0\          A   0\       /«    a' 


ana 

/a    0WO    -IWa    a'\         /O    -  1\ 

W/r/v    oA/3)3';-rVi    o;- 

The  determinant  of  the  matrix  will  be  subsequently  proved  to  be 


538  CONVERGENCE   OF   TRANSFORMED    FUNCTION.  [324 

Ex.  ii.     Prove  that  the  equations  (V.)  of  §  324  are  equivalent  to 
(M      0     \  /2v  2iA  _  /2o>  2«A  fa   |3  \ 

Vo  RfftV  W  «V  "  k*i  *i')  V  ft'J  ' 

Ex.  iii.     If  x,  y,  xlt  y±  be  any  row  letters  of  p  elements,  and  X,  Y,  Jfo  Y±  be  other 
such  row  letters,  such  that 

f         .  X 

tey),  °      T 

then  the  equations  (VIII.)  are  the  conditions  for  the  self-transformation  of  the  bilinear 
form  xy±  —  x$,  which  is  expressed  by  the  equation 

XTl-XlY^r(xy^-xly). 

325.  Conversely  when  the  matrices  a,  a,  j3,  ft  satisfy  the  equations 
(VIII.),  the  function  ^  (u  ;  ^  )  satisfies  the  determining  equation  for  a  theta 
function  in  w1}  ...,  wp,  of  order  r,  with  the  characteristic  (K,  K'},  and  with 
the  associated  constants  2u,  2t/,  2f,  2£";  and  in  virtue  of  the  equations  (VII.), 
the  determinant  of  v  not  vanishing,  matrices  a,  b,  h,  of  which  the  first  two 
are  symmetrical,  can  be  taken  such  that 

a  =  \  £v~l,    h  =  ^  Triv~l,   b  =  7riv~l  v'  ; 

we  proceed  now  to  shew*  that  the  real  part  of  the  quadratic  form  bw3  is 
negative  for  real  values  of  nl}  ...,np>  r  being  positive,  as  was  supposed. 

The  quantity,  or  matrix,  obtainable  from  any  complex  quantity,  or 
matrix  of  complex  quantities,  by  changing  the  sign  of  the  imaginary  part 
of  that  quantity,  or  of  the  imaginary  parts  of  every  constituent  of  that 
matrix,  will  be  denoted  by  the  suffix  0  ;  and  a  similar  notation  will  be  used 
for  row  letters  ;  further  the  symmetrical  matrices  w~l(a,  v~lv  will  be  denoted 
respectively  by  T  and  r',  so  that  b  =  TTIT,  b  =  TTIT'  ;  also  r,  r  will  be  written, 
respectively,  in  the  forms  TL  +  irz>  T/  +  ira',  where  T!,  r2,  iV,  r2'  are  matrices 
of  real  quantities.  Then,  putting 

x  =  vM(a~[x,  and  therefore  #„'  =  V^MQW^XQ, 

where  x,  x  denote  rows  of  p  complex  quantities,  and  x0',  x0  the  rows  of  the 
corresponding  conjugate  complex  quantities,  and  recalling  that 

r'^r'  =  vv-1,    a>-1Mv  =  OL  +  TCL',    a)~lM  v  =  /3  +  rft, 
we  have  _  _  _ 

^x  .  V^M^W^XQ  =  v'MwT^x  .  v^M^^Xo 


and,  if  x  =  xl  +  ix2,  sc0  =  x1  —  ix^,  where  xlf  x2  are  real,  this  is  equal  to 
(]3  +  ft^  +  ift-r.?)  (^  +  ix2)  .  (a  +  S'T! 


or 

\ftP  +  ftP'  +  i  (J3Q  +  ftQ'}}  [5P  +  fi'P'  -  i  (aQ  +  a'Q')], 

*  Hermite,  Compt.  Eendus,  XL.  (1855),  Weber,  Ann.  d.  Mat.,  Ser.  2,  t.  ix.  (1878—9). 


326]  SIMPLEST   FORM   OF   THE    LINEAR   TRANSFORMATION.  539 

where  P,  P',  Q,  Q'  are  row  letters  of  p  real  quantities  given  by 

P  =  Xlt    P  =  T^  -  T2#2,    Q  =  X2,    Q'=  7V 

so  that 

thus  the  coefficient  of  i  in  T'X'XQ  is 

(fiP  +  a'F)  08Q  +  ft'Q')  -  (ftP  +  ft'P')  («Q  +  a'Q'), 

which,  in  virtue  of  the  equations  (IX.),  is  equal  to  r  (PQ'  —  P'Q)  or 
rrz  (x?  +  #22)  ;  thus  the  coefficient  of  i  in  r'afx^  is  equal  to  the  coefficient 
of  i  in  rTXxn.  Since  x  may  be  regarded  as  arbitrarily  assigned  this  proves 
that  the  imaginary  part  of  r'x'x0  is  necessarily  positive  ;  and  this  includes 
the  proposition  we  desired  to  establish. 

Ex.     Prove  that  the  equation  obtained  is  equivalent  to 

J/Q  VQ  T2'vM  =  rWQ  T2  <5. 

326.  Of  the  general  formulae  thus  obtained  for  the  transformation  of 
theta  functions,  the  case  of  a  linear  transformation,  for  which  r=l,  is  of 
great  importance  ;  and  we  limit  ourselves  mainly  to  that  case  in  the 
following  parts  of  this  chapter.  We  have  shewn  that  a  theta  function  of  the 
first  order,  with  assigned  characteristic  and  associated  constants,  is  unique, 
save  for  a  factor  independent  of  the  argument  ;  we  have  therefore,  for  r  =  1, 
as  a  result  of  the  theory  here  given,  the  equation 


We  suppose  a,  ft,  a,  ft'  to  be  any  arbitrarily  assigned  matrices  of  integers 
satisfying  the  equations  (VIII.)  or  (IX.);  then  there  remains  a  certain 
redundancy  of  disposable  quantities  ;  we  may  for  instance  suppose  co,  w  ,  77,  T/ 
and  M  to  be  given,  and  choose  v,  v,  £,  £'  in  accordance  with  these  equations  ; 
or  we  may  suppose  to,  &>',  v,  %  and  £'  to  be  prescribed  and  use  these  equations 
to  determine  M,  v',  r)  and  ?/.  It  is  convenient  to  specify  the  results  in  two 
cases.  We  replace  u,  w  respectively  by  U,  W. 

(i)     2o)  =  1,  2co'  =  r  ,  T;  =  a,  T/'  =  ar  —  m,  h  =  TTI,  b  =  TTIT, 

2u  =  1,  2i/  =  T',  £  =  0,  £"  =  —  iri      ,  a  =  0  ,  h  =  iri  ,  b  =  TTI'T', 
U  =  MW,  M  =  a  +  ra',  (a  +  TO!)  r'  =  ft  +  rft', 

so  that,  as  immediately  follows  from  equations  (IX.), 

Ta')  =  r  =  (/3/-aV)(a  +  aT),  U=(a  +  Ta')W,  W  =\(&  -r'a.')U, 


and,  because  ij'  =  rjr  —  TTI  and  £  =  0, 

| 

from  which  we  get 


7T"?  — 

a  =  77  =  iria! (a  +  ra')'1  =  ~  a' (ft'  -  r'a), 


540  SIMPLEST   FORM    OF   THE   LINEAR   TRANSFORMATION.  [326 

a  U*  =  —  «'  (£'  -  T'O')  tf2  =  TriV  F  U  =  Trt  V  (a  +  ra')  Fa. 
These  equations  satisfy  the  necessary  conditions,  and  lead,  when  r  =  1,  to 

';    *')  f  (X.) 


where  A  is  independent  of  £/!,  ...,  Up,  and  the  characteristic  (K,  K'}  is  deter 
mined  from  (Q,  Q'}  by  the  equations  (§  324) 

IT  =  aQ'  -  a'Q  -  id  (aa'),     -K  =  0Q[ 


The  appearance  of  the  exponential  factor  outside  the  e-function,  in  equation  (X.), 
would  of  itself  be  sufficient  reason  for  using,  as  we  have  done,  the  5-function,  in  place  of 
the  6-function,  in  all  general  algebraic  investigations*. 

If  in  §  324  we  put 


we  easily  find 

via1  (a  +  ra')  TF2  =  ^o>  ~  %2  -  irfw  ~  %2  ; 

thus  (§  189,  p.  283)  equation  (X.)  includes  the  initial  equation  of  this  Article. 

In  general  the  function  occurring  on  the  left  side  of  equation  (X.)  is 
a  theta  function  in  W  of  order  r  with  associated  constants  2v  —  1,  2i/  =  T', 
2£=0,  2£'=-27rt,  and  characteristic  (K,  K'). 

(ii)  A  particular  case  of  (i),  when  the  matrix  a!  consists  of  zeros,  is  given 
by  the  formulae 

2&)  =  1,  2&>'  =  T  ,  V)  =  0,  t\  =  —  TTI,  a  =  0,  A  =  7n,  6  =  TH'T  , 
2u  =  1,  2i/  =  T',  £  =  0,  £'  =  -  Tri,  a  =  0,  h  =  TTt,  b  =  TUT', 

£7  =  «  If,  T  =  a-1  (£  +  r/3'),  r  =  -  (err7  -  /3)  a, 

r 


/a    £  \      /a  /3     \        ,  5 

'   /o'    =    A     —  i    >  wnere  a£  =  /3a. 
\a    p  1      \0  ra  V 


Then  the  function  @((7;  r;  «')  or  ©  [a  W;  1  (ar7  -  /9)  a  ;  |]  is  a  theta 

function  in  W,  of  order  r,  with  associated  constants  2u  =  1,  2i»'  =  r/,  2^=0, 
2  ^"  =  —  2-Tn,  and  characteristic  (.ST,  K')  given  by 


and,  in  particular,  when  r  =  1  we  have 

.'--          :    ,      ''  e(tr;r;f)=4@(Tf;T';5'))  "  (XL) 

where  A  is  independent  of  U1}  ...,  Z7P. 

*  Of.  §  189  (Chap.  X.);   and   for  the  case  _p  =  l,  Cayley,  Liouville,  x.  (1845),  or  Collected 
Works,  Vol.  i.,  p.  156  (1889). 


327]  TRANSFORMATION   OF  CHARACTERISTICS.  541 

327.  It  is  clear  that  the  results  just  obtained,  for  the  linear  trans 
formation  of  theta  functions,  contain  the  answer  to  the  enquiry  as  to  the 
changes  in  the  Riemann  theta  functions  which  arise  in  virtue  of  a  change  in 
the  fundamental  system  of  period  loops.  Before  considering  the  results  in 
further  detail,  it  is  desirable  to  be  in  possession  of  certain  results  as  to  the 
transformation  of  the  characteristics  of  the  theta  function,  which  we  now 
give  ;  the  reader  who  desires  may  omit  the  demonstrations,  noticing  only  the 
results,  and  proceed  at  once  to  §  332.  We  retain  the  general  value  r  for  the 
order  of  the  transformation,  though  the  applications  of  greatest  importance 
are  those  for  which  r  =  1. 

As  before  let  ^(7)  denote  the  row  of  p  quantities  constituted  by  the 
diagonal  elements  of  any  matrix  7  of  p  rows  and  columns  ;  in  all  cases  here 
arising  y  is  a  symmetrical  matrix  ;  then  we  have 

a  d  03/3')  +  /3d  (aa')  =  rd(aft  ),     ft'd  (aft)  +  fid  (aft')  =  rd  (ft  ft') 

_  _  _  (mod.  2) 

ad  (ft  ft')  +  ft'd  (aa')  =  rd  (a'  ft'),      *'d  (aft)  +  ad  (a/3')  =  rd(aa') 

and 

d  (a*')  d  (#3')  =  (r+l)  2d  (fta)  =  (r  +  l)  2d  (ft'a) 


-  -  _  (mod.  2), 

d  (a/9)  d  (a'  ft')  =  (r  +  I)  2d  (aft')  =  (r  +  1)  2d  (ft  a') 

so  that,  when  r  =  1  or  is  any  odd  integer, 

d  (aa)  .  d  (ft/3')  =  d  (aft)  .  d  (a'  ft')  =  0     (mod.  2). 

The  last  result  contains  the  statement  that  the  linear  transformation  of 
the  zero  theta-characteristic  is  always  an  even  characteristic. 

For  the  equations 

ft'd  -a'  ft  =  r,     aft  =  ftd, 
give 

aft  ft'a  -ftaa'  ft  =  raft, 
and  therefore 

ftft'z*-aay  =  raftx2, 

where  x  is  any  row  letter  of  p  integers,  and  z—ax,  y  =  $x;  but  if  y  be  a  symmetrical 
matrix  of  integers  and  t  be  any  row  letter  of  p  integers  yp,  =yn^2  +  ...  +  2y12^2-f...,  is 
=  yn'i2+  •••  +  Wp2>  and  therefore  =yut1+...  +ypptp,  or  =d(y).  t,  for  modulus  2  ;  hence 

d  (ftp)  z-d  (aa')  y  =  rd  (aft)  x    (mod.  2) 
or 

[ad  (ftp)  +pd  (aa')  -  rd  (aft)]  x  =  0    (mod.  2)  ; 

and  as  this  is  true  for  any  row  letter  of  integers,  #,  the  first  of  the  given  equations  follows 
at  once.  The  second  of  the  equations  also  follows  from  /3'a  -  a'J3  =  r,  in  the  same  way,  and 
the  third  and  fourth  follow  similarly  from  pa  —  fia=r. 

To  prove  the  fifth  equation,  we  have,  since  PS  —  aft  =  r, 

ftft'aa'  =  fta'fta' 

or 


542  PROPERTIES   UNALTERED   BY   LINEAR  TRANSFORMATION.  [327 

where  b=ftftr,  a  =  aa,  c  =  fta' ;  hence,  equating  the  sums  of  the  diagonal  elements  on  the  two 
sides  of  the  equation,  we  have 

p    P  p    p  P 

2T    7).    -n  •    • —    ^      T    P'    ./>.   .-L.V  *9    s>     .  . 
£i    k%  j  MJ,  i  —  ^      ^    ^j  V  C-*  j  T-  /    2i   Cj •  ^  , 

j=l  i=l  j=l  i=l  i=l 

therefore,  as,  unless  i=j,  bitjO,jti  =  bj<iai>j,  because  a,  b  are  symmetrical  matrices,  and  as 

we  obtain 

p  P  P 

2  aiti\i=  2  (c2i>i+rc1-)i)  =  (r+ 1)  2  c,-jt-. 

The  sixth  equation  is  obtained  in  a  similar  way,  starting  from  ft'a  —  fta'  =  r. 

Of  the  results  thus  derived  we  make,  now,  application  to  the  case  when  r  is  odd,  limiting 
ourselves  to  the  case  when  the  characteristic  (Q,  Q')  consists  of  half-integers  ;  we  put  then 
Q  —  fyi  Q'  =  Wi  so  that  q,  q'  each  consist  of  p  integers  ;  then  K,  K'  are  also  half-integers, 
respectively  equal  to  \k,  \k' ,  say,  where 

k'  =  aq'  -a'q-d  (aa'),      -k  =  ftq'-ft'q-d  (ft  ft'). 

In  most  cases  of  these  formulae,  it  is  convenient  to  regard  them  as  congruences,  to 
modulus  2.  This  is  equivalent  to  neglecting  additive  integral  characteristics. 

From  these  equations  we  derive  immediately,  in  virtue  of  the  equations  of  the  present 
Article 

q=ak  +  ftk'  +  d(aft),     q'  =  a'k  +  ft'k'  +  d  (a' ft')     (mod.  2) 
and 

qq'  =  kk'     (mod.  2). 

Further  if  p,  p'  be  row  letters  of  p  integers,  and 

v'  =  afj.'  —  a'p.  —  d(aa),      —v=ftp  —  ft'fj.  — d  (ftff), 
we  find,  also  in  virtue  of  the  equations  of  the  present  Article, 

kv  -  k'v = qp  -  q'fi.  +  (p  +  q')  d  (aft)  +  (n  +  q)d  (aft'),     (mod.  2) ; 

therefore,  if  also 

o-'  =  ap  -  a'p  -  d  (aa),      —a~  =  ftp'  —  ft'p  —  d  (ft  ft'), 
we  have 

k  v  -  k'v + vcr  —  v'cr  -f  o-fc'  —  a'k  =  qp  —  q'p. + pp  —  p'p  +  p  q'  —  p'q     (mod.  2 ). 


Denoting  the  half-integer  characteristics  i  ( ^  ) .  A  y    } .  A  ( p  }  by  A,  B,  C, 

2  V?  /  2  W     VP  /   * 

,7/,  .     A  /      '\ 

and  the  characteristics  A(7  1,  Jr'f    1,  |f  (     J,  which  we  call  the  transformed 

\K  I       \v  J        \cr  J 

characteristics,  by  A',  B',  C',  we  have  therefore  the  results  (§  294) 
A\=  A'\,     \A,B,C  =\A',B',C'\,    (mod.  2) 

or,  in  words,  in  a  linear  transformation  of  a  theta  function  with  half-integer 
characteristic,  and  in  any  transformation  of  odd  order,  an  odd  (or  even) 
characteristic  transforms  into  an  odd  (or  even)  characteristic,  and  three 
syzygetic  (or  azygetic)  characteristics  transform  into  three  syzygetic  (or 
azygetic)  characteristics. 

Of  these  the  first  result  is  immediately  obvious  when  r  =  \   from   the   equation   of 
transformation  (§  326),  by  changing  w  into  —w. 


THETA   CHARACTERISTICS   AND   PERIOD   CHARACTERISTICS.  543 

Hence  also  it  is  obvious  that  if  A  be  an  even  characteristic  for  which 
;  A)  vanishes,  then  the  transformed  characteristic  A'  is  also  an  even 
characteristic  for  which  the  transformed  function  ^  (0 ;  A')  vanishes. 

328.     If  in  the  formula  of  linear  transformation  of  theta  functions  with 
half-integer  characteristic,  which  we  may  write 


we  replace  u  by  u  +  ^£lm  =  u  +  com  +  a>'m'  ,  where  m,  m'  denote  rows  of 
integers,  and,  therefore,  since  w  =M(vJ3'  —  v'af),  w  —  M  (—  v/3  +  i/a),  (cf.  Ex.  i., 
§  324),  replace  w  by  w  +  vn  +  v'n',  where 

n'  =  am'  —  a'm,     —  n  =  $m!  —  J3'm, 
we  obtain  (§  189,  formula  (L)) 


f 

\u  ; 

|_    ' 


=  <«•  a  \w  ; 

- 


where  A'  is  independent  of  u1}  ...,  up,  and  k'  +  n',  k  +  n  are  obtainable  from 
q'  +  m',  q  +  m  by  the  same  formulae  whereby  k',  k  are  obtained  from  q',  q, 
namely 

k'  +  m'  =  a  (q'  +  m')  -a'(q  +  m)-d  (aa'), 
-  (k  +  m)=0(q'  +  mf)  -  ff  (q  +  m)-d(J3ff); 
these  formulae  are  different  from  those  whereby  n',  n  are  obtained  from 

m',  m  ;  for  this  reason  it  is  sometimes  convenient  to  speak  of  1  f  ^  ]  as  a  theta 

2\qJ 

characteristic,  and  of  ^  I      )  as  a  period  characteristic  ;  as  it  arises  here  the 


difference  lies  in  the  formulae  of  transformation  ;  but  other  differences  will 
appear  subsequently;  these  differences  are  mainly  consequences  of  the 
obvious  fact  that,  when  half-integer  characteristics  which  differ  by  integer 
characteristics  are  regarded  as  identical,  the  sum  of  any  odd  number  of 
theta  characteristics  is  transformed  as  a  theta  characteristic,  while  the 
sum  of  any  even  number  of  theta  characteristics  is  transformed  as  a 
period  characteristic.  In  other  words,  a  period  characteristic  is  to  be 
regarded  as  the  (sum  or)  difference  of  two  theta  characteristics. 

It  will  appear  for  instance  that  the  characteristics  associated  in  §§  244,  245, 
Chap.  XIII.  with  radical  functions  of  the  form  JX  (2"+1>  are  to  be  regarded  as 
theta  characteristics  —  and  the  characteristics  associated  in  §  245  with  radical 
functions  of  the  form  JX^,  which  are  denned  as  sums  of  characteristics 
associated  with  functions  JX(*"+v,  are  to  be  regarded  as  period  characteristics. 


544  LINEAR  TRANSFORMATION   OF  ANY   EVEN  [328 

We  may  regard  the  distinction*  thus  explained  somewhat  differently,  by  taking  as  the 
fundamental  formula  of  linear  transformation  that  which  expresses  #  \  u  ;  £  (     j    in  terms 

where 


Q,.;  |ffj  L 


and 

l'  =  kr  +  d(aa')  =  aq'-aq,      -1=  -  k  +  d  ($$}  =  &q'  -  ffq. 

In  the  following  pages  we  shall  always  understand  by  '  characteristic,'  a 
theta  characteristic  ;  when  it  is  necessary  to  call  attention  to  the  fact  that  a 
characteristic  is  a  period  characteristic  this  will  be  done. 

329.  It  is  clear  that  the  formula  of  linear  transformation  of  a  theta 
function  with  any  half-integer  characteristic  is  obtainable  from  the  particular 
case 


where  r'  =  d  (act),  r  =  d  (ft  ft),  by  the  addition  of  half  periods  to  the  argu 
ments.  It  is  therefore  of  interest  to  shew  that  matrices  a,  ft,  of,  ft'  can  be 
chosen,  satisfying  the  equations 

aft  =  ft  a,     a'  ft'  =  ft'  a,     aft'  -fta=l, 

ir'\ 
which  will  make  the  characteristic  ^  I     j   equal  to  any  even  half-integer 

characteristic. 

Any  even  half-integer  characteristic,  being  denoted  by 

/If  '     If  '\ 

1  Ki  •••Kp  \ 

2  I  J,          I.        > 
\n,i  .  .  .  Up  J 

lk'\ 
we  may,  momentarily,  call  (   *  )  the  i-th  column  of  the  characteristic  ;  then 

V^i  / 

the  columns  may  be  of  four  sorts, 


o' 

but  the  number  of  columns  of  the  last  sort  must  be  even  ;  we  build  now  a 
matrix 

*    *} 

'  ft') 

*  Theta  characteristics  have  also  been  named  eigentliche  Charakteristiken  and  Primcharak- 
teristiken  ;  they  consist  of  2>'-1(2P-l)  odd  and  2P~1(2*>  +  1)  even  characteristics.  The  period 
characteristics  have  been  called  Gruppencharakteristiken  and  Elementarcharakteristiken  or 
sometimes  relative  Charakteristiken.  For  them  the  distinction  of  odd  and  even  is  unimportant  — 
while  the  distinction  between  the  zero  characteristic  —  which  cannot  be  written  as  the  sum  of  two 
different  theta  characteristics  —  and  the  remaining  22P  -  1  characteristics,  is  of  great  importance. 
The  distinction  between  theta  characteristics  and  period  characteristics  has  been  insisted 
on  by  Noether,  in  connection  with  the  theory  of  radical  forms  —  Cf.  Noether,  Math.  Annal. 
xxvin.  (1887),  p.  373,  Klein,  Hath.  Annal.  xxxvi.  (1890),  p.  36,  Schottky,  Crelle,  en.  (1888), 
p.  308.  The  distinction  is  in  fact  observed  in  the  Abel'sche  Functionen  of  Clebsch  and  Gordaii, 
in  the  manner  indicated  in  the  text, 


329] 


CHARACTERISTIC    INTO   THE   ZERO   CHARACTERISTIC. 


545 


of  *2p  rows  and  columns  by  the  following  rule*  —  Corresponding  to  a  column 
of  the  characteristic  of  the  first  sort,  say  the  i-th  column,  we  take  &i,i=l3>i,i=  1  , 
but  take  every  other  element  of  the  t'-th  row  and  t'-th  column  of  a  and  /3', 
and  every  element  of  the  i-th  row  and  i-th  column  of  $  and  a'  to  be  zero  ; 
corresponding  to  a  column  of  the  characteristic  of  the  second  sort,  say  the 
j-ih  column,  we  take  «/,_,-  =  P'jj  =  afjj  —  1,  but  take  every  other  element  of 
the  j-th  row  and  j-th  column  of  a,  /?',  a',  and  every  element  of  the  j-th  row 
and  column  of  @,  to  be  zero  ;  corresponding  to  a  column  of  the  characteristic 
of  the  third  sort,  say  the  ra-th  column,  we  take  am>m  =  fim,m  =  ftm,m  =  1,  but 
take  every  other  element  of  the  m-th  row  and  column  of  a,  /3,  /3'  and  every 
element  of  the  m-th  row  and  column  of  «'  to  be  zero  ;  corresponding  to  a  pair 
of  columns  of  the  characteristic  of  the  fourth  sort,  say  the  p-ih  and  cr-th,  we 
take  ap>  p  =  /3P)  p  =  j3'pi  p  =  l,  a<r>tr  =  a^  „  =  ft'*,  «  =  1,  a^  p  =  1,  /8pt  v  =  -  1,  a!Vt  p  =  1, 
/3'p)(r  =  —  1,  and  take  every  other  element  of  the  p-ih  row  and  column  and  of 
the  o--th  row  and  column,  of  each  of  the  four  matrices  a,  a',  yS,  /3',  to  be  zero. 
Then  it  can  be  shewn  that  the  matrix  thus  obtained  satisfies  all  the 
necessary  conditions  and  gives  k'  =  d  (««'),  k  =  d  (/S/3'). 

Consider  for  instance  the  case  p  =  5,  and  the  characteristic 


/O  1  0  1  1\ 
\0  0  1  1  \) 


the  matrix  formed  by  the  rules  from  this  characteristic  is 


1 

0 

0 

o 

0 

0 

0 

0 

0 

0 

0 

1 

0 

0 

0 

'o 

0 

0 

0 

0 

0 

0 

1 

a 

0 

0 

0 

1 

0 

0 

0 

0 

0 

i 

0 

0 

0 

0 

1 

_  J 

0 

0 

0 

i 

1 

0 

0 

0 

0 

0 

0 

0 

0 

o 

0 

1 

0 

0 

0 

0 

0 

1 

0 

0 

0 

0 

1 

0 

0 

0 

0 

0 

0 

0 

0 

0 

0 

1 

0 

0 

0 

0 

0 

0 

0 

0 

0 

0 

1 

_  J 

0 

0 

0 

1 

1 

0 

0 

0 

0 

1 

and  it  is  immediately  verified  that  this  satisfies  the  equations  for  a  linear  transformation 
(§  324  (IX.),  for  r  =  l),  and  gives,  for  the  diagonal  elements  of  aa',  J3f¥,  respectively,  the 
elements  01011  and  00111. 

Since  we  can  transform  the  zero  characteristic  into  any  even  characteristic,  we  can  of 
course  transform  any  even  characteristic  into  the  zero  characteristic ;  for  instance,  when 
there  is  an  even  theta  function  which  vanishes  for  zero  values  of  the  arguments,  we  can 
by  making  a  linear  transformation,  take  for  this  function  the  theta  function  with  zero 
characteristic. 


*  Clebsch  and  Gordan,  Abel.  Fctnen  (Leipzig,  1HGO),  p.  318. 


35 


546 


TRANSFORMATION  OF  ANY  AZYGETIC  SYSTEM 


[329 


Ex.     For  the  hyperelliptic  case,  when  jo  =  3,  the  period  loops  being  taken  as  in  §  200, 
the  theta-function  whose  characteristic  is  \  ( ,  .,  ,  )  vanishes  for  zero  arguments  (§  203) ; 


prove  that  the  transformation  given  by 


a  =  (       100),          /3=( 

-1       00),           a'  =  (  00-1 

),         £'  =  ( 

101) 

010 

0-10 

loo    o 

010 

-101 

1      00 

00-1 

001 

is  a  linear  transformation  and  gives  an  equation  of  the  form 


where  A  is  independent  of  ul9  ...,  up. 

330.  We  have  proved  (§327)  that  if  three  half-integer  theta  character 
istics  be  syzygetic  (or  azygetic)  the  characteristics  arising  from  them  by  any 
linear  transformation  are  also  syzygetic  (or  azygetic).     It  follows  therefore 
that  a  Gb'pel  system  of  2r  characteristics,  syzygetic  in  threes  (§  297,  Chap. 
XVII.),  transforms  into  such  a  Gbpel  system.     Also  the  22<r  Gb'pel  systems  of 
§  298,  having  a  definite  character,  that  of  being  all  odd  or  all  even,  transform 
into  systems  having  the  same  character.     And  the  2o-  +  1  fundamental  Gopel 
systems  (§  300),  which  satisfy  the  condition  that  any  three  characteristics 
chosen  from  different  systems  of  these  are  azygetic,  transform  into  such 
systems  ;  moreover  since  the  linear  transformation  of  a  characteristic  which 
is  the  sum  of  an  odd  number  of  other  characteristics  is  the  sum  of  the 
transformations  of  these  characteristics,  the  transformations  of  these  2cr  +  1 
systems  possess  the  property  belonging  to  the  original  systems,  that  all  the 
22<r  Gopel  systems  having  a   definite    character   are   representable   by  the 
combinations  of  an  odd  number  of  them.     It  follows  therefore  that   the 
theta  relations  obtained  in  Chap.  XVII.,  based  on  the  properties  of  the 
Gb'pel  systems,  persist  after  any  linear  transformation. 

331.  But  questions  are  then  immediately  suggested,  such  as  these  :   What  are  the 
simplest  Gopel  systems  from  which  all  others  are  obtainable*  by  linear  transformation1? 
Is  it  possible  to  derive  the  22<r  Gopel  systems  of  §  298,  having  a  definite  character,  by 
linear  transformation,  from  systems  based  upon  the  22<r  characteristics  obtainable  by  taking 
all  possible  half-integer  characteristics  in  which  p  —  a-  columns  consist  of  zeros  ?     Are  the 
fundamental  sets  of  2p  +  1  three-wise  azygetic  characteristics,  by  the  odd  combinations  of 
which  all  the  22p  half-integer  characteristics  can  be  represented  (§  300),  all  derivable  by 
linear  transformation  from  one  such  set  ? 

We  deal  here  only  with  the  answer  to  the  last  question  —  and  prove  the  following 
result:  Let  D,  Dlt  ...,  AP  +  I  be  any  2p  +  2  half  -integer  characteristics,  such  that,  for  i<j, 


*  An  obvious  Gopel  group  of  2v  characteristics  is  formed  by  all  the  characteristics  in  which 
the  upper  row  of  elements  are  all  zeros,  and  the  lower  row  of  elements  each  =  0  or  £ . 


331]  INTO    A   STANDARD    AZYGETIC   SYSTEM.  547 

i=l,  ...,  2p,  j  =  2,  ...,  2/>-fl,  we  have  \D,  Dt,  D,  =1  ;  then  it  is  possible  to  choose  a  half- 
integer  characteristic  E,  and  a  linear  transformation,  such  that  the  characteristics 

ED,  EDlt  .. 
transform  into 

0,  Xu  ..., 

where  Xj,  ...,  X2P  +  1  are  certain  characteristics  to  be  specified,  of  which  (by  §  327)  every  two  are 
azygetic.  It  will  follow  that  if  D',  D^,  .  .  .  ,  D'2P  +  1  be  any  other  set  of  2p  +  2  characteristics 
of  which  every  three  are  azygetic,  a  characteristic  E',  and  a  linear  transformation,  can  be 
found  such  that,  with  a  proper  characteristic  E,  the  set  ED,  ED±,  ...,  ED2p  +  l  transforms 
into  E'D1,  E'Di,  ...,  E'D'^p  +  l.  It  will  be  shewn  that  the  characteristics  X1}  ...,X2p  +  1 
can  be  written  down  by  means  of  the  hyperelliptic  half-periods  denoted  (§  200)  by  ua>  c\ 
ua,a^  ua,c^  ^  ua'a",  ua'°  ;  it  has  already  been  remarked  (§  294,  Ex.)  that  the  charac 
teristics  associated  with  these  half-periods  are  azygetic  in  pairs.  The  proof  which  is  to  be 
given  establishes  an  interesting  connexion  between  the  conditions  for  a  linear  transforma 
tion  and  the  investigation  of  §  300,  Chap.  XVII. 
Taking  an  Abelian  matrix, 

/-  P-\ 

V/37' 

for  which 

aa'-a'a  =  0,     jS/S'  -  J3'/3  =  0,     ap  -&'&=!, 

define  characteristics  of  integers  by  means  of  the  equations 


where  a'g>r  is  the  r-th  element  of  the  s-th  row  of  the  matrix  a',  etc.  and  r=l,2,  ...  ,  p  •  tfeen 
the  symbol  which,  in  accordance  with  the  notation  of  §  294,  Chap.  XVII.,  we  define  by  the 
equation 

Mr>  •5»i=ai,r£'i>*+'"+ap,rP>'p,«~a/l,>-P>l,«~  •••  —  O-'p,  r  Pp,s> 

is  the  (?•,  s)-th  element  of  the  matrix  a/rf-a'p1,  and  may  be  denoted  by  (a^'-a'/3)r)g;  thus 
the  conditions  for  the  matrices  a,  a',  /3,  p"  are  equivalent  to  the  p  (2p—l)  equations 

\Ar,Br\  =  l,     \Ar,B8\=0,     1^,^1=0,     \J3r,Bs=0,     (r=j=«,  r,  s  =  l,  2,  ...,  p), 

whereof  the  first  gives  p  conditions,  the  second  p(p-  1)  conditions,  and  the  third  and 
fourth  each  \p(p—  1)  conditions.  It  is  convenient  also  to  notice,  what  are  corollaries 
from  these,  the  equations 

\B,,Ar\=-  Ar,£,=0,    \Br,Ar\=-\Ar,Br\=-l,     Br,  Ar'\=  -\Ar\Br\  =  \Ar)Br\  =  l. 
Consider  now  the  2p  +  l  characteristics,  of  integers,  given  by 


whereof  the  first  2p  are  pairs  of  the  type 


for  r=l,  2,  ...,  p,  and  a^b^  means  the  sum,  without  reduction,  of  the  characteristics  a/, 
blt  a.j,  and  so  in  general.  The  sum  of  these  characteristics  is  a  characteristic  consisting 
wholly  of  even  integers.  If  these  characteristics  be  denoted,  in  order,  by  cn  c2,  ...,  c2p+l, 
it  immediately  follows,  from  the  fundamental  equations  connecting  at,  ...,  6P,  that 


35— -2 


548 


TRANSFORMATION    OF   AZYGETIC    SYSTEMS. 


[331 


Thus  the  (2p  +  l)  half-integer  characteristics  derivable  from  clt  c2,  ...,  c-2p  +  1,  namely 

Ci  =  i«i»  —  »  CIP+I=&*P+I>  are  azJgetic  in  Pairs- 

Conversely  let  Z>,  D^  ...,  D2p  +  l  be  any  half-integer  characteristics  such  that,  for  i<j, 

i  =  l,  ...,  2jt>,  .7  =  2,  ...,  2/>  +  l,  we  have  |  D,  A,  A  =1»  so  that  (§  30°,  P-  496)  there  exist 
connecting  them  only  two  relations  (i)  that  their  sum  is  a  characteristic  of  integers,  and 
(ii)  a  relation  connecting  an  odd  number  of  them  ;  putting  Ci  =  DfDi(i=l,  ...,  *2p),  where 
2y=  -  D,  we  obtain  a  set  of  independent  characteristics  C1}  ...,  C2p,  such  that  for  i<j, 


taking 
tions 


Thus  putting  ^  =  1^,  ...,  C'2J)  + 
the  equations,  previously  given, 


the  i-th  column  of  this  matrix  consisting  of  the  elements  of  the  lower  and  upper  rows  of 
the  integer  characteristic  af  or  bt,  according  as  i<p  +  l  or  i>p.  We  proceed  now  to  find 
the  result  of  applying  the  linear  transformation,  given  by  this  Abelian  matrix,  to  the 
half-integer  characteristics  C1}  ...,  C'2P+1. 

The  equations  for  the  transformation  of  the  characteristic     (        to  the  characteristic 


j  =  2,  3,  ...,2p 

where  C"2)._1=  —  (72,._1,  we  have  also  the  2p  equa- 

=  1,     (m=l,  2,  ...,2p). 

+  1,  we  can  obtain  an  Abelian  matrix  by  means  of 


,  which  are  (§  324,  VI.), 

/?;/  =  aj/-a/2'-c?(aa'),      -k  =  $q'  -ftq-d  0/3'), 
are  equivalent,  in  the  notation  here  employed,  to 

#  =  1^*,  e|-[^(Sa')]i,      -*i  =  |5t,  §  -[^(^')]i,     (*  =  1,  2,  ..., 
where  ^=^4,  ^^Jg-;  taking 


in  turn,  we  immediately  find  that  the  transformations  of  the  characteristics  <72r-i> 
1,  are  given,  omitting  integer  characteristics,  by 

1...100...0\     ,/rf(fi«')\      ,/11...110...0\     ,/rf(aa')\      ,A1... 
l...l  10..  .O'  *d(pp)   +  *\II...IQO...O)'  *VW)/     ^Vll- 


or,  say,  by 


rf(aa')\  , 
* 


«    ,  ! 


respectively. 

Now  let  the  characteristics 

°\  f° 

i/vp 

be  respectively  denoted  by 


then  we  have  proved  that  the  half-integer  characteristic  DDi  transforms,  save  for  an 

(r'\ 
),  where  r=c?(/3/3'),  r'  =  d(aa);  since  the  transforma- 


331]  NUMBER   OF   INCONGRUENT  TRANSFORMATIONS.  549 

tion  of  the  sum  of  two  characteristics  is  the  sum  of  their  transformations  added  to  \  (  r\  , 


-  - 

and  since  the  characteristic  £(     ),  where  s'  =  d(a'p'),  s  =  d(ap),  transforms  into  the  zero 

\s  / 

//\ 

characteristic  (§  327),  it  follows  that  the  transformation  of  the  characteristic  |(     )+DDi 

\s  / 


is  the  characteristic  Xj ;  hence,  putting  E=$  (     }  +D,  and  omitting  integer  characteristics, 

v*/ 

the  characteristics 

ED,  ED,,  ...,  ED2p  +  l 
transform,  respectively,  into 

0,  Xj,  ...,  X2p  +  1 ; 

and  this  is  the  result  we  desired  to  prove. 

The  number  of  matrices  of  integers,  of  the  form 


in  which  aa-aa  =  0,  /3/3'-£'£=0,  5/3'-a'/3  =  l,  is  infinite;  but  it  follows  from  the 
investigation  just  given  that  if  all  the  elements  of  these  matrices  be  replaced  by  their 
smallest  positive  residues  for  modulus  2,  the  number  of  different  matrices  then  arising  is 
finite,  being  equal  to  the  number  of  sets  of  2p  +  l  half-integer  characteristics,  with  integral 
sum,  of  which  every  two  characteristics  are  azygetic.  As  in  §  300,  Chap.  XVII.,  this 
number  is 

3  ......  (22-l)2; 


we  may  call  this  the  number  of  incongruent  Abelian  matrices,  for  modulus  2.     Similarly 
the  number*  of  incongruent  Abelian  matrices  for  modulus  n  is 


Ex.    By  adding  suitable  integers  to  the  characteristics  denoted  by  1,  2,  3,  4,  5,  6,  7  in 
the  table  of  §  205,  for  p  =  3,  we  obtain  respectively 

-100N         /-i  -ION         /-l-lix      ,/-101 

-i  o  o)'         o  -i  o'         o    o  i'        o  i 


00  -IN        /O  1  -IN        (01  ON. 

1  o  -I/1  *Vi  i    o/'  *v  i  i/' 

denoting  these  respectively  by  C^  C2,  ...,  Cr,  we  find,  for  i<j,  that 


The  equations  of  the  text 
give 

and  therefore,  in  this  case,  we  find 

-  1      0  ON  /  -  1  0  IN  /O  0  -  1 

i          n    n      >          aZ  =  [  -,    )i          «<«  =  ( 

—  1      0  O/  \  — Illy  \  0  0  —  1 

-1-1  ON        ft  _  /  - 1  1  IN  /Ol-l 

*  Another  proof  is  given  by  Jordan,  Traits  des  Substitutions  (Paris,  1870),  p.  176. 


550 


TRANSFORMATION    OF   AZYGETIC   SYSTEMS. 


[331 


hence   the '  linear  substitution,   of  the  text,    for  transforming   the   fundamental   set  of 
characteristics  Clt  ...,  C<j  is 

(-1-1       0        0-1       0) 


1       0 

1  -1 


-1 


0 


1    -1   1      0       1-1 


T7  *l.-  C.     A 

from  this  we  find 


1 

=f(1   a 
\s  /         \(»(ap)/         \«  ^ 

integral  characteristic,   it  follows   by   the    general    theorem,   that    if   the  characteristic 

matrix  be  applied,  they  will  be  transformed  respectively  into  the  characteristics  X1?  ...,  \j. 
A  further  result  should  be  mentioned.     On  the  hyperelliptic  Riemann  surface  suppose 
the  period  loops  drawn  as  in  the  figure  (12)  ; 


l  1  '  t   n  ,1     • 

—\\  j,    3()=f(1   a      )>  since  the  sum  of  Clt  ...,  C7  is  an 
\(»(ap)/         \«  ^  »/ 

llows   by   the    general    theorem,   that    if   the  characteristic 
be  added  to  each  of  0^  ...,  C7,  and  then  the  linear  transformation  given  by  the 


FIG.  12. 

then  the  characteristics  associated  with  the  half-periods  ua>  °l,  ua>  a\  ...,  ua>  Cp,  ua>  **", 
ua'  c  will  be,  save  for  integer  characteristics,  respectively  X1}  X2,  ...,  X2P,  X2P+1;  this  the 
reader  can  immediately  verify  by  means  of  the  rule  given  at  the  bottom  of  page  297  of  the 
present  volume. 

Ex.     Prove  that  if  the  characteristics  0,  Xj,....,  X2P  +  1  be  subjected  to  the  transforma 


tion  given  by  the  Abelian  matrix  of  2p  rows  and  columns  which  is  denoted  by 
then,  save  for  integer  characteristics,  Xf  is  changed  to  Si  +  ^f    J  ,  where 


1,  - 
0, 


iN /ov 

(0(o) 


332]  COMPOSITION    OF   TRANSFORMATIONS.  551 

are  the  characteristics  which  arise  in  §  200,  Chap.  XI.  as  associated  with  the  half-periods 
ua>Cr,  ua'ar,  ua'°  respectively.  The  characteristics  2n  ...,  22p  +  1  satisfy  the  p(2p-I) 
conditions  |  2(,  2/|  =  l,  for  i<j. 


332.  We  proceed  now  to  shew  how  any  linear  transformation  may  be 
regarded  as  the  result  of  certain  very  simple  linear  transformations  performed 
in  succession.  As  a  corollary  from  the  investigation  we  shall  be  able  to  infer 
that  every  linear  transformation  may  be  associated  with  a  change  in  the 
method  of  taking  the  period  loops  on  a  Riemann  surface  ;  we  have  already 
proved  the  converse  result,  that  every  change  in  the  period  loops  is  associated 
with  matrices,  a,  a',  /3,  /3',  belonging  to  a  linear  substitution  (§  322). 

It  is  convenient  to  give  first  the  fundamental  equations  for  a  composition 
of  two  transformations  of  any  order.  It  has  been  shewn  (§  324)  that  the 
equations  for  the  transformation  of  a  theta  function  of  the  first  order,  in  the 
arguments  u,  with  characteristic  (Q,  Q')  and  associated  constants  2eo,  2<u', 
277,  27;',  to  a  theta  function  of  order  r,  in  the  arguments  w,  where  u  =  Mw, 
with  characteristic  (K,  K'}  and  associated  constants  2v,  2v,  2£,  2f,  are 

K'  =  aQ'  -  a'Q  -  \d  (aa'),     -K  =  $Q'-  P'Q 

M,      0    \  /2u,  2iA  _  /2w,  2ftA  /a  , 
0,  rM-*J  fa  2(T/  ~  U?,  27/J  U', 


and  from  the  last  equation,  writing  it  in  the  form  /*U  =  OA,  it  follows,  in 
virtue  of  the  equations  OeH  =  -  ^Trie,  UeU'  =  —  ^irie  (§  140,  Chap.  VII.),  and 
the  easily  verifiable  equation  JLep  =  re,  where  the  matrix  e  is  given  by 


O  - 


that  also  AeA  =  re,  as  in  Ex.  i.,  §  324.  And,  just  as  in  §  324,  it  can  be  proved 
that  equations  for  the  transformation  of  a  theta  function  of  order  r  in  the 
arguments  w,  with  characteristic  (K,  K'),  and  associated  constants  2u,  2i/,  2f, 
2£',  to  a  theta-  function  of  order  rs,  in  the  arguments  u1}  given  by  w^Nu^, 
with  characteristic  (Ql9  Q/),  and  associated  constants  2o)!,  2ft)/,  27/j,  2?7/,  are 

Q/  =  yK'  -  y'K  -  %rd  (77  ),     -  &  =  8K'  -  I'K  - 

N,    _ 
0,  « 

and  writing  the  last  equation  in  the  form  vfli  =  UV,  we  infer  as  before  that 
^eV  =  se. 

Now  from  the  equations  /u,U  =  HA,  i/ni  =  UV,  we  obtain  //-i>ni=;u,UV  = 
or,  if  A!  =  AV, 


fMN,      _0_    \  /2ft),,  2&>A  =  /2ft),  2ft)'\      . 
V  0   ,  rtinSr-V  UT;,,  2r/1/)~U^,  2V/ 


552  SUPPLEMENTARY   TRANSFORMATIONS.  [332 

from  this  equation  we  find  as  before  that  the  matrix  A1}  given  by 


A  -AV- 

Al  -         -      '7  +  /3V, 

satisfies  the  equation  Aj  e  Aj  =  rse.     Similarly  from  the  two  sets  of  equations 
transforming  the  characteristics,  by  making  use  of  the  equations 


d  (aja/)  =  7<Z  (oa')  +  yd  (££')  +  rd  (77), 

d  (&&')  =  $d  (aa')  +  B'd  (££')  +  rd  (SS'),     (mod.  2), 

which  can  be  proved  by  the  methods  of  §  327,  we  immediately  find 

'),     -Q,=  M  -  fr'Q  -  \d  (&&'),     (mod- 


Hence  any  transformation  of  order  rs  may  be  regarded  as  compounded  of 
two  transformations,  of  which  the  first  transforms  a  theta-function  of  the 
first  order  into  a  theta  function  of  the  r-th  order,  and  the  second  transforms 
it  further  into  a  theta  function  of  order  rs. 

It  follows  therefore  that  the  most  general  transformation  may  be  con 
sidered  as  the  result  of  successive  transformations  of  prime  order.  It  is 
convenient  to  remember  that  the  matrix  of  integers,  A1?  associated  with 
the  compound  transformation,  is  equal  to  AV,  the  matrix  A,  associated 
with  the  transformation  which  is  first  carried  out,  being  the  left-hand 
factor. 

One  important  case  should  be  referred  to.     The  matrix 


is  easily  seen  to  be  that  of  a  transformation  of  order  r  ;  putting  it  in  place  of  y,  the  final 
equations  for  the  compound  transformation  Vi  may  be  taken  to  be 


The  transformation  rA~:  is  called  supplementary  to  A  (cf.  Chap.  XVII.,  §  317,  Ex.  vii.). 

333.     Limiting  ourselves  now  to  the  case  of  linear  transformation,  let 
AK  (k  =  2,  3,  .  .  .  ,  p)  denote  the  matrix  of  2p  rows  and  columns  indicated  by 

^*  =  (A*t,    0   ), 
0,  /** 

where  fj,k  has  unities  in  the  diagonal  except  in  the  first  and  &-th  places,  in 
which  there  are  zeros,  and  has  elsewhere  zeros,  except  in  the  &-th  place  of 
the  first  row,  and  the  k-ih  place  of  the  first  column,  where  there  are  unities  ; 
let  J9  denote  the  matrix  of  *2p  rows  and  columns  indicated  by 


333] 


FOUR   ELEMENTARY   LINEAR   TRANSFORMATIONS. 


553 


0 

which  has  unities  in  the  diagonal,  except  in  the  first  and  (p  +  l)-th  places, 
where  there  are  zeros,  and  has  elsewhere  zeros  except  in  the  (p  +  l)-th  place 
of  the  first  row,  where  there  is  —  1,  and  the  (p  +  l)-th  place  of  the  first 
column,  where  there  is  + 1 ;  let  C  denote  the  matrix  of  2p  rows  and  columns 
indicated  by 


which  has  unities  everywhere  in  the  diagonal  and  has  elsewhere  zeros, 
except  in  the  (p  +  l)-th  place  of  the  first  row,  where  it  has  -  1 ;  let  D  denote 
the  matrix  of  2p  rows  and  columns  indicated  by 

D  =  (l  0-1          ), 

1  -1      0 

1  0 

1  0 

0  1 

0  1 

0  1 

0  1 

which  has  unities  everywhere  in  the  diagonal  and  has  elsewhere  zeros,  except 
in  the  (p  +  2)-th  place  of  the  first  row  and  the  (p  +  l)-th  place  of  the  second 
row,  in  each  of  which  there  is  —  1.  It  is  easy  to  see  that  each  of  these 
matrices  satisfies  the  conditions  (IX.)  of  §  324,  for  r  =  1. 

Then  it  can  be  proved  that  every  matrix  of  2p  rows  and  columns  of 
integers, 

a , 

«', 


554 


ANY   LINEAR   TRANSFORMATION    OBTAINABLE 


[333 


for  which  aft  =  fta,  a'  ft'  =  ft'a,  aft'  —  @a?  =  1,  can  be  written*  as  a  product  of 
positive  integral  powers  of  the  (p  +  2)  matrices  AZ)  ...,  Ap,  B,  C,  D.  The 
proof  of  this  statement  is  given  in  the  Appendix  (II)  to  this  volume. 

We  shall  therefore  obtain  a  better  understanding  of  the  changes  effected 
by  a  linear  transformation  by  considering  these  transformations  in  turn.  We 
have  seen  that  any  linear  transformation  may  be  considered  as  made  up  of 
two  processes,  (i)  the  change  of  the  fundamental  system  of  periods,  effected 
by  the  equations 

[<w]  =  coo.  +  co'a.',     [&>']  =  6>/3  +  aft', 
[77]  =  773  +  7/a',      [77']  =  7}  ft  +  rj'ft', 

(ii)  the  change  of  the  arguments,  effected  by  the  equation  u  =  Mw,  and 
leading  to 


of  these  we  consider  here  the  first  process.     Applying  the  equations  •}• 
[CD]  =  «oa  +  &>V,     [&>']  =  to/3  +  a)'  ft', 

respectively  for  the  transformations  Ak,  B,  C,  D,  we  obtain  the  following  results  : 
For  the  matrix  (Ak)  we  have 

[(i>r,i]  =  <0r,k,       [<0r,k]  =  Vr,i,       [<>>'r,i]  =  <0'r,k,       [a>'r,k]  =  <»'r,i,       0"  =  1,  2>   •  •  •  »  P)  > 

or,  in  words,  if  2a)r>i,  2&>'r>;  be  called  the  i-th  pair  of  periods  for  the  argument 
ur,  the  change  effected  by  the  substitution  A^  is  an  interchange  of  the  first 
and  A;-th  pairs  of  periods  —  no  other  change  whatever  being  made. 

When  we  are  dealing  with  p  quantities,  the  interchange  of  the  first  and  £-th  of  these 
quantities  can  be  effected  by  a  composition  of  the  two  processes  (i)  an  interchange  of  the 
first  arid  second,  (ii)  a  cyclical  change  whereby  the  second  becomes  the  first,  the  third 
becomes  the  second,  ...,  thep-th  becomes  the  Q»-l)-th,  and  the  first  becomes  the  p-tln. 
Such  a  cyclical  change  is  easily  seen  to  be  effected  by  the  matrix 


'0                             1 

^ 

1  0 

0 

ro 

0                            1 

1  0 

1  0. 

0 

X. 

0 

*  Other  sets  of  elementary  matrices,  by  the  multiplication  of  which  any  Abelian  matrix  can 
be  formed,  can  easily  be  chosen.  One  other  obvious  set  consists  of  the  matrices  obtained  by 
interchanging  the  rows  and  columns  of  the  matrices  Ak,  B,  C,  D. 

t  We  may  state  the  meaning  of  the  matrices  A*,  B,  C,  D  somewhat  differently  in  accordance 
with  the  property  remarked  in  Ex.  iii. ,  §  324. 


333]  BY   COMPOSITION   OF   THESE   FOUR.  555 

which  verifies  the  equations  (IX.)  §  324,  for  r=l.  Hence  the  matrices  A3,  ...,  Ap  can 
each  be  represented  by  a  product  of  positive  powers  of  the  matrices  E  and  Az.  Thereby 
the  (jo  +  2)  elementary  matrices  A2,  ...,  Ap,  B,  C,  D  can  be  replaced  by  only  5  matrices  E, 
Az,  B,  C,  D*. 

Considering  next  the  matrix  B  we  obtain 

[1  '  r     '      n  r          n  r     /      n  /  f*  ^  •*•>  ^>  •••>  ?^\ 

ft)nlj  =  ft)r)1,       |G>r,iJ=  —  Wr,i,       |wr,tj  =  <»r,ii       Lft)r(rJ  =  <wr,i,       I..  o  1, 

\1  —        Z,  .  .  .,  JP/ 

so  that  this  transformation  has  the  effect  of  interchanging  m.r>l  and  &>',.,  i> 
changing  the  sign  of  one  of  them  ;  no  other  change  is  introduced. 
The  matrix  G  gives  the  equation 

[w'r.i]  =  0>'r,i  -  «r,i,       (r  =  1,  2,   .  .  .  ,  p), 

but  makes  no  other  change. 

The  matrix  D  makes  only  the  changes  expressed  by  the  equations 

[«•>,  1]  =  w  'r,  i  —  d>r,  2  ,       [w'r,  2]  =  <u'r,  2  ~  &>r,  i  • 

In  applying  these  transformations  to  the  case  of  the  theta  functions  we 
notice  immediately  that  A^,  C  and  D  all  belong  to  the  case  considered  in 
§  326  (ii),  in  which  the  matrix  a  =  0. 

Thus  in  the  case  of  the  transformation  A^  we  have 


where  w  differs  from  u  only  in  the  interchange  of  u^  and  uk,  T  differs  from  r 
only  in  the  interchange  of  the  suffixes  1  and  k  in  the  constituents  Tr>s  of  the 
matrix  T,  and  K,  K'  differ  from  Q,  Q'  only  in  the  interchange  of  the  first  and 
&-th  elements  both  in  Q  and  Q'.  Thus  in  this  case  the  constant  A  is  equal 
to  1. 

In  the  case  of  the  matrix  (C),  the  equations  of  §  326  (2)  give 


where 

u-w,  T'=T  save  that  r\tl=Tltl-I,  and  K'=Q',  K=Q  save  that  Ki  =  Ql 

now  the  general  term  of  the  left-hand  side,  or 


is  equal  to 

r'  (n+K')*+iir 


_  g-tV  (Q,'2-  Q,')  e2wiw  (n+K')+iirr'(n+K"Jf>+2niK(n+K')  . 

thus  in  the  case  of  the  transformation  (C)  the   constant   A   is    equal    to 
g-i><Q,"-Q,')  ;  wnen  Q/  is  a  half-integer,  this  is  an  eighth  root  of  unity. 

*  See  Krazer,  Ann.  d.  Mat.,  Ser.  n.,  t.  xii.  (1884).  The  number  of  elementary  matrices  is 
stated  by  Burkhardt  to  be  further  reducible  to  3,  or,  in  case  p  =  2,  to  2;  Getting.  Nachrichten 
1890,  p.  381. 


556  DETERMINATION   OF   THE   CONSTANT   FACTOR  [333 

In  the  case  of  the  matrix  (D),  the  equations  of  §  326  (ii)  lead  to 


where  u  =  w,  r  —r  save  that  r'1)2  =  rli2  —  1,  r'2)i  =  r2)1  —  1,  and  K'  =  Q',  K  =  Q 
save  that  Kl  =  Q1  +  Q2',  Kz  =  Q2  +  Q/  ;  now  we  have 


riK  (n+K1) 


thus,  in  the  case  of  the  matrix  (D)  the  constant  A  is  equal  to  e~ZiriQi'Q*. 

We  consider  now  the  transformation  (B)  —  which  falls  under  that  con 
sidered  in  (i)  §  326.  In  this  case  Trio.'  (a  +  TO?)  wz  is  equal  to  irirltl  w-?,  and 
the  equation  (a  +  TO?)  r  =  J3  +  r/3'  leads  to  the  equations 


or,  the  equivalent  equations  (?^,  s  =  2,  3,  .  .  .  ,  p), 

Iii  /it  _   /          ''/'. 

i.x  /T"  1,1>     ^"l,r  —        •,ttrl*1t\i    ^"r,8  —  *f,t       T  i,r  T  i,«/'r  i,i> 

also  WI  =  TI)IWI,  w;.  =  Tljr  Wj  +  wr,  so  that  Wj  =  —  r'^iMj,  wr  =  wr  —  r\>Tult  and 
Tl)1  Wj2  =  -  T'J,!  Mj2  ;  further  we  find 

K'  =  Q'  save  that  K,'  =-Ql,andK=Q  save  that  K-,  =  Q/  ; 
with  these  values  we  have  the  equation 


334.     To  determine  the  constant  A   in  the  final  equation  of  the  last 
Article  we  proceed  as  follows*  :  —  We  have 

ri 

(i)  e*wimwdw  =  0  or  1, 

Jo 

according  as  m  is  an  integer  other  than  zero,  or  is  zero  ; 

(ii)     if  a  be  a  positive  real  quantity  other  than  zero,  and  /9,  7,  8  be  real 
quantities, 


where  for  the  square  root  is  to  be  taken  that  value  of  which  the  real  part  is 
positive*f ; 

*  For  indications  of  another  method  consult  Clebsch  u.  Gordan,  Abel.  Funct.,  §  90;  Thomae, 
Crelle,  LXXV.  (1873),  p.  224. 

+  By  the  symbol  *J n,  where  /*  is  any  constant  quantity,  is  to  be  understood  that  square  root 
whose  real  part  is  positive,  or,  if  the  real  part  be  zero,  that  square  root  whose  imaginary 
part  is  positive. 


335]  FOR  THESE   FOUR   TRANSFORMATIONS.  557 

(iii)  with  the  relations  connecting  u,  w  and  r,  r'  given  in  the  previous 
Article, 

un  =  (wn\  +  (T!,  l  nt  + +  rlt  p  np)  wl , 

where  (wn\  denotes  W2n2  + +  wpnp ; 

(iv)  the  series  representing  the  function  ©  (w,  T')  is  uniformly  con 
vergent  for  all  finite  values  of  wlt  ...,  wp,  and  therefore,  between  finite  limits, 
the  integral  of  the  function  is  the  sum  of  the  integrals  of  its  terms. 

Therefore,  taking  the  case  when  (?')  and  therefore  (j£')  are  (°),  and 
integrating  the  equation 

in  regard  to  Wi,  ... ,  wp,  each  from  0  to  1,  we  have 

oo  —  oo,  oo      rl  rl 

Ao=nl=-«,n^,nl,L'"he7>  n*dw1...dwp, 

where,  on  the  right  hand,  the  integral  is  zero  except  for  n2  =  0,  . . . ,  np  =  0 ; 
thus 

oo  rl 

n,=  -oo  Jo 

v      f1  i2 

M1=-oo  JO 
J  —ao 

hence  since  the  real  part  of  irirltl  is  negative  (§  174),  we  have 

A          l^  I  * 

0  =  A/        :      =  A/  — ' 

v        7rirltl       v    rlfl 

where  the  square  root  is  to  be  taken  of  which  the  real  part  is  positive. 
Hence 


e»ir.,.wi«®(M;  T)  =  A@(w;  T')f 

V  T1>a 

and  from  this  equation,  by  increasing  w  by  K+r'K ,  we  deduce  that 

er*TIllWl«0(M;    T     Q')=         /J.^.riQ.Q,'©^;     T'     ^ 

Hence,  when  the  decomposition  of  any  linear  transformation  into  trans 
formations  of  the  form  Ak,  B,  C,  D  is  known,  the  value  of  the  constant 
factor,  A,  can  be  determined. 

335.  But,  save  for  an  eighth  root  of  unity,  we  can  immediately  specify  the  value  in 
the  general  case ;  for  when  Q,  $  are  zero,  the  value  of  the  constant  A  has  been  found  to 
be  unity  for  each  of  the  transformations  Ak,  C,  D,  and  for  the  transformation  B  to  have  a 


558     THE  CONSTANT  FACTOR  FOR  ANY  LINEAR  TRANSFORMATION.    [335 

value  which  is  in  fact  equal  to  *Ji/\M\,  \M\  denoting  the  determinant  of  the  matrix  M. 
Hence  for  a  transformation  which  can  be  put  into  the  form 


,  .........  ......  .... 

a'  £7  *  * 

if  the  values  of  the  matrix  M  for  these  component  transformations  be  respectively 

...M^...\...\...M^..  .!...!..., 
the  value  of  the  constant  A,  when  Q,  ty  are  zero,  for  the  complete  transformation,  will  be 


but  if  the  complete  transformation  give  u  =  Mw,  we  have  M=...M2M1...;   thus,  for  any 
transformation  we  have  the  formula 


\M\ 

where  M=a  +  ra,  u  =  Mw,  and  e  is  an  eighth  root  of  unity,  r,  r  being  as  in  §  328,  p.  544. 
Putting  2o>M,  2vw  for  u,  w,  as  in  §  326,  this  equation  is  the  same  as 

3  (u  ;  2»,  2»',  2V,  2,')=    7===  *  U  5  2u,  2«',  2f,  2f  '  |          fl 

/J 


V|* 


where  |  o>  |  is  the  determinant  of  the  matrix  w,  etc. 

Of  such  composite  transformations  there  is  one  which  is  of  some  importance,  that, 
namely,  for  which 


so  that 
Then 


We  may  suppose  this  transformation  obtained  from  the  formula  given  above  for  the 
simple  transformation  B — thus— Apply  first  the  transformation  B  which  interchanges 
•"mi  «'r,i  with  a  certain  change  of  sign  of  one  of  them;  then  apply  the  transformation 
A 2BA2  which  effects  a  similar  change  for  the  pair  <or)2,  a>'r>2  •  then  the  transformation 
A3£A3,  and  so  on.  Thence  we  eventually  obtain  the  formula 


Q 

where 


t                                        T    -i     a  ..                       .  T     o    o 

—J  —  I»ji  'f  /  &t   Q 

T  2,  2  —  T2,  2                  )  r    .3,  3  —  T  3,  3  ~i         >  •  •  •  > 

Tl,  1  T  2,  2 


and,  save  for  an  eighth  root  of  unity, 

/~*~      / '~~i~      /    i~  1 

where  |T|  is  the  determinant  of  the  matrix  T. 


336]        ELEMENTARY  TRANSFORMATIONS  OF  PERIOD  LOOPS.         559 

The  result  can  also  be  obtained  immediately,  and  the  constant  obtained  by  an  integra 
tion  as  in  the  simple  case  of  the  transformation  B ;  we  thus  find,  for  the  value  of  the 

constant  here  denoted  by  x/        x/  ~  ...,  the  integral* 

v   Ti,  i   v   T  2, 2 

r ...  r  e™x*dxi---dxP- 

J    -CO  J    _CO 

^!r.  i.     Prove  that  another  way  of  expressing  the  value  of  this  integral  is 

4tStan-i\r    . 
e     r=i  /V|TTO|, 

where,  if  the  matrix  T  be  written  p  +  icr,    TTO|  is  the  determinant  of  the  matrix  p2  +  o-2, 
which  is  equal  to  the  square  of  the  modulus  of  the  determinant  of  the  matrix  T,  also 
A!,  ...,  \p  are  the  (real)  roots  of  the  determinantal  equation  \p-\a-\  =  0,  and  tan"1  Ar  lies 
between  -  7r/2  and  w/2.     Of  the  fourth  root  the  positive  real  value  is  to  be  taken. 
Ex.  ii.     For  the  case  p  =  1,  the  constant  for  any  linear  transformation  is  given  by 


according  as  a  or  a'  is  odd ;  where  a  is  positive,  and 

'       i          /  7r^a'  •>      I        «• 

as  —  a  S  —  aa  ,        T       —. —  «2      /          i 

L  =  e*<>-     \/ /  • 


336.  Returning  now  to  consider  the  theory  more  particularly  in  con 
nexion  with  the  Riemann  surface,  we  prove  first  that  every  linear  trans 
formation  of  periods  such  as 

[to]  =  toot  +  6>V,     [a/]  =  w/3  +  to'/S', 
where 

a£-£o  =  0,     «'£'  -  £'a'  =  0,     a0'-/3a'  =  l, 

can  be  effected  by  a  change  in  the  manner  in  which  the  period  loops  are 
taken.  For  this  it  is  sufficient  to  prove  that  each  of  the  four  elementary 
types  of  transformation,  Ak,  B,  G,  D,  from  which,  as  we  have  seen,  every 
such  transformation  can  be  constructed,  can  itself  be  effected  by  a  change  in 
the  period  loops. 

The  change  of  periods  due  to  substitutions  Ak  can  clearly  be  effected 
without  drawing  the  period  loops  differently,  by  merely  numbering  them 

*  Weber  has  given  a  determination  of  the  constant  A  for  a  general  linear  transformation  by 
means  of  such  an  integral,  and  thence,  by  means  of  multiple-Gaussian  series.  See  Crelle,  LXXIV. 
(1872),  pp.  57  and  09. 


560 


ELEMENTARY    TRANSFORMATIONS. 


[336 


differently — attaching  the  numbers  1,  k  to  the  period-loop-pairs  which  were 
formerly  numbered  k  and  1.  No  further  remark  is  therefore  necessary  in 
regard  to  this  case. 

The  substitution  B,  which  makes  only  the  change  given  by 

[Q)ri  J  =  ft)',.,  j  ,         [ft/ r,  i]  =  -  ft),.,  !  , 

can  be  effected,  as  in  §  320,  by  regarding  the  loop  (6j)  as  an  \a^\  loop,  with 
retention  of  its  positive  direction ;  thus  the  direction  of  the  (old)  loop  (a^), 
which  now  becomes  the  [6J  loop,  will  be  altered ;  the  change  is  shewn  by 
comparing  the  figure  of  §  18  (p.  21)  with  the  annexed  figure  (13). 


FIG.  13. 


The  change,  due  to  the  substitution  G,  which  is  given  by 

[**  r,  i]  =  to'r,  1  ~  Mr,  i  > 

is  to  be  effected  by  drawing  the  loop  [aj  in  such  a  way  that  a  circuit  of  it 
(which  gives  rise  to  the  value  [2ft/r,i]  for  the  integral  ur)  is  equivalent  to  a 
circuit  of  the  original  loop  («j)  taken  with  a  circuit  of  the  loop  (6j)  from  the 
positive  to  the  negative  side  of  the  original  loop  (a^. 

This  may  be  effected  by  taking  the  loop  [aj  as  in  the  annexed  figure  (14) 
(cf.  §  331). 


FIG.  14. 


For  the  transformation  D  the  only  change  introduced  is  that  given  by 

[ft)'r,  i]  =  ft>'r,  i  —  &>r,  2 >       [o>'r,  2]  =  «'»•,  2  ~  <»>•,  1 , 

and   this  is   effected  by  drawing  the  loops   \a^\,  [a2],  so  that  a  circuit  of 


337] 


OF   PERIOD   LOOPS. 


561 


[«j]  is  equivalent  to  a  circuit  of  the  (original)  loop  (a^  together  with  a 
circuit  of  (62),  in  a  certain  direction,  and  similarly  for  [a2].  This  may  be 
done  as  in  the  annexed  diagram  (Fig.  15). 


FIG.  15. 

For  instance  the  new  loop  [«2]  in  this  diagram  (Fig.  15)  is  a  deformation  of  a  loop 
which  may  be  drawn  as  here  (Fig.  16) ; 


FIG.  16. 

since  the  integrand  of  the  Abelian  integral  ur  is  single-valued  on  the  Riemann  surface, 
independently  of  the  loops,  the  doubled  portion  from  L  to  M  is  self-destructive ;  and 
a  circuit  of  this  new  loop  [a2]  gives  w'r>  2  -  a>r>  j ,  as  desired. 

Hence  the  general  transformation  can  be  effected  by  a  composition  of  the 
changes  here  given.  It  is  immediately  seen,  for  any  of  the  linear  transform 
ations  of  §  326,  that  if  the  arguments  there  denoted  by  Ult  ...,  Up  be  a  set 
of  normal  integrals  of  the  first  kind  for  the  original  system  of  period  loops, 
then  Wlt  ...,  Wp  are  a  normal  set  for  the  new  loops  associated  with  the 
transformation. 

337.     Coming  next  to  the  question  of  how  the  theory  of  the  vanishing  of 
the  Riemann  theta  function,  which  has  been  given  in  Chap.  X.,  is  modified 
B.  36 


562  TRANSFORMATION   OF   THE   PLACES   TO1}  ...,mp.  [337 

by  the  adoption  of  a  different  series  of  period  loops,  we  prove  first  that  when 
a  change  is  made  equivalent  to  the  linear  transformation 

[eo]  =  <ya  +  a/a',      [a/]  =  &>/3  +  &//3', 

the  places  m^,  ...,  mp  of  §  179,  Chap.  X.,  derived  from  any  place  TO,  upon 
which  the  theory  of  the  vanishing  of  the  theta  function  depends,  become 
changed  into  places  TO/,  .  .  .  ,  mp'  which  satisfy  the  p  equations 

)],  +  J  T;,  ,  [d  («'£')]!  +...  +  lriip[d 


wherein  tt1}  ...,  t*p  denote  the  normal  integrals  of  the  first  kind  for  the 
original  system  of  period  loops. 

For  let  w1}  ...,wp  be  the  normal  integrals  of  the  first  kind  for  the  new 
period  loops,  and  let  TO/,  .  .  .  ,  mp  be  the  places  derived  from  the  place  TO,  in 
connexion  with  the  new  system  of  period  loops,  just  as  m1}  ...,  mp  were 
derived  from  the  original  system.  In  the  equation  of  transformation 


e*ia'  ,a+ra)  vfi  <H)  ;    T  =  A,®  (w  J    T'), 

put 


=  Wx'm  — 


so  that  the  right-hand  side  of  the  equation  vanishes  when  x  is  at  any  one  of 
the  places  TO/,  ...,  mp;  then  we  also  have 


u  = 
hence  the  function 


f  ,  ;    3  ( 
l^(a/5)J 


vanishes  when  x  is  at  any  one  of  the  places  acl)  ...,  xp\  therefore,  by  a 
proposition  previously  given  (Chap.  X.,  §  184  (X.)),  the  places  TO/,  ...,  TO/ 
satisfy  the  equivalence  stated  above. 

It  is  easy  to  see  that  this  equivalence  may  be  stated  in  the  form 


It  may  be  noticed  also  that,  of  the  elementary  transformations  associated 
with  the  matrices  Ak,  B,  C,  D,  of  §  333,  only  the  transformation  associated 
with  the  matrix  C  gives  rise  to  a  change  in  the  places  mlf  ...,  mp\  for  each 
of  the  others  the  characteristic  [^d(a/3),  ^d(ct'/3')]  vanishes. 

338.  From  the  investigation  of  §  329  it  follows,  by  interchanging  the 
rows  and  columns  of  the  matrix  of  transformation,  that  a  linear  trans- 


339]  CHARACTERISTICS  OF   RADICAL   FUNCTIONS.  563 


formation   can   be   taken   for   which    the   characteristic    [^d  (ot/3),  |d 
represents  any  specified  even  characteristic;  thus  all  the  2p-1(2p  +  1)  sets*, 


/,  ...,  mp',  which  arise  by  taking  the  characteristic  Jrj  in  the  equivalence 


to  be  in  turn  all  the  even  characteristics,  can  arise  for  the  places  w/,  .  .  .  ,  mp'. 
In  particular,  if  ^fi^  M<  be  an  even  half-period  for  which  0  (i^M,  /*)  vanishes, 
we  may  obtain  for  w/,  ...,  mp'  a  set  consisting  of  the  place  m  and  p-l 
places  ??/,  ...,  n'p_i,  in  which  w/,  ...,  yi'^-j  are  one  set  of  a  co-residual  lot  of 
sets  of  places  in  each  of  which  a  ^-polynomial  vanishes  to  the  second  order 
(cf.  Chap.  X.,  §  185). 

Ex.  If  in  the  hyperelliptic  case,  with  jt>  =  3,  the  period  loops  be  altered  from  those 
adopted  in  Chap.  XI.,  in  a  manner  equivalent  to  the  linear  transformation  given  in  the 
Example  of  §  329,  the  function  e  (w  ;  T'),  denned  by  means  of  the  new  loops,  will  vanish 
for  w  =  0;  and  the  places  mx',  m2',  m3',  arising  from  the  place  a  (§  203,  Chap.  XL),  as 
mlf  ...,mp  arise  from  m  in  §  179,  Chap.  X.,  will  consist  t  of  the  place  a  itself  and  two 
arbitrary  conjugate  places,  z  and  ~z. 

339.  We  have,  on  page  379  of  the  present  volume,  explained  a  method 
of  attaching  characteristics  to  root  forms  V.X(1),  VF(3)  ;  we  enquire  now  how 
these  characteristics  are  modified  when  the  period  loops  are  changed.  It  will 
be  sufficient  to  consider  the  case  of  VF(3)  ;  the  case  of  */Xw  arises  (§  244)  by 
taking  <f>0*/Xw  in  place  of  VF(3).  Altering  the  notation  of  §  244,  slightly,  to 
make  it  uniform  with  that  of  this  chapter,  the  results  there  obtained  are  as 
follows  ;  the  form  X®  is  a  polynomial  of  the  third  degree  in  the  fundamental 
^-polynomials,  which  vanishes  to  the  second  order  in  each  of  the  places 
Alt  ...,  Azp-3,  ml,  ...,  mp,  where  A1}  ...,  A2p_3  are,  with  the  place  m,  the 
zeros  of  a  ^-polynomial  <£0;  the  form  F(3)  is  a  polynomial,  also  of  the  third 
degree  in  the  fundamental  ^-polynomials,  which  vanishes  to  the  second  order 
in  each  of  the  places  A1}  ...,  Azp_3,  fj,1,  ...,  /^;  if 


g/T<ll+...+2P/TiiJ,),     (i  =  1,2,.  ..,|>), 
where  ul}  ...,  up  are  the  Riemann  normal  integrals  of  the  first  kind,  the 
characteristic  associated  with  the  form  F(3)  is  that  denoted  by  £K  J  ;   andj 

it  may  be  defined  by  the  fact  that  the  function  \/F(3)/VZ(3),  which  is  single- 
valued  on  the  dissected  Riemann  surface,  takes  the  factors  (—  I)?.',  (—  1)?« 
respectively  at  the  t'-th  period  loops  of  the  first  and  second  kind. 

Take  now  another  set  of  period  loops  ;    let  m/,  .  .  .  ,  mp    be  the  places 

*  Or  lot  of  sets,  when  the  equivalence  has  not  an  unique  solution. 
t  Cf.  the  concluding  remark  of  §  185. 
t  Integer  characteristics  .being  omitted. 

36—2 


564  TRANSFORMATION   OF   THE   CHARACTERISTICS  [339 

which,  for  these  loops,  arise  as  ??ij,  ...,  mp  arise  for  the  original  set  of  period 
loops;  let  Z{s)  be  the  form  which,  for  the  new  loops,  has  the  same  character 
as  has  the  form  X(*}  for  the  original  loops,  so  that  Z®  vanishes  to  the  second 
order  in  each  of  Al}  ...,  A2p-3>  m/,  ...,  mp  ;  then  from  the  equivalences 
(§  337) 

*'  mp  s  *  [d  (0/3%  +  K<,i  [d  (fiaOl  +  •  •  •  +  i  r  it  p  (d  (aa')]p, 


where  wlt  ...,  wp  are  the  normal  integrals  of  the  first  kind,  it  follows,  as  in 
§  244,  that  the  function  V/£(3)  /VJT(3)  is  single-valued  on  the  Riemann  surface 
dissected  by  the  new  system  of  period  loops,  arid  at  the  r-th  new  loops, 
respectively  of  the  first  and  second  kind,  has  the  factors 

e-iri[d  (oa'(  ~\r        Qiri  [d  (J3|3')  ],._ 

The  equations  of  transformation, 

[<w]  =  &)«  +  &>V,     [&>']  =  w/3  +  o)'/3', 
of  which  one  particular  equation  is  that  given  by 


express  the  fact  (cf.  §  322)  that  a  negative  circuit  of  the  new  loop  [br]  is 
equivalent  to  ai>r  negative  circuits  of  the  original  loop  (bi)  and  di<r  positive 
circuits  of  the  original  loop  (o^)  ;  thus  a  function  which  has  the  factors  e~™qt, 
e^i  at  the  i-th  original  loops,  will  at  the  r-th  new  loop  [ar]  have  the  factor 
e—*Ur  \  where  lr'  is  an  integer  which  is  given  by 

-  lr'  =  S  [-  qi  «i,  r  +  qt  <*'i,  r],          (mod.  2)  ; 

i=l 

thus  the  factors  of  VF(3)/VX(3)  at  the  new  period  loops  are  given  by  e~vil/, 
e1"1,  where  I,  I'  are  rows  of  integers  such  that 

I'  =  aq'  -  a'q,     -l  =  J3qf-  ft'q,         (mod.  2). 


Therefore  the  factors  of  \iT®/^Z1®  =  (VF^Vl/^^/VZ^Xat  the 
new  period  loops,  are  given  by  e~irik>,  e™*,  where 

k'  =  aq'  -aq-d  (aax),     -k  =  P<f-ffq-d  (yS/97),         (mod.  2)  ; 

now  the  characteristic  associated  with  VF(3)   corresponding  to  the  original 
system  of  period  loops  may  be  defined  by  the  factors  of  VF(3)/VjT<3>  at  those 

loops;  similarly  the  characteristic  which  belongs  to  VF(3)  for  the  new  system 

_        _  /£'\ 

of  loops  is  defined  by  the  factors  of  \/F(3)  /*JZ®,  and  is  therefore  if.,);  the 

equations  just  obtained  prove  therefore  that  the  characteristic  associated  with 
VF(3)  is  transformed  precisely  as  a  theta  characteristic. 


340]  OF   RADICAL   FUNCTIONS.  565 

The  same  result  may  be  obtained  thus  ;  the  p  equations  of  the  form 


are  immediately  seen,  by  means  of  the  equation  (a  +TO.')  (&'  —  r'd')  =  1  to  lead  to  p  equations 
expressible  by 

if"  m'  4-  .  .  . 


subtracting  from  these  the  equations 

(i=},..., 


we  obtain  equations  from  which  (as  in  §  244)  the  characteristic  of  V  'F<3>,  for  the  new 
loops,  is  immediately  deducible. 

Similar  reasoning  applies  obviously  to  the  characteristics  of  the  forms 
considered  on  page  380  (§  245).  But  the  characteristic  for  a  form 
(p.  381),  which  is  obtained  by  consideration  of  the  single-valued 
function  ^JT***/^W  —  into  which  the  form  *JX®,  depending  on  the  places 
m1)  ...,  mp,  does  not  enter  —  is  transformed  in  accordance  with  the  equations 

k'  =  aq  -aq,     -k  =  J3q'  -  J3'q,     (mod.  2), 
and  may  be  described  as  &  period-  characteristic,  as  in  §  328. 

340.  Having  thus  investigated  the  dependence  of  the  characteristics 
assigned  to  radical  forms  upon  the  method  of  dissection  of  the  Riemann 
surface,  it  is  proper  to  explain,  somewhat  further,  how  these  characteristics 
may  be  actually  specified  for  a  given  radical  form.  The  case  of  a  form 
\/Jf  w  differs  essentially  from  that  of  a  form  VJT(2"+1>.  When  the  zeros  of  a 
form  \fX(<i>i)  are  known,  and  the  Riemann  surface  is  given  with  a  specified 


system  of  period  loops,  the  factors  of  a  function  VX(a't)/3>('t)  at  these  loops 
may  be  determined  by  following  the  value  of  the  function  over  the  surface, 
noticing  the  places  at  which  the  values  of  the  function  branch  —  which  places 
are  in  general  only  the  fixed  branch  places  of  the  Riemann  surface  ;  the 
process  is  analogous  to  that  whereby,  in  the  case  of  elliptic  functions,  the 


values  of  Vp  (u  +  2^)  -  ^  /  \/p  (u)  -  el  ,  Vp  (u  +  2&>o)  -  ej^p  (u)  -  ^  may  be 


determined,  by  following  the  values  of  Vp  (u)  -  el  over  the  parallelogram  of 
periods.  But  it  is  a  different  problem  to  ascertain  the  factors  of  the  function 
\/F(3)/vAA>)  at  the  period  loops,  because  the  form  VZ(3)  depends  upon  the 
places  MI,  ...,  mp,  and  we  have  given  no  elementary  method  of  determining 
these  places  ;  the  geometrical  interpretation  of  these  places  which  is  given  in 
§  183  (Chap.  X.),  and  the  algebraic  process  resulting  therefrom,  does  not 
distinguish  them  from  other  sets  of  places  satisfying  the  same  conditions; 
the  distinction  in  fact,  as  follows  from  §  338,  cannot  be  made  algebraically 
unless  the  period  loops  are  given  by  algebraical  equations.  Nevertheless  we 


566  DETERMINATION    OF   THE    PLACES   m1}  ...,mp  [34-0 

may  determine  the  characteristic  of  a  form  F(3),  and  the  places  m^  ...,  mp, 
by  the  following  considerations*:  —  It  is  easily  proved,  by  an  argument  like 
that  of  §  245  (Chap.  XIII.),  that  if  there  be  a  form  VX(1)  having  the  same 
characteristic  as  \/F(3),  there  exists  an  equation  of  the  form  *JX(l]  \/F(3)  =  <E>(2)  ; 
and  conversely,  if  q  +  1  linearly  independent  polynomials,  of  the  second 
degree  in  the  p  fundamental  ^-polynomials,  vanish  in  the  zeros  of  VF(3),  and 
M^2*  denote  the  sum  of  these  q  +  1  polynomials,  each  multiplied  by  an 
arbitrary  constant,  that  we  have  an  equation  \/F(1)  \^F®»1!*',  where  VF(1)  is 
a  linear  aggregate  of  q  +  1  radical  forms  like  *JX(l),  all  having  the  same 
characteristic  as  VlT(s)  ;  in  general,  since  a  form  M^2'  can  contain  at  most 
3  (p  —  1)  linearly  independent  terms  (§  111,  Chap.  VI.),  and  the  number  of 
zeros  of  VF(3)  is  3  (p  —  1),  we  have  ^  +  1=0;  in  any  case  the  value  of  q  +  1 
is  capable  of  an  algebraic  determination,  being  the  number  of  forms  4>('2) 
which  vanish  in  assigned  places.  Now  the  number  of  linearly  independent 


forms  VjT(l)  with  the  same  characteristic  is  even  or  odd  according  as  the 
characteristic  is  even  or  odd  (§§  185,  186,  Chap.  X.)  ;  hence,  without  deter 
mining  the  characteristic  of  VF(3)  we  can  beforehand  ascertain  whether  it  is 
even  or  odd  by  finding  whether  q  +  1  is  even  or  odd.  Suppose  now  that 
fa,  ...,  fj,p  and  fa,  ...,  fjLp'  are  two  sets  of  places  such  that 


m  being  an  arbitrary  place,  and  m,  A1}  ...,  A2p_3  being  the  zeros  of  any 
^-polynomial  </>0  ;  so  that  /^  ,  .  .  .  ,  pp  and  /V,  •••>  /V  are  two  sets  arbitrarily 
selected  froni  2'2p  sets  which  can  be  determined  geometrically  as  in  §  183, 
Chap.  X.  (cf.  §  244,  Chap.  XIII.)  ;  let  F(3)  vanish  to  the  second  order  in  each 
of  yLtj,  ...,  /Ap,  A1}  ...,  A2p_3  and  F/3'  vanish  to  the  second  order  in  each  of 
pi>  •••,  Pp,  AI,  ...,  A2p_3;  by  following  the  values  of  the  single-valued 


function  VF^ys/F^  on  the  Riemann  surface,  we  can  determine  its  factors  at 
the  period  loops  ;  at  the  r-th  period  loops  of  the  first  and  second  kind  let 
these  factors  be  (—I)*'-',  (—  !)*'•  respectively;  then  if  ^(qit  ...,  <&,')  and 
2"  (Qi>  ••••  Qp)  be  respectively  the  characteristics  of  VF(3)  and  VF/3',  which  we 
wish  to  determine,  we  have  (§  244) 

krf  =  Qr'  -  qr',     kr  =  Qr  -  qr,     (mod.  2). 

Take  now,  in  turn,  for  /*/,  ...,  /A/,  all  the  possible  2^  sets  which,  as  in  §  183, 
are  geometrically  determinate  from  the  place  m;  and,  for  the  same  form 
VF(3),  determine  the  2'*  characteristics  of  all  the  functions  VF^'/VF*3'  arising 


*  Noether,  Jahresbericht  der  Deutschen  Mathematiber  Vereinigung,  Bd.  iii.  (1894),  p.  494, 
where  the  reference  is  to  Fuchs,  Crelle,  LXXIII.  (1871)  ;  cf.  Prym,  Zur  Theorie  der  Fumtionen  in 
einer  zweibldttrigen  Fldche  (Zurich,  1866). 


341]  WHEN   THE   PERIOD   LOOPS  ARE   GIVEN.  567 

by  the  change  of  the  forms  \f  Y^  ;    then  there  exists  one,  and  only  one, 

s'\ 
}  ,  satisfying  the  condition  that  the  characteristic 


_ 

is  even  when  VF/3'  has  an  even  characteristic  and  odd  when  VFj(3)  has  an  odd 

characteristic  ;  for,  clearly,  the  characteristic  \  (     1  is  a  value  for  \  (    ]  which 

\q  /  \s  / 

satisfies  the  condition,  and  if  i  I      I  were  another  possible  value  for  1-  (     1 

\<r  )  \s) 

we  should  have 

(k  +  o-)  (k'  +  </)  =  (k  +  q)(k  +  q')         (mod.  2), 
or 

k  (<r'  -  q)  +  k'  (<r-q)  =  qq'  -  <ra' 


for  all  the  22^  possible  values  of  |-    ,     ;  and  this  is  impossible  (Chap.  XVII., 

\fc  1 
§  295). 

Hence  we  have  the  following  rule  :  —  Investigate  the  factors  of  V  F^/V  F(3) 
for  an  arbitrary  form  V  F(3)  and  all  2^  forms  V  F^3'  ;  corresponding  to  each 
form  VFj'3'  determine,  by  the  method  explained  in  the  earlier  part  of  this 
Article,  whether  its  characteristic  is  even  or  odd  ;  then,  denoting  the  factors  of 
any  function  \/Fj(3)/v  F(3)  respectively  at  the  first  and  second  kinds  of  period 

loops  by  quantities  of  the  form  (—  !)*,(—  1)*,  determine  the  characteristic  M    ), 

satisfying  the  condition  that  the  characteristic  A-  (          ,  1  is,  for  every  form 

\    +  k  )  y  J 


j'3',  even  or  odd  according  as  the  characteristic  of  that  form,  VF/3',  is  even  or 
odd;  then  ^  (  }  is  the  characteristic  of  the  form  VF(3);  this  being  determined 

the  characteristic  of  every  form  VF^  is  known;  the  particular  form  ^Y^  for 
which  the  characteristic,  thus  arising,  is  actually  zero,  is  the  form  previously 
denoted  by  VZ(3>  —  namely  the  form  vanishing  in  the  places  ml}  ...,  mp  which  are 
to  be  associated  (as  in  §  179,  Chap.  X.)  with  the  particular  system  of  period 
loops  of  the  Riemann  surface  which  has  been  adopted. 

Thus  the  method  determines  the  places  m1}  ...,mp  and  determines  the 
characteristic  of  every  form  \/F(3);  the  characteristic  of  any  other  form 
v/F(2l/+1)  is  then  algebraically  determinable  by  the  theorems  of  §  245  (p.  380). 

341.  For  the  hyperelliptic  case  we  have  shewn,  in  Chap.  XL,  how  to 
express  the  ratios  of  the  2^  Riemann  theta  functions  with  half-integer 
characteristics  by  means  of  algebraic  functions  ;  the  necessary  modification 


568  APPLICATION   OF   THE  THEORY  [341 

of  these  formulae  when  the  period  loops  are  taken  otherwise  than  in 
Chap.  XL,  follows  immediately  from  the  results  of  this  chapter.  If  the 
change  in  the  period  loops  be  that  leading  to  the  linear  transformation 
which  is  associated  with  the  Abelian  matrix  formed  with  the  integer 
matrices  a,  /3,  a',  ft',  we  have  (§  324) 


where 

k'  =  aq'  -a'q-d  (aa'),     -  k  =  J3q'  -  0'q  - 

If  now,  considering  as  sufficient  example  the  formula  of  §  208  (Chap.  XL),  we 
have 

ur  a  =  ?l6)M  +  •"  +  <fpt°r,p  +  qi'w'r.i  +  »•  +  Qp'  O>r,p, 

then  we  have 

Wr'a=  llVr>1+  ...  +  lpVr,p  +  liVrtl  +  ...  +lpVfip, 

where 

l'  =  aq'-a'q  =  k'+d(aa'),     -  I  =  0q'  -  /3'q  =  -  k  +  d(W)  ; 

therefore,  if  the  characteristic  \  (d  (/9/3'),  d  (aa'))  be  denoted  by  p,  the  function 

&r  1  40  ;  £  (  ,  )  I   is  a  constant  multiple  of  ^x  \w  ;  \  (  ,  )  +  p    ;    and  we  may 
\/c  /  \  \*/ 

denote  the  latter  function  by  ^  [w\wb'a  +  fi\.     Thus  the  formula  of  §  208  is 
equivalent  to 

-  \  —  71  -  ~\      n  ^i  (w  I  w*'  a  +  /*) 
,...6-= 


where  C  is  independent  of  the  arguments  w1}  ...,  wp,  and,  as  in  §  206, 
Wr  =  <""'  +  .  ..  +  <"<**,         (r  =  1,2,..  .,/)). 

Similar  remarks  apply  to  the  formula  of  §§  209,  210.     It  follows  from 
§  337  that  the  characteristic  fj,  is  that  associated  with  the  half-periods 


where  m^,  ...,  mp'  are  the  places  which,  for  the  new  system  of  period  loops, 
play  the  part  of  the  places  ml}  ...,  mp  of  §  179,  Chap.  X.  It  has  already 
(§  337)  been  noticed  that  for  the  elementary  linear  substitutions  Ak,  B,  D  the 
characteristic  yu,  is  zero. 

342.     In  case  the  roots  clt  alt  ca,  «2>  •••>  c,  in  the  equation  associated  with 
the  hyperelliptic  case 

7/2  _  4  (x  _  Cj)  ^  _  tti)  ^  _  Cz)  (x  —  at)...(x-  Cp)  (x  -  Op)  (x  -  c), 

be  real  and  in  ascending  order  of  magnitude,  we  may  usefully  modify  the 
notation  of  §  200,  Chap.  XI.  Denote  these  roots,  in  order,  by  byp,  62p_i,  .  ..,  b0, 


342] 


TO   THE   HYPERELLIPTIC   THETA   FUNCTIONS. 


569 


so  that  bti,  byi-i  are  respectively  cp_t+i,  ap-i+i  and  b0  is  c,  and  interchange 
the  period  loops  (a;),  (£>;),  with  retention  of  the  direction  of  (&{),  as  in  the 
figure  annexed  (Fig.  17). 


FIG.  17. 


Then  if  U*'  a,  ...,  Ux<  a  are  linearly  independent  integrals  of  the  first  kind, 
such  that  dUxr'a  ldx  =  -^r/y,  where  tyr  is  an  integral  polynomial  in  x,  of  degree 
p  —  1  at  most,  with  only  real  coefficients,  the  half-periods 


are  respectively  real  and  purely  imaginary,  so  that  [a/,.,;]  is   also   purely 
imaginary  ;  if  now  w*'  a,  ...,  w^'  a  be  the  normal  integrals,  so  that 


then  the  second  set  of  periods  of  w*'a,  ...,  wx'a,  which  are  given  by 
T'r,i  =  Lr<l[2a>\!i]  +  ...+Lr>p[2a>'p>i],         (r,s=l,  2,  ...,p\ 

are  also  purely  imaginary*  ;  forming  with  these  the  theta  function  ®  (w  ;  T'), 
the  theta  function  of  Chap.  XI.  is  given  (§  335)  by 

e-in*  @  (u.  T   Q')  =  AeMQQ>  ®(w.r>\  -x)t 

where  K,  K'  are  obtainable  from  Q,  Q'  respectively  by  reversing  the  order 
of  the  p  elements,  and  A  is  the  constant  Vt/A7  Vt'Si/A^  Vt'A2/  A3  .  .  .  ,  in  which 
^  =  TI,I,  A2  =  T^T^  —  T21)2,  etc.  We  find  immediately  that 


(i  =  (),  1,  ....  p),  and  may  hence  associate  with  &„•_,,  62i  the  respective  odd  and 
even  characteristics 


vo;  v- 1 

*  The  quantities  rt.,  of  Chap.  XI.  (of  which  the  matrix  is  given  in  terms  of  the  r'<  of  §  342 
by  rr'  =  -  1)  are  also  purely  imaginary  when  c, ,  a,,  ...,  cp,  ap,  c  are  real  and  in  ascending  order 
of  magnitude. 


570  WEIERSTRASS'S   RULE.  [342 

and  may  denote  the  theta  functions  with  these  characteristics  respectively  by 
@2t-i(w;  T'),  ©«(w;  T');  if  bk,  blt  bm,  ...,  be  any  of  the  places  b.2p,  ...,  60,  not 
more  than  p  in  number,  and  if,  with  0  }>  qt  <  2,  0  >  g/  <  2,  we  have 


then  the  function  whose  characteristic  is  A-  (     *  J  may  be  denoted  by 

- 


This  function  is  equal  to,  or  equal  to  the  negative  of,  the  function  with 
characteristic  J  (     )  j  according  as  the  characteristic  is  even  or  odd. 


We  have  thus  a  number  notation  for  the  22p  half-integer  characteristics*, 
equally  whether  the  surface  be  hyperelliptic  or  not ;  this  notation  is  under 
stood  to  be  that  of  Weierstrass  (Kb'nigsberger,  Crelle,  LXIV.  (1865),  p.  20). 
For  the  numerical  definition  of  the  half-periods,  which  are  given  by  the  rule 
at  the  bottom  of  p.  297,  precise  conventions  are  necessary  as  to  the  allocation 
of  the  signs  of  the  single  valued  functions  V#  —  br  on  the  Riemann  surface 
(cf.  Chap.  XXII.). 

In  the  hyperelliptic  case  j»  =  2,  the  characteristics  of  the  theta  functions  given  in  the 
table  of  §  204  are  supposed  to  consist  of  positive  elements  less  than  unity ;  when  Q1 ,  Q2 , 
Qi,  Q2'  are  each  either  0  or  ^,  the  formula  of  the  present  article  gives 

«"*"•  9  \u  ;  r  \  y  Vl^Ae-MW  6  \w  ;  r' 

**1       %  J  I- 

the  number  notations  for  the  transformed  characteristics  are  then  immediately  given  by 
the  table  of  §  204.     The  result  is  that  the  numbers 

02,  24,  04,  1,  13,  3,  5,  23,  12,  2,  01,  0,  14,  4,  34,  03 
are  respectively  replaced  by 

3,  1,  13,  24,  04,  02,  5,  0,  4,  2,  34,  23,  14,  12,  01,  03. 

*  For  convenience  in  the  comparison  of  results  in  the  analytical  theory  of  theta  functions,  it 
appears  better  to  regard  it  as  a  notation  for  the  characteristics  rather  than  for  the  functions. 


344] 


CHAPTER    XIX. 

ON   SYSTEMS   OF  PERIODS   AND   ON   GENERAL   JACOBIAN   FUNCTIONS. 

343.  THE  present  chapter  contains  a  brief  account  of  some  general  ideas 
which  it  is  desirable  to  have  in  mind  in  dealing  with  theta  functions  in 
general  and  more  especially  in  dealing  with  the  theory  of  transformation. 

Starting  with  the  theta  functions  it  is  possible  to  build  up  functions 
of  p  variables  which  have  2p  sets  of  simultaneous  periods — as  for  instance 
by  forming  quotients  of  integral  polynomials  of  theta  functions  (Chap.  XL, 
§  207),  or  by  taking  the  second  differential  coefficients  of  the  logarithm  of 
a  single  theta  function  (Chap.  XL,  §  216,  Chap.  XVIL,  §  311  (8)).  Thereby 
is  suggested,  as  a  matter  for  enquiry,  along  with  other  questions  belonging  to 
the  general  theory  of  functions  of  several  independent  variables,  the  question 
whether  every  such  multiply-periodic  function  can  be  expressed  by  means  of 
theta  functions*.  Leaving  aside  this  general  theory,  we  consider  in  this 
chapter,  in  the  barest  outline,  (i)  the  theory  of  the  periods  of  an  analytical 
multiply-periodic  function,  (ii)  the  expression  of  the  most  general  single 
valued  analytical  integral  function  of  which  the  second  logarithmic  dif 
ferential  coefficients  are  periodic  functions. 

344.  If    an    uniform    analytical    function   of  p   independent   complex 
variables  ul}  ...,up  be  such  that,  for  every  set  of  values  of  u^,  ...,up,  it 
is  unaltered   by  the  addition,  respectively  to  u1}...,up,  of  the   constants 
PH  ...,  Pp,  then  Pj,  ...,  Pp  are  said  to  constitute  a  period  column  for  the 
function.     Such  a  column  will  be  denoted  by  a  single  letter,  P,  and  Pk  will 
denote  any  one  of  Plt  ...,  Pp.     It  is  clear  that  if  each  of  P,  Q,  R,  ...  be 
period  columns  for  the  function,  and  X,  p,  v,  ...  be  any  definite  integers, 
independent  of  k,  then  the  column  of  quantities  \Pk  +  (jbQk  +  vRk  +  ...  is 
also   a   period  column  for  the  function ;    we  shall  denote  this  column  by 
\P  +  pQ  +  vR+  ...,  and   say  that  it  is  a  linear  function  of  the  columns 
P,  Q,  R,  ...,  the  coefficients  X,  p,  v,  ...,  in  this  case,  but  not  necessarily 

*  Cf.  Weierstiass,  (Jrelle,  LXXXIX.  (1880),  p.  8. 


572  CONDITIONS   THAT   AN   UNIFORM   FUNCTION  [344 

always,  being  integers.  The  real  parts  of  the  new  column  are  the  same 
linear  functions  of  the  real  parts  of  the  component  columns,  as  also  are  the 
imaginary  parts.  More  generally,  when  the  p  quantities  XP*  +  pQk  +  vRk  +  •  •  • 
are  zero  for  the  same  values  of  X,  /JL,  v,  .  .  .  ,  we  say  that  the  columns  P,Q,R,... 
are  connected  by  a  linear  equation  ;  it  must  be  noticed,  for  the  sake  of 
definiteuess,  that  it  does  not  thence  follow  that,  for  instance,  P  is  a  linear 
function  of  the  other  columns,  unless  it  is  known  that  X  is  not  zero. 

It  is  clear  moreover  that  any  2p  +  l,  or  more,  columns  of  periods  are 
connected  by  at  least  one  linear  equation  with  real  coefficients  (that  is,  an 
equation  for  each  of  the  p  positions  in  the  column  —  p  equations  in  all,  with 
the  same  coefficients)  ;  for,  in  order  to  such  an  equation,  the  separation  of 
real  and  imaginary  gives  2p  linear  equations  to  be  satisfied  by  the  2p  4-  1 
real  coefficients  ;  allowing  possible  zero  values  for  coefficients  these  equations 
can  always  be  satisfied. 


For  instance  the  periods  Q  —  Qj^  +  iQ^,  o)  =  <a1  +  t<»2>  w'^wj'  +  iwg',  are  connected  by  an 
equation 


in  which  however,  if  a>1a>2'  —  ^ta^O,  also  £  =  0. 

Thus,  for  any  periodic  function,  there  exists  a  least  number,  r,  of  period 
columns,  with  r  lying  between  1  and  2p  +  1,  which  are  themselves  not 
connected  by  any  linear  equation  with  real  coefficients,  but  are  such  that 
every  other  period  column  is  a  linear  function  of  these  columns  with  real 
finite  coefficients.  Denoting  such  a  set*  of  r  period  columns  by  P(1),  ...,P(r), 
and  denoting  any  other  period  column  by  Q,  we  have  therefore  the  p 
equations 


XrP<r) 


wherein  X1?  ...,  Xr  are  independent  of  k,  and  are  real  and  not  infinite.  It  is 
the  purpose  of  wharf  follows  to  shew,  in  the  case  of  an  uniform  analytical 
function  of  the  independent  complex  variables  ult  ...,  up,  (I.)  that  unless  the 
function  can  be  expressed  in  terms  of  less  than  p  variables  which  are  linear 
functions  of  the  arguments  ul}  ...,  up,  the  coefficients  \ly  .  .  .  ,  X,.  are  rational 
numbers,  (II.)  that,  Xls  ...,X,.  being  rational  numbers,  sets  of  r  columns  of 
periods  exist  in  terms  of  which  every  existing  period  column  can  be  linearly 
expressed  with  integral  coefficients. 

Two  lemmas  are  employed  which  may  be  enunciated  thus  :  — 
(a)     If  an  uniform  analytical  function  of  the  variables  ult  ...,  up  have  a 
column  of  infinitesimal  periods,  it  is  expressible  as  a  function  of  less  than 
p  variables  which  are  linear  functions  of  w1,  ...,  up.     And  conversely,  if  such 

*  It  will  appear  that  the  number  of  such  sets  is  infinite  ;  it  is  the  number  r  which  is  unique. 
t  These    propositions   are  given   by   Weierstrass.      Abhandlungen  am  der  Functionenlehre 
(Berlin,  1886),  p.  165  (or  Berlin.  Monatsber.  1876). 


345]  HAVE   INFINITESIMAL   PERIODS.  573 

uniform  analytical  function  of  ul}  ...,  uv  be  expressible  as  a  function  of  less 
than  p  variables  which  are  linear  functions  of  ull  ...,  up,  it  has  columns  of 
infinitesimal  periods. 

(#)  Of  periods  of  an  uniform  analytical  function  of  the  variables 
•ult...,up,  which  does  not  possess  any  columns  of  infinitesimal  periods, 
there  is  only  a  finite  number  of  columns  of  which  every  period  is  finite. 

345.  To  prove  the  first  part  of  lemma  (a)  it  is  sufficient  to  prove  that 
when  the  function  f(ui,  ...,  up)  is  not  expressible  as  a  function  of  less  than 
p  linear  functions  of  ult  ...,  up,  then  it  has  not  any  columns  of  infinitesimal 
periods. 

We  define  as  an  ordinary  set  of  values  of  the  variables  ult  ...,up  a  set 
Ui,  ...,  up',  such  that,  for  absolute  values  of  the  differences  ut  —  «/,  ...,up  —  Up' 
which  are  within  sufficient  (not  vanishing)  nearness  to  zero,  the  function, 
/(MI,  ...,  Up),  can  be  represented  by  a  converging  series  of  positive  integral 
powers  of  these  differences  —  the  possibility  of  such  representation  being  the 
distinguishing  mark  of  an  analytical  function  ;  other  sets  of  values  of  the 
variables  are  distinguished  as  singular  sets  of  values*. 

Then  if  the  function  be  not  expressible  by  less  than  p  linear  functions  of 
«!,  ...,  Up,  there  can  exist  no  set  of  constants  d,  ...,  cp  such  that  the 
function 


vanishes  for  all  ordinary  sets  of  values  of  the  variables;  for  this  would 
require  /  to  be  a  function  of  the  p-l  variables  c^  -  c&i  (i  =  2,  ...,  p). 
Hence  there  exist  sets  of  ordinary  values  such  that  not  all  the  differential 
coefficients  df/du,,  ...,df(dup  are  zero;  let  <$\  ....u™  be  such  an  ordinary 
set  of  values;  for  all  values  of  «,,  ...,  up  in  the  immediate  neighbourhoods 
respectively  of  «,  ,  ...,  u™,  the  statement  remains  true  that  not  all  the  partial 
differential  coefficients  are  zero. 

Then,  similarly,  the  determinants  of  two  rows  and  columns  formed  from 
the  array 


dup 


do  not  all  vanish  for  every  ordinary  set  of  values  of  the  variables;    let 
*!,...,«*,  be  an  ordinary  set  for  which  they  do  not  vanish  ;  for  all  values  of 

*  The  ordinary  sets  of  values  constitute  a  continuum  of  2p  dimensions,  which  is  necessarily 
limited;   the  limiting  sets  of  values  are   the   singular   sets.     Of.   Weierstrass,  Crelle    LXXXIX 
1880       .  3. 


(1880),  p.  3. 


574  INFINITESIMAL   PERIODS.  [345 

ul}  ...,up  in  the  immediate  neighbourhoods  respectively  of  u? ,  ...,  U* ,  the 
statement  remains  true  that  not  all  these  determinants  are  zero. 

Proceeding  step  by  step  in  the  way  thus  indicated  we  infer  that  there  exist 
sets  of  ordinary  values  of  the  variables,  (ul\  ...,  u(p),  . . . ,  (u\p\  . . . ,  •z/jf)),  such 
that  the  determinant,  A,  of  p  rows  and  columns  in  which  the  k-ih  element  of 
the  r-th  row  is  df(u(i\  ...,  u^^/du^,  does  not  vanish;  and  since  these  are 
ordinary  sets  of  values  of  the  arguments,  this  determinant  will  remain 
different  from  zero  if  (for  r=l,  . ..,  p)  the  set  u(i\  ...,  u(p  be  replaced 
by  vf ,  ...,  Vp,  where  t^  is  a  value  in  the  immediate  neighbourhood  of 

(r) 

%• 

This  fact  is  however  inconsistent  with  the  existence  of  a  column  of 
infinitesimal  periods.  For  if  Hl}  ...,  Hp  be  such  a  column,  of  which  the 
constituents  are  not  all  zero,  we  have 


f    TT     J    r,,w  _L  A  TT  Jr)   .    a  77  1 

=  k=i       du  L  '  +    l    "  '"'    p  +  WW 

where  #1}  ...,  0p  are  quantities  whose  absolute  values  are  ^  1,  and  the 
bracket  indicates  that,  after  forming  df/duk,  we  are  (for  ra=l,  . ..,  p)  to 
substitute  urm  +  6mHm  for  u^ ;  these  p  equations,  by  elimination  of  Hl> ... ,  5^ 
give  zero  as  the  value  of  a  determinant  which  is  obtainable  from  A  by  slight 
changes  of  the  sets  u[ ,  ...,Up  ;  we  have  seen  above  that  such  a  determinant 
is  not  zero. 

To  prove  the  converse  part  of  lemma  (a)  we  may  proceed  as  follows. 
Suppose  that  the  function  is  expressible  by  m  arguments  vl}  ...,  vm  given  by 

Vk  =  aktlu1+  ...  +  akt pup,         (k  =  1,  . . .,  m), 

wherein  m< p.  The  conditions  that  v1}...,vm  remain  unaltered  when 
MI,  ...,  up  are  replaced  respectively  by  u1  +  tQi,  ...,  up  +  tQp  are  satisfied  by 
taking  Q1}  ...,  Qp  so  that 


and  since  m<p  these  conditions  can  be  satisfied  by  finite  values  of  Qlt  ...,QP 
which  are  riot  all  zero.  The  additions  of  the  quantities  tQi,...,tQp  to 
HI,  ...,up,  not  altering  vlt  ...,  vm,  will  not  alter  the  value  of  the  function  f. 
Hence  by  supposing  t  taken  infinitesimal ly  small,  the  function  has  a  column 
of  infinitesimal  periods. 

346.  As  to  lemma  (@),  let  Pk  =  pk  +  ia-k  be  one  period  of  any  column  of 
periods,  (k=I,  ...,  p),  wherein  pk,  <rk  are  real,  so  that,  in  accordance  with  the 
condition  that  the  function  has  no  column  of  infinitesimal  periods,  there 


347]  A   SYSTEM   OF   INDEPENDENT   PERIODS.  575 

is  an  assignable  real  positive  quantity  e  such  that  not  all  the  2p  quantities 
pk,  ak  are  less  than  e.  Then  if  fit,  vk  be  2p  specified  positive  integers, 
there  is  at  most  one  column  of  periods  satisfying  the  conditions 

<(/**+l)e,         vke$\<rk\<(vk  +  l)c,         (k  =  1,  ...,  p)  ; 


wherein  \pk\,  \<fk\  are  the  numerical  values  of  pk,  crk;  for  if  pk  +  i<rk  were 
one  period  of  another  column  also  satisfying  these  conditions,  the  quantities 
pk'  —  pk  -|-  {  (0-j/  _  o-j.)  would  form  a  period  column  wherein  every  one  of  the 
2p  quantities  pk  —  pk>  a-k  —  o~k  was  numerically  less  than  e. 

Hence,  since,  if  g  be  any  assigned  real  positive  quantity,  there  is  only  a 
finite  number  of  sets  of  2p  positive  integers  /jik,  vk  such  that  each  of  the 
2p  quantities  pke,  rke  is  within  the  limits  (—g,  g),  it  follows  that  there 
is  only  a  finite  number  of  columns  of  periods  Pk  =  pk  +  i(rk,  such  that  each  of 
pk,  <rk  is  numerically  less  than  g.  And  this  is  the  meaning  of  the  lemma. 

347.  We  return  now  to  the  expression  (§  344)  of  the  most  general 
period  column  of  the  function  /by  real  linear  functions  of  r  period  columns, 
of  finite  periods,  in  the  form 


here  the  suffix  is  omitted,  and  we  make  the  hypothesis  that  the  function 
is  not  expressible  by  fewer  than  p  linear  combinations  of  ult  ...,  up. 

Consider,  first,  the  period  columns  Q  from  which  X2  =  X3  =  ...  =  Xr  =  0 
and  0  <  A!  :}>  1.  Since  there  are  no  columns  of  infinitesimal  periods,  there 
is  a  lower  limit  to  the  values  of  \  corresponding  to  existing  period  columns 
Q  satisfying  these  conditions  ;  and  since  there  is  only  a  finite  number  of 
period  columns  of  wholly  finite  periods,  there  is  an  existing  period  for  which 
Xj  is  equal  to  this  lower  limit.  Let  Xltl  be  this  least  value  of  \1}  and  Q(1) 
be  the  corresponding  period  column  Q. 

Consider,  next,  the  period  columns  Q  for  which  X3  =  \4  —  .  .  .  =  Xr  =  0, 
and  O^-Xj^-l,  0  <  X-j  ^  1.  As  before  there  are  period  columns  of  this 
character  in  which  X2  has  a  least  value,  which  we  denote  by  X2)  2.  If  there 
exist  several  corresponding  values  of  X1}  let  X1)2  denote  one  of  these,  and 
denote  \1>2PW  +  X2)2P<2>  by  Q<2'. 

In  general  consider  the  period  columns  of  the  form 


wherein 


Since  there  are  no  infinitesimal  periods,  there  is  a  lower  limit  to  the  values 
of  \m  corresponding  to  existing  period  columns  satisfying  these  conditions  ; 
since  there  is  only  a  finite  number  of  period  columns  of  wholly  finite  periods, 
there  is  at  least  one  existing  column  Q  for  which  X™  is  equal  to  this  lower 


576  EXPRESSION    OF   ANY    PERIOD  [347 

limit;  denote  this  value  of  X™  by  Xm,w,  and  denote  by  X1(TO,  ...,  \m-i,m  values 
arising  in  an  actual  period  column  Q(w)  given  by 

Q<™>  =  X1)WP<1>  +  X2,mP<2>  +  ...  +  \m,mP(m>  5 

there  may  exist  more  than  one  period  column  in  which  the  coefficient  of 
P<«>  is  Xw,m. 

Thus,  taking  m  =  l,  2,  ...,  r,  we  obtain  r  period  columns  Q*1*,  ...,  Q(r). 
In  terms  of  these  any  period  column  Q,  =  XjP'1'  +  ...  +  XrP(r>,  in  which 
Xj,  ...,  Xr  are  real,  can  be  uniquely  written  in  the  form 


wherein  Nlt  ...,  Nr  are  integers,  and  ^,  ...,  /ir  are  real  quantities  which  are 
zero  or  positive  and  respectively  less  than  \l>1,  ...,  \r,r-  For,  putting  Xr  into 
the  form  Nr\r,r  +  Pr,  where  Nr  is  an  integer  and  fir,  if  not  zero,  is  positive 
and  less  than  \rtr,  we  have 


where 

Xj  =  Xj  —  lv,.X1)r,  .  .  .  ,  X  r_j  =  Xr_j      IV  r  \r—i>r  , 

and  herein  the  column  Q'  =  X1/P<1)  +  ...  +  X/r_iP(r~1)  can  quite  similarly  be 
expressed  in  the  form 


and  so  on. 

But  now,  if  AW  +  ...  +  ^rQ(r)  +/*iP(1)  +  ...  +  P<rP(r)  be  a  period  column, 
it  follows,  aaNlt  ...,Nr  are  integers,  that  also  ^Pw  +...+  /^rP(r>  is  a  period 
column;  and  this  in  fact  is  only  possible  when  each  of  ^,  ...,  /j,r  is  zero. 
For,  by  our  definition  of  Q(r),  the  coefficient  fj,r  is  zero  ;  then,  by  the  definition 
of  Q(r~l),  the  coefficient  /*,._!  is  zero  ;  and  so  on. 

On  the  whole  we  have  the  proposition  (II.,  §  344)  —  if 

Qw  =X1,mP<1»  +  ...  +Xm,mP<™>,  (m  =  l,  ...,  r), 

be  that  real  linear  combination  of  the  first  in  columns  from  P(1>,  ...,  P(r]  in 
which  the  m-th  coefficient  \m,  m  has  the  least  existing  value  greater  than  zero 
and  not  greater  than  unity,  or  be  one  such  combination  for  which  \m,m  satisfies 
the  same  condition,  then  every  period  column  is  expressible  as  a  linear  combina 
tion  of  the  columns  Q(1),  ...,  Q(r)  with  integral  coefficients. 

It  should  be  noticed  that  #*),  ...,  $r>  are  not  connected  by  any  linear  equation  with 
real  coefficients,  or  the  same  would  be  true  of  PW,  ...,  &rl  And  it  should  be  borne 
in  mind  that  the  expression  of  any  period  column  by  means  of  integral  coefficients, 
in  terms  of  QW,  ...,  tyr\  is  a  consequence  of  the  fact  that  the  function  /(MI}  ...,  up) 
has  only  a  limited  number  of  period  columns  which  consist  wholly  of  finite  periods. 
Conversely  the  period  columns,  of  finite  periods,  obtainable  with  such  integral  coefficients, 
are  limited  in  number, 


348]  BY   MEANS   OF   INDEPENDENT   PERIODS.  577 

Another  result  (I.,  §  344)  is  thence  obvious  —  The  coefficients  in  the  linear 
expression  of  any  period  column  in  terms  of  P(1),  ...,  P(r)  are  rational 
numbers. 

For  by  the  demonstration  of  the  last  result  it  follows  that  the  period 
columns  P(1),  ...,  P{r}  can  be  expressed  with  integral  coefficients  in  terms  of 
Q'1',  ...,  Q(r)  in  the  form 

P<™>  =  N("l]Q(l}  +  ...  +  N^Qv,        (m=  1,  ..;,*•)  ; 

from  these  equations,  since  the  columns  P(1),  ...,  P(r)  are  not  connected  by 
any  linear  relation  with  real  coefficients,  the  columns  Q(1),  ...,  Q(r)  can  be 
expressed  as  linear  combinations  of  P(1),  ...,  P(r)  with  only  rational  numbers 
as  coefficients;  hence  any  linear  combinations  of  Qw,  ...,  Q(r)  with  integral 
coefficients  is  a  linear  combination  of  P(1),  ...,  P(r}  with  rational-number 
coefficients. 

It  needs  scarcely*  to  be  remarked  that  the  set  of  period  columns 
Q(l),  ...,  Q(r},  in  terms  of  which  any  other  column  can  be  expressed  with 
integral  coefficients,  is  not  the  only  set  having  this  property. 

348.  We  consider  briefly  the  application  of  the  foregoing  theory  to  the  case  of  uniform 
analytical  functions  of  a  single  variable  which  do  not  possess  any  infinitesimal  periods.  It 
will  be  sufficient  to  take  the  case  when  the  function  has  two  periods  which  have  not  a  real 
ratio  ;  this  is  equivalent  to  excluding  singly  periodic  functions. 

If  2(0!,  2«2  be  two  periods  of  the  function,  whose  ratio  is  not  real,  and  2Q  be  any  other 
period,  it  is  possible  to  find  two  real  quantities  Xx,  X2  such  that 

Q  =  X1o>1  -|-X2&}2  ; 

then  of  periods  of  the  form  2X1o>1,  in  which  0<X1^>1,  of  which  form  periods  do  exist,  2<a1 
itself  being  one,  there  is  one  in  which  Xj  has  a  least  value,  other  than  zero  —  as  follows 
because  the  function  has  only  a  finite  number  of  finite  periods.  Denote  this  least  value 
by  /ij,  and  put  Ql=p.1tal.  Of  periods  of  the  form  2X1o>1  +  2X2w2  in  which  G^>X!  ^>1,  0<X2^>1, 
there  is  a  finite  number,  and  therefore  one,  in  which  X2  has  the  least  value  arising,  say  /z2; 
let  one  of  the  corresponding  values  of  X,  be  X  ;  put  Q2  =  Xa>1  +  /i2<B2-  Then  any  period 
2Q  =  2X1&>1  +  2X2o>2  is  of  the  form  2NlQl  +  2N2Q2  +  2v1o>1  +  2v<2<o2,  where  vlt  v2  are  (zero  or) 
positive  and  respectively  less  than  ^  and  p2,  and  jYj,  Nz  are  integers,  such  that  X2  =  -/V2/i2  +  »'2> 
Xj  —  N^  =  Nlpl-\-vl.  But  the  existence  of  a  period  Q-2iV1Q1-2iV2G2  =  2j/1a>1  +  2i/2<B2  with 
!/!</*!,  v%<pi  is  contrary  to  the  definition  of  /^  and  ^2,  unless  vv  and  i>.2  be  both  zero. 
Hence  every  period  is  expressible  in  the  form  .  « 


where  N^  N2  are  integers. 

In  other  words,  a  uniform  analytical  function  of  a  single  variable  without  infinitesimal 
periods  cannot  be  more  than  doubly  periodic^. 

*  For  the  argument  compare  Weierstrass  (1.  c.,  §  344),  Jacobi,  Ges.  Werke,  t.  ii.,  p.  27, 
Hermite,  Crelle,  XL.  (1850),  p.  310,  Biemarm,  Crelle,  LXXI.  (1859)  or  Werke  (1876),  p.  276.  See 
also  Kronecker,  "Die  Periodensysteme  von  Functionen  reeller  Variabeln,"  Sitzungsber.  der 
Berl.  Akad.,  1884,  (Jun.  bis  Dec.),  p.  1071. 

t  Cf.  Forsyth,  Theory  of  Functions  (1893),  §§  108,  107.  It  follows  from  these  Articles,  in 
this  order,  that  any  three  periods  of  a  uniform  function  of  one  variable  can  be  expressed,  with 

B.  37 


OF   THK 

UNIVERSITY 


578  BEARINGS   OF   THE   THEORY.  [348 

It  follows  also  that  every  period  is  expressible  by  2o>l,  2o>2  with  only  rational-number 
coefficients. 

349.  Ex.  i.     If  r  quantities  be  connected  by  k  homogeneous  linear  equations  with 
integral  coefficients (r>k\  it  is  possible  to  find  r  -  k  other  quantities,  themselves  expressible 
as  linear  functions  of  the  r  quantities  with  integral  coefficients,  in  terms  of  which  the  r 
quantities  can  be  linearly  expressed  with  integral  coefficients. 

Ex.  ii.  If  PW, ... ,  PM  be  r  columns  of  real  quantities,  each  containing  r  -  1  constituents, 
a  column  JVlP(l)  + ...+JVrP^r)  can  be  formed,  in  which  Nlt  ...,  Nr  are  integers,  whose  r-l 
constituents  are  within  assigned  nearness  of  any  r  —  1  assigned  real  quantities  (cf. 
Chap.  IX.,  §  166,  and  Clebsch  u.  Gordan,  Abels.  Funct.,  p.  135). 

Ex.  m.  An  uniform  analytical  function  of  p  variables,  having  r  period  columns  P*1), 
...,  PW,  each  of  p  constituents,  and  having  a  further  period  column  expressible  in  the 
form  X1P<1)  +  ...+XrP<r),  wherein  X1}  ...,  Xr  are  real,  will  necessarily  have  a  column  of 
infinitesimal  periods  if  even  one  of  the  coefficients  X1}  ... ,  Xr  be  irrational. 

From  this  result,  taken  with  Ex.  i.,  another  demonstration  of  the  proposition  of  the 
text  (§  347)  can  be  obtained.  The  result  is  itself  a  corollary  from  the  reasoning  of  the 
text. 

Ex.  iv.     If  7/j'a,  ...,  ux'a  be  linearly  independent  integrals  of  the  first  kind,  on  a 

Riemann  surface,  and  the  periods,  2a>r,g,  2w'r,8,  of  the  integral  u*'  a  be  written  pr,,-H'oy,,, 
p'^  +  iV,.,,,  shew  that  the  vanishing  of  the  determinant  of  2p  rows  and  columns  which  is 
denoted  by 

°V,i>  •••>  °V,  PJ      °>,i>  •••>  °"r,p 

would  involve*  the  equation 

( Ml  —  iNj)  u*' a  + . . .  +  (Mp  —  iNp}  ux>  a  =  constant, 

where  Ml,  Nlt  ...,  Mp,  JVP  are  the  minors  of  the  elements  of  the  first  column  of  this 
determinant  and  are  supposed  not  all  zero. 

The  vanishing  of  this  determinant  is  the  condition  that  the  period  columns  of  the 
integrals  should  be  connected  by  a  homogeneous  linear  relation  with  real  coefficients. 

350.  The  argument  of  the  text  has  important  bearings  on  the  theory  of  the  Inversion 
Problem  discussed  in  Chap.  IX.     The  functions  by  which  the  solution  of  that  problem  is 
expressed  have  2p  columns  of  periods  in  terms  of  which  all  other  period  columns  can  be 
expressed  linearly  with  integral  coefficients  ;  these  %p  columns  are  not  connected  by  any 
linear  equation  with  integral  coefficients  (§  165),  and,  therefore,  are  not  connected  by  any 
linear  equation  with  real  coefficients. 

It  has  been  remarked  (§  174,  Chap.  X.)  that  the  Riemann  theta  functions  whereby  the 
2j9-fold-  periodic  functions  expressing  the  solution  of  the  Inversion  Problem  can  be  built 
up,  are  not  the  most  general  theta  functions  possible.  The  same  is  therefore  presumably 
true  of  the  2/?-fold  periodic  functions  themselves.  Weierstrass  has  stated  a  theorem  t 

integral  coefficients,  in  terms  of  two  periods.  These  two  periods,  and  any  fourth  period  of  the 
function,  can,  in  their  turn,  be  expressed  integrally  by  two  other  periods — and  so  on.  The 
reasoning  of  the  text  shews  that  when  the  function  has  no  infinitesimal  periods,  the  successive 
processes  are  finite  in  number,  and  every  period  can  be  expressed,  with  integral  coefficients, 
in  terms  of  two  periods. 

*  Forsyth,  Theory  of  Functions  (1893),  p.  440,  Cor.  ii. 

t  Berlin,  Monatsber.  Dec.  2,  1869,  Crelle,  LXXXIX.  (1880).  For  an  application  to  integrals 
of  radical  functions,  Cf.  Wirtinger,  Untersuchungen  ilber  Thetafunctionen  (Leipzig,  1895),  p.  77. 


351] 


DEFINITION   OF   GENERAL   JACOBIAN    FUNCTION. 


579 


whereby  it  appears  that  the  most  general  2p-fold  periodic  functions  that  are  possible  can 
be  supposed  to  arise  in  the  solution  of  a  generalised  Inversion  Problem ;  this  Inversion 
Problem  differs  from  that  of  Jacobi  in  that  the  solution  involves  multiform  periodic 
functions*;  the  theorems  of  the  text  possess  therefore  an  interest,  so  far  as  they 
hold,  in  the  case  of  such  multiform  functions.  The  reader  is  referred  to  Weierstrass, 
Abhandlungen  am  der  Functionenlehre  (Berlin,  1886),  p.  177,  and  to  Casorati,  Acta 
Mathematica^  t.  viii.  (1886). 

351.  We  pass  now  to  a  brief  account  of  a  different  theory  which  is 
necessary  to  make  clear  the  position  occupied  by  the  theory  of  theta 
functions.  Considering,  a  priori,  uniform  integral  analytical  functions 
which,  like  the  theta  functions,  are  such  that  their  partial  logarithmic 
differential  coefficients  of  the  second  order  are  periodic  functions,  we  in 
vestigate  certain  relations  which  must  necessarily  hold  among  the  periods, 
and  we  prove  that  all  such  functions  can  be  expressed  by  means  of  theta 
functions. 

Suppose  that  to  the  p  variables  u^,  ...,up  there  correspond  a-  columns  of 
quantities  af(i=l,  ...,  p,  j  =  1,  ...,  a)  and  a  columns  of  quantities  &(/>— 
according  to  the  scheme 


a 


" 


and  suppose  </>(V)  to  be  an  uniform,  analytical  function  of  Wj,  ...,  up  which 
for  finite  values  of  ult  ...,  up  is  finite  and  continuous — which  further  has  the 
property  expressed  by  the  equations 


<£  (U  +  d®)  =  e*r»W[«+JaM]+2«*<>»  0  (U\  (j=l,...,a),  (I.) 

wherein  fttf)  is  a  symbol  for  a  column  6<J),  ...,  by  and  c'^  is  a  single  quantity 
depending  only  on  j.  The  aggregate  of  c(1),...,c«"  will  be  called  the 
characteristic  or  the  parameter  of  <f>(u);  af  will  finally  be  denoted  by  aitj. 
We  suppose  that  the  columns  a^  are  independent,  in  the  sense  that  there 
exists  no  linear  equation  connecting  them  of  which  the  coefficients  are 
rational  numbers;  but  it  is  not  assumed  that  the  columns  a®  constitute  all 
the  independent  columns  for  which  the  function  $  satisfies  an  equation  of 
the  form  (I.).  Also  we  suppose  that  the  equation  (I.)  is  not  satisfied  for 
any  column  of  wholly  infinitesimal  quantities  put  in  place  of  a&.  The 
reason  for  this  last  supposition  is  that  in  such  case  it  is  possible  to  express 
</>  as  the  product  of  an  exponential  of  a  quadric  function  of  ul}  ...,  up, 
multiplied  into  a  function  of  less  than  p  variables,  these  fewer  variables 
being  linear  functions  of  u1}  ...,  up.  The  function  <j>(u)  in  the  most  general 
*  With  a  finite  number  of  values. 

37—2 


580  NECESSARY   LIMITATIONS  [351 

case  is  a  generalisation  of  a  theta  function ;  it  will  be  distinguished  by  the 
name  of  a  Jacobian  function ;  but,  for  example,  it  may  be  a  theta  function, 
for  which,  when  <r  <  2p,  the  columns  a(J)  are  a-  of  the  2p  columns  of  quasi- 
periods,  2o>tf). 

A  consequence  of  the  two  suppositions  is  that  in  the  matrix  of  a 
columns  and  2p  rows,  of  which  the  (2t  —  l)th  and  2t-th  rows  are  formed 
respectively  by  the  real  and  imaginary  parts  of  the  row  c^1*,  ...,a,(?\  not 
every  determinant  of  a-  rows  and  columns  can  vanish.  For  if  with  a  arbitrary 
real  variables  x1,...,xa.  we  form  2p  linear  functions,  the  (2i  —  l)th  and 
2t-th  of  these  having  for  coefficients  the  (2i  —  l)th  and  2*-th  rows  of  the 
matrix  of  cr  columns  and  2p  rows  just  described,  the  condition  that  every 
determinant  from  this  matrix  with  a  rows  and  columns  should  vanish,  is 
that  all  these  2p  linear  functions  should  be  expressible  as  linear  functions  of 
at  most  cr  —  1  of  them.  Now  it  is  possible  to  choose  rational  integer  values 
of  xi}  ...,0V  to  make  all  of  these  cr  —  1  linear  functions  infinitesimally 
small*;  they  cannot  be  made  simultaneously  zero  since  the  cr  columns  of 
periods  are  independent.  Therefore  every  one  of  the  2p  linear  functions 
would  be  infinitesimally  small  for  the  same  integer  values  of  xly...,xa. 
Thus  there  would  exist  a  column  of  infinitesimal  quantities  expressible  in 
the  form  ^a'1'  +  •••  +x<raw.  Now  it  will  be  shewn  to  be  a  consequence  of 
the  coexistence  of  equations  (I.)  that  also  an  equation  of  the  form  (I.)  exists 
when  a(b  is  replaced  by  an  expression  acja^  +  ...  +#aa(<r),  wherein  xl}  ...,xa 
are  integers.  This  however  is  contrary  to  our  second  supposition  above. 

Hence  also  the  matrix  of  a-  columns  and  2p  rows,  wherein  the  (2*  —  l)th 
and  2i-th  rows  consist  of  a(}\  ...,  a(*]  and  the  quantities  which  are  the 
conjugate  complexes  of  these  respectively,  is  such  that  not  every  determinant 
of  cr  rows  and  columns  formed  therefrom  is  zero. 

And  also,  by  the  slightest  modification  of  the  argument,  a  cannot  be 
>  2p.  The  case  when  a  is  equal  to  2p  is  of  especial  importance ;  in  fact 
the  case  cr  <  2p  can  be  reduced  to  thisf  case. 

352.  Consider  now  the  equations  (I.).  We  proceed  to  shew  that  in 
order  that  they  should  be  consistent  with  the  condition  that  <f>  (u)  is  an 
uniform  function,  it  is  necessary,  if  a,  b  denote  the  matrices  of  p  rows  and  cr 
columns  which  occur  in  the  scheme  of  §  351,  that  the  matrix  of  cr  rows  and 

columns^,  expressed  by 

ab  —  ba,  (A), 

should  be  a  skew  symmetrical  one  of  which  each  element   is   a   rational 

*  Chap,  ix.,  §  166. 

+  When  ff  =  2p,  the  hypothesis  of  no  infinitesimal  periods  is  a  consequence  of  the  other 
conditions  (cf.  §  345). 

J  The  notation  already  used  for  square  matrices  can  be  extended  to  rectangular  matrices. 
See,  for  example,  Appendix  n.,  at  the  end  of  this  volume  (§  406). 


353]  IN   THE   GENERAL   DEFINITION.  581 

integer.  Denote  it  by  k,  so  that  kaa  =  0,  kap  =  —  kpa.  But  further  also  we 
shew  that  it  is  necessary,  if  x  denote  a  column  of  cr  quantities  and  x^  denote 
the  column  whose  elements  are  the  conjugate  complexes  of  those  of  x,  that 
for  all  values,  other  than  zero,  satisfying  the  p  equations 

ax  =  0,  (B), 

the  expression  ikxxl  should  be  positive.  We  shew  that  ikxxl  cannot  be  zero 
unless,  beside  ax,  also  a#j  be  zero :  a  condition  only  fulfilled  by  putting  each 
of  the  elements  of  x  —  0  (as  follows  because  the  a-  columns  of  periods  are 
independent  and  there  are  no  infinitesimal  periods).  The  condition  (B)  is  in 
general  inoperative  when  cr  <  p  +  1. 

353.     Before  giving  the  proof  it  may  be  well  to  illustrate  these  results  by  shewing  that 
they  hold  for  the  particular  case  of  the  theta  functions  for  which  (cf.  §  284,  Chap.  XV.) 

(r  =  2p,     a  =  \  2o>,  2o>'|,     2irib=  2rj,  2ij'  , 
and  therefore 

ax-Za>X+^(a'X'  —  Qx,     bx  =  - — .Hx, 

ZTTl 

where  X  is  a  column  of  p  quantities,  X'  a  column  of  p  quantities,  and  x= 


Let 


X 

X' 
Y 

y,  ,  where,  similarly,  each  of  Y  and  Y'  is  a  column  of  p  quantities  ;  then* 

XY'  -  XT=^—. (HxQy-HYQx)  =  ay .  bx -  ax .  by  =  (ab  -  ba)  xy=kxy, 
but 

where  ei+wi=  +1=  —  ti,i  +  p  and  fj,j  =  0  when  i~j  is  not  equal  to  p  ;  thus  we  may  write 

kxy=XY'-X'Y=exy, 

namely,  the  matrix  k  is  in  the  case  of  the  theta  functions  the  matrix  «•,  of  2p  rows  and 
columns,  which  has  already  been  employed  (Chap.  XVIII.,  §  322). 

It  can  be  similarly  shewn  that  in  the  case  of  theta  functions  of  order  r,  k  =  r*. 

Next  if  a,  b,  h  denote  the  matrices  occurring  in  the  exponents  of  the  exponential  in  the 
theta  series,  we  havet 


namely  h.  ax  =  iriX+\>X'.  Hence  the  equations  ax  =  0  give  X=--.bX'.  If  -Xt,  X± 
denote  the  conjugate  complexes  of  X,  X'  we  have  therefore  Xl  =  —.  \X{. 

Tfl 

Hence  ikxx^  =  ifxxl = i(XXJ  -  X'XJ  =  - 1  [bX'X^  +  \  X^X']  =  -  -  (b + bx)  X'X,',  since 

b=b  and  b^b^  Thus  if  b  =  c+id,  \  =  c-id,  the  quantity  -cX'X^  is  positive  unless 
each  element  of  X'  is  zero,  namely,  the  real  part  of  bX'X^  is  negative  for  all  values  of  X' 
(except  zero).  If  X'=m  +  in,  b  (m2  +  »2)  is  equal  to  bm2+b?i2 ;  and  the  condition  that  this 
be  negative  is  just  the  condition  that  the  theta  series  converge. 

*  For  the  notation  see  Appendix  n. 
t  Chap.  x.  §  190,  Chap.  vn.  §  140. 


582  PROOF   OF   THE   NECESSITY  [354 

354.     Passing  from  this  case  to  the  proof  of  equations  (A),  (B)  of  §  352, 
we  have,  from  equation  (I.), 


*  [t* 

_    2Ti6(1'[«  +  a(»  +  Jo'1"]  +  2iric«  +  2iri&<s>[tt  +  £a<2)]  +  27ric'2>  . 


where  Lu  =  iri  [6(1)a(2)  -  6(2>a(1)],  =  -  L2l.  Since  the  left-hand  side  of  the 
equation  is  symmetrical  in  regard  to  ax  and  a2,  eL"  must  be  =  eL",  and 
hence  LK/iri  is  a  rational  integer,  =k2l  say,  such  that  k12  =  —  k2l. 

Obviously,  in  &u  =  a<1>&(3)  -a(2)6(1),  the  part  a(1'6(2)  is  formed  by  compound 
ing  the  first  column  of  the  matrix  a  (of  a-  columns  and  p  rows)  with  the 
second  column  of  the  matrix  6.  Similarly  with  a(s)6(1).  Namely  k12  is  the 
(1,  2)th  element  of  k  =  ab  -  ba.  Since  similar  reasoning  holds  for  every 
element,  it  follows  that  the  matrix  &  is  a  skew  symmetrical  matrix  of 
integers.  Conversely,  if  this  be  so,  it  is  easy  to  prove  by  successive  steps 
the  equation 

u) 


= 

where 


a</3 


and  mi,  ...,  mff  are  integers  ;  this  equation  may  be  represented*  by 


P       am~|  a  <  ^ 

tb?»    «  +  -^-    +27riCHi  +  7ri    S 

L       ^  J 


<f>(u  +  am)  =  <f)(u)e 

In  fact,  assuming  the  equation  (II.)  to  be  true  for  one  set  ml,  ...,  wff,  we 
have,  by  the  equations  (I.), 


a</3 

-  ^am]  +  27ri&(1)  [M  +  am  +  Ja'11]  +  2iricm  +  27ri'c(1)  +  iri    S    fca)3  »ia  JK^  ^  /^ 

a</3 

_  e27ri  [6m  +  &'1']  [M + ^aw  +  ^a'11]  +  2^1  [cm  +  c'11]  +  vi   S    fca)3  7^?)^  +  irf-R  ^  ^  u^ 
For  the  notation  see  Appendix  11. — or  thus — 


.m1+ +b(<T)u.m<T 

=  bwm1.u+ +b((T)mff.u 


355]  OF   THESE   LIMITATIONS.  583 

where  R  is  equal  to  b(l} .  am  —  bm .  a(1),  namely  equal  to 


a</3 

R  +  S  k 


1 
so  that 


=  2  (k2lm2  +  .  .  .  +  knm0)  +  &,2  (7^  +  1)  m.2  +  .  .  .  +  &1(r  (m^  +  l)mv  +  &23ra2ra3  +  .  .  .  ; 
hence 

iriR  +  iri   S   k-giH-iiig         iri   S    kaoma'i>io' 
6  aO  =  6     a</3     '  r  , 

where 

[m/,  .  .  .  ,  wi,']  =  [X  +  1,  7«2,  .  .  .  ,  m,]  ; 
therefore 

.  r  1-1         27ri6nt'ru  +  inm'l  +  2iricm'  +  7rt   S   k.om'mo'i   /    \ 

<f>  [u  +  am  ]  =  e  a</5  ap  a   ^  9  (?*)• 

Similarly  we  can  take  the  case  <f>(u  +  am  —  a(1)),  noticing  that  equation 
(I.)  can  be  written 


where  v  =  w  +  ft'-". 

355.  The  theorem  (A)  is  thus  proved.  The  theorem  (B)  is  of  a  different 
character,  and  may  be  made  to  depend  on  the  fact  that  a  one-valued 
function  of  a  single  complex  variable  cannot  remain  finite  for  all  values  of 
the  variable. 

Consider  the  expression 

L  (£)  =  e-^t  (o+4af)-*rfcf  0  (v  +  a£), 

wherein  %l,  ...,  %g  are  real  quantities. 

Then  £({•  +  «»)/£(£),  wherein  mlt  ...,  wa  are  rational  integers,  is  equal 

a</3 

to  e*ikmt+lfi  s  V71*7"?,  as  immediately  follows  from  equation  (L),  and  is 
therefore  a  quantity  whose  modulus  is  unity.  Now  when  £,...,  £ff  are  each 
between  0  and  1  and  v  is  finite,  L  (£)  is  finite.  Its  modulus  is  therefore 
finite  for  all  real  values  of  £  ;  let  0  be  an  upper  limit  to  the  modulus  of  L  (£)  ; 
G  can  be  determined  by  considering  values  of  £  between  0  and  1.  Let  now 
#!,  ...,xa  be  such  that  ax  —  0,  and  let  x1  denote  the  column  of  quantities 
which  are  the  conjugate  complexes  of  the  elements  of  the  column  x.  Put 
f  =  x  +  #1,  so  that  af  =  a#j. 
Then 


wherein  an  upper  limit  of  the  modulus  of  L  (£)  is  a  positive  quantity  G  whose 
value  may  be  taken  large  enough  to  be  unaffected  by  replacing  x  by  any 


584  PROOF   OF   THE  LIMITATIONS.  [355 

other  solution  of  ax  =  0  ;  it  is  necessary  in  fact  only  to  consider  the  modulus 
of  L  (£)  when  £  is  between  0  and  1. 
We  have 

b%  .  a^  =  b  (x  +  x^)  .  a  (x  +  x^)  =  bx  .  ax1  +  bxl  .  axl 

=  bx  .  a#!  —  bxl  .  ax  +  bxl  .  axl  =  kxxl  +  abxf, 
(c  +  bv)  %,  =  w  (x  +  xj,  say,  =  wx  +  w^  +  (w  —  w^  xlt 

where  w  =  c  +  bv  ;  therefore 

gTri&f  .  af+27ri  (c+bv)  f  J^  /  fc\  _  giirkxx^iTrdbx^+zni  (w—wj  a;,  gini  (wx+wtx,)  J^  /  fc\  • 

this  equation  is  the  same  as 


where 

J£     _  £  /  fc\ 

has  the  same  modulus  as  L  (£),  less  than  G,  and  where 
p  = 


—  yiZj}  =  Zirkyz,  is  a  real  quantity  (x  being  equal  to  y  +  iz). 

Now  if  x  be  any  solution  of  the  equations  ax  =  0,  then  ^x  is  also  a 
solution,  yu,  being  any  arbitrary  complex  quantity  and  ^  its  conjugate 
complex.  Replace  x  throughout  by  fj^x,  and  therefore  £  by  ^x  +  /JLXI.  Then 
the  equation  just  written  becomes 

K  having  also  its  modulus  <  G. 

Herein  the  left  side,  if  not  independent  of  //,,  is,  for  definite  constant 
values  of  v  and  x,  a  one-valued  continuous  (analytical)  function  of  p  which  is 
finite  for  all  finite  values  of  p.  Hence  it  must  be  infinite  for  infinite  values 
of  ytt.  Hence  p  must  be  positive,  viz.,  values  of  x  such  that  ax=0  are  such 
that  the  real  quantity  ikxxl  is  necessarily  positive  provided  only  the  ex 
pression 

is  not  independent  of  /a. 

Now  if  this  expression  be  independent  of  p,  it  is  equal  to  </>  (v),  the  value 
obtained  when  ft  =  0,  and  therefore 


£(0) 

here  the  left  side  is  a  function  of  v  provided  ax±  be  not  zero ;   when  ax1 
is  zero  its  value  is  unity ;  we  take  these  possibilities  in  turn : 
(i)     Suppose  first  ax^  is  not  zero, 


355]  FURTHER  DEDUCTIONS.  585 

then 

(w  —  w-i)  xl  =  (bv  —  b^)  xl*=bx1.v  —  b^  .  v1 

must,  like  the  left  side,  be  a  function  of  v  and  therefore  a  linear  function,  say 
^-.(Bv+C),  so  that 


<f)  (v  +  fiax^  =  <f>  (v)  e^H-BBM+e^  where  A  =  iirabx?  ; 


hence  pax^  represents  a  column  of  periods*  for  the  function  <£  (v)  —  and  this 
for  arbitrary  values  of  /A. 

In  this  case  however  <f>  (v)  would  be  capable  of  a  column  of  infinitesimal 
periods,  contrary  to  our  hypothesis. 

Hence  p  must  be  positive  for  values  of  x  such  that  ax  =  0,  ax^  4  0. 
(ii)     But  in  fact  as  there  are  a-  columns  of  independent  periods  we  cannot 
simultaneously  have  ax  =  0,  axl  =  0.     For  the  last  is  equivalent  to  a^x  =  0  ; 
and  ax  =  0,  a^x  =  0,  together,  involve  that  every  determinant  of  <r  rows  and 


columns  in  the  matrix 


a 


is  zero — and  thence  involve  the  existence  of 


o, 

infinitesimal  periods  (§  351). 

Hence   ikxxl  is   necessarily  positive  for  values   of  x,  other   than   zero, 
satisfying  ax  =  0  ;   and  this  is  the  theorem  (B). 

Remark  i.  From  the  existence  of  two  matrices  a,  b  of  p  rows  and  o-  columns,  for 
which  ab  —  ba  is  a  skew  symmetrical  matrix  of  integers  k  such  that  ikxxl  is  positive 
for  values  of  x  other  than  zero  satisfying  ax  =  0,  can  be  inferred  that  in  the  matrix 

,  not  every  determinant  of  a-  rows  and  columns  can 
ai  \ 

vanish  —  and  also  that  the  o-  columns  of  quantities  which  form  the  matrix  a  are  inde 
pendent,  namely  that  we  cannot  have  the  p  equations  a,-,.r<1)  +  ...+ai<Tx(<r)  =  Q  satisfied 
by  rational  integers  oX1),  ...,  yW.  For  then,  also,  a1^?  =  0,  since  x=xv. 

Remark  ii.  In  the  matrix  k,  if  <r  be  not  less  than  p,  all  determinants  of  2  (o-  -p)  rows 
and  columns  cannot  be  zero.  In  the  matrix  a,  not  all  determinants  of  \<r  or  £  (o-  +  l)  rows 
and  columns  can  be  zero.  In  particular  when  o-  =  2p,  for  the  matrix  k,  the  determinant  is 
not  zero  ;  for  the  matrix  a,  not  all  determinants  of  p  rows  and  columns  can  be  zero. 

Let  £,  TJ  be  columns  each  of  or  quantities.  Then  the  coexistence  of  the  3  sets  of 
equations 


is  inconsistent  with  the  conditions  (A)  and  (B)  (§  352),  except  for  zero  values  of  £  and 
The  second  of  them  obviously  gives  also  at]l  =  0. 

For  from  these  equations  we  infer  that  k^  =  a^  .  b^  -  b£  .  a^  is  zero,  and  also 


and  therefore  also  k^  is  zero.     But  by  condition  (B)  the  vanishing  of  ki^  when,  as  here, 
«»7i  =  0,  enables  us  to  infer  rj=0. 

*  We  use  the  word  period  for  the  quantities  «(»  occurring  in  our  original  equation  (I.). 


586  COMPARISON   OF  THE   CASE  [355 

Similarly 


is  zero  when  I  (£  +  »?i)  =  0,  <%  =  (),  a£  =  0.     Thence  by  condition  (B),  since  a|=0,  £  is  zero. 

Suppose  now  that  the  number  of  the  p  linear  functions  a£  which  are  linearly  inde 
pendent  is  v,  so  that  all  determinants  of  («/  +  !)  rows  and  columns  of  the  matrix  a  are  zero, 
but  not  all  determinants  of  v  rows  and  columns  ;  and  that  the  number  of  the  a  linear 
functions  k£  which  are  linearly  independent  is  2**,  so  that  in  the  matrix  k  all  determinants 
of  2/c  +  l  rows  and  columns  vanish,  but  not  all  of  2/c  rows  and  columns.  Then  we  can 
choose  2«/  +  2K  linearly  independent  linear  functions  from  the  2p  +  o-  functions  «£,  a^, 
&  (!  +  »?)•  If  this  number,  2i/  +  2*,  of  independent  functions,  were  less  than  the  number  2o- 
of  variables  |,  rj,  the  chosen  independent  functions  could  be  made  to  vanish  simultaneously 
for  other  than  zero  values  of  the  variables,  and  then  all  the  linear  functions  dependent  on 
these  must  also  vanish. 

Hence 

2i/  +  2*  5  2o-  or  v  +  K  >  (r. 
Now 

i/<jt>,    2K<<r;    hence    v^\v,    2ic>2(o--j»). 

Remark  iii.  It  follows  from  (ii)  that  if  £  =  0,  then  i/  =  <r  and  <r=jo.  Also  that  a  function 
of  p  variables  which  is  everywhere  finite,  continuous  and  one-valued  for  finite  values  of  the 
variables  and  has  no  infinitesimal  periods  cannot  be  properly  periodic  (without  exponential 
factors)  for  more  than  p  columns  of  independent  periods  ;  in  every  set  of  o-  independent 
periods  of  such  a  function  the  determinants  of  a-  rows  and  columns  are  not  all  zero.  The 
proof  is  left  to  the  reader. 

Remark  iv.  When  a-=2p  we  can  put  a=|2&>,  2«'  ,  wherein  the  square  matrix  2o>  is 
chosen  so  that  its  determinant  is  not  zero.  When  we  write  a—\  2<o,  2o>'  |  we  shall  always 
suppose  this  done. 

356.  Ex.  i.  Prove  that  the  exponential  of  any  quadric  function  of  ult  ...,  up  is  a 
Jacobian  function  of  the  kind  here  considered,  for  which  the  matrix  k  is  zero. 

Ex.  ii.  Prove  that  the  product  of  any  two  or  more  Jacobian  functions,  <£,  with  the 
same  number  of  variables  and  the  same  value  for  o-,  is  a  function  of  the  same  character, 
and  that  the  matrix  k  of  the  product  is  the  sum  of  the  matrices  k  of  the  separate  factors. 

Ex.  iii.  If  0  be  considered  as  a  function  of  other  variables  v  than  u,  obtained  from 
them  by  linear  equations  of  the  form  u=n  +  cv  (p  being  any  column  of  p  quantities,  and  c 
any  matrix  of  p  rows  and  columns),  prove  that  the  matrix  k  of  the  function  $,  regarded 
as  a  function  of  v,  is  unaltered. 

Obtain  the  transformed  values  of  a,  6,  c  and  bm(u+^am)  +  cm.  (Of.  Ex.  i.,  §  190, 
Chap.  X.) 

Ex.  iv.  If  instead  of  the  periods  a  we  use  a'  =  ag,  where  g  is  a  matrix  of  integers  with 
<r  rows  and  columns,  prove  that  <^(u  +  a'm}  is  of  the  form  e^ib'^('ll+Wm)+Zniem  ^^  and 
that  V=gkg  ;  and  also  that  kxy  becomes  changed  to  k'x'y'  by  the  linear  equations  x=gxf, 
y  =gy'.  In  such  case  the  form  k'x'y'  is  said  to  be  contained  in  kxy.  When  the  relation  is 
reciprocal,  or  #2  =  1,  the  forms  are  said  to  be  equivalent.  Thus  to  any  function  $  there 
corresponds  a  class  of  equivalent  forms  k.  (Cf.  Chap.  XVIII.,  §  324,  Ex.  i.) 

Examples  iii.  and  iv.  contain  an  important  result  which  may  briefly  be  summarised  by 

*  That  the  number  must  be  even  is  a  known  proposition,  Frobenius,  Crelle,  LXXXH.  (1877), 
p.  242. 


356] 


OF  THE   THETA   FUNCTIONS. 


587 


saying  that  for  Jacobian  functions,  qua  Jacobian  functions,  there  is  no  theory  of  transfor 
mation  of  periods  such  as  arises  for  the  theta  functions.  A  transformed  theta  function  is 
a  Jacobian  function  ;  the  equations  of  Chap.  XVIII.  (§  324)  are  those  which  are  necessary 
in  order  that,  for  this  Jacobian  function,  the  matrix  k  should  be  the  matrix  e,  or  n 
(cf.  §  353). 

Ex.  v.     If  A  be  a  matrix  of  2p  rows  and  <r  columns  of  which  the  first  p  rows  are  the 
rows  of  a  and  the  second  p  rows  those  of  b,  prove  that 


In  fact  if  g  =  Ax,  g^Ax1,  then 

kx'x  =  ax  .  bx'  -  ax'  .bx  =  2  [&  £'<  +  p  -  £/  &  +  p]  =  «££' 
=  f  Ax  .  A  x'  =  A  eA  .  x'x. 

Hence  also  when  a-  =  2p  the  determinant  of  A  is  the  square  root  of  the  determinant  of  /•, 
which  in  that  case,  being  a  skew  symmetrical  determinant  of  even  order,  is  a  perfect 
square. 

Ex.  vi.     Shew  that  when  tr  —  Zp  and  with  the  notation  a  =  |2co,  2a>'|,  2irib  =  \2r),  2^'|, 
that 

2 

I  7]  —  T)  CO,         £0  ?;'  —  T!  ft)'       , 


At  A  =  - 


(a  T)  —  tj  <o,     co  77  —  T)  a> 

the  notation  being  an  abbreviated  one  for  a  matrix  of  2p  rows  and  columns.  Thus  in  the 
case  when  k  =  e,  the  equation  of  Ex.  v.  expresses  the  Weierstrass  equations  for  the  periods 
(Chap.  VII.,  §  140). 

Ex.  vii.  In  the  case  of  the  theta  functions  we  shewed  (§  140,  and  p.  533)  that  the 
relations  connecting  the  periods  could  be  written  in  two  different  ways,  one  of  which  was 
associated  with  the  name  of  Weierstrass,  the  other  with  that  of  Riemann.  We  can  give  a 
corresponding  transformation  of  the  equations  (A),  (B)  (§  352)  in  this  case,  provided  <r  =  2jo, 
the  determinant  of  the  matrix  k  not  being  zero. 

As  to  the  equation  (A),  writing  it  in  the  equivalent  form  given  in  Ex.  v.,  we 
immediately  deduce 

Ak-iA=e,  (A'), 

which  is  the  transformation  of  equation  (A). 

As  to  the  equation  (B),  let  x  be  a  column  of  a-=2p  arbitrary  quantities,  and  determine 
the  column  2,  of  <r  =  2p  elements,  so  that  the  2p  equations  expressed  by  az=0,  bz=x,  are 


satisfied.     Then 
thus 


C(x=abz  =  (ab-ba)z  =  h,  =/*,  say;   so  that  k~lu=z,  k-1u,=z, 
ikzzl  =  i  (ab-  ba)  zzt  =  i  (azl  .bz-az.bz})  =  iazl  .  bz  =  iaZjX  =  iaxzl  =  i 

=  ik~l  Hi/j,  =  ik-^a^  .  ax  =  iak  ~  l  a^x  ; 
therefore,  the  form 


(B'), 


is  positive  for  all  values  of  the  column  x,  other  than  zero.     This  is  the  transformed  form 
of  equations  (B). 

Ex.  viii.     When  a  =  \  2«,  2«'  ,  b  =   l  .  \  2,,  2,'  |  ,  a-  =  2jo,  we  have 


27Tl' 


A(A 


2o>,   2o>' 


•n        ni 


0   -  1 

•"•i 

= 

At     -'           '-N                 2    /      -1            -X 

—  4  (coco  —  co  co),      i  (COT;  —  co  rj) 
irl 

1       0 

K,  1 

m 

2                 _,               1 

Tl                                 (TTI) 

588 


EXPRESSION    OF   A   JACOBIAN    FUNCTION. 


[356 


Hence  when  k  =  e,  the  equation  (A')  of  Ex.  vii.,  equivalent  to  A(A=-e,  expresses  the 
Biemann  equations  for  the  periods  (Chap.  VIL,  §  140).  In  the  same  case  the  equation 
(B'),  of  Ex.  vii.,  expresses  that 


=  2       2 

V=l    K,  \  =  l 


is  negative  for  all  values  of  x  other  than  zero. 

Ex.  ix.     When£>  =  l,  the  two  conditions  (B),  (B'),  or 

±  =  positive  for  ax—Q,     iaealxlx  =  negative  for  arbitrary  x, 


become,  for  a  =  |2o),  2a>'  ,  if  the  elements  of  x  be  denoted  by  x  and  x',  and  the  conjugate 
imaginaries  by  xlt  x^  respectively, 

i  (wwj)"1  (cow/  -  co'dj)  x'x±  =  positive,     i  (o^w'  -  «&>/)  xx^  =  negative, 
and  if  o>=p  +  io-,  <»1=p-io-,  a>'  =  p'  +  i<r',  &>/  =  p  -  ia-',  these  conditions  are  equivalent  to 

pa-'  —  p'<r>0, 
and  express  that  the  real  part  of  io>'/a)  is  negative. 

357.  Suppose  now  that  cr  =  2p  ;  we  proceed  (§  359)  to  consider  how  to 
express  the  Jacobian  function.  Two  arithmetical  results,  (i)  and  (ii),  will  be 
utilised,  and  these  may  be  stated  at  once  :  (i)  if  k  be  a  skew  symmetrical 
matrix  whose  elements  are  integers,  with  2p  rows  and  columns,  and  e  have  the 
signification  previously  attached  to  it,  it  is  possible  to  find  a  matrix  g,  of  2p 
rows  and  columns,  whose  elements  are  integers,  such  that*  k  =  geg.  For 
instance  when  p  =  1,  we  can  find  a  matrix  such  that 


0     &12 
-k      0 


#12    #22 


0  -1 

1  0 


ffll    ff 
ffa.  #22  ! 


fu  -  gng*  g<*g™  - 

ll  -  #12^21      #20^12  - 


namely,  such  that  &12  =  #2i#i2  —  #11^22 ;  f°r  this  we  can  in  fact  take  gn,  g12 
arbitrarily.  In  general  the  4p2  integers  contained  in  g  are  to  satisfy 
p  (2p  —  1)  conditions. 

Ex.  i.     If  a  be  a  matrix  of  integers,  of  p  rows  and  columns,  and  X  be  an  integer,  and 

0,    —  Xa 
Xa,       0 
g  may  have  either  of  the  two  following  forms 


ffi  = 


X,  0 


0,  a 

for  we  immediately  find  p.k/ji=k. 


Xa,  0 
0,  1 


=    X,  0 


0,  a 


a,  0 
0,  a-1 


For  a  proof  see  Frobenius,  Crelle,  LXXXVI.  (1879),  p.  165,  Crelle,  LXXXVIII.  (1880),  p.  114. 


357] 


PRELIMINARY   ARITHMETICAL   LEMMAS. 


589 


Ex.  ii.  If  /x  be  any  matrix  of  integers,  with  2jo  rows  and  columns,  such  that  ntn  =  f 
(cf.  §  322,  Chap.  XVIIL),  we  have,  if  k=*geff,  also  k=g^~l(ti-lg)  and  instead  of  g  we  may 
take  the  matrix  p~lff. 

(ii)  If  g  be  a  given  matrix  of  integers,  of  2p  rows  and  columns,  and  x  be 
a  column  of  2p  elements,  the  conditions,  for  ac,  that  the  2p  elements  gas 
should  be  prescribed  integers  cannot  always  be  satisfied,  however  the  elements 
of  x  (which  are  necessarily  rational  numerical  fractions)  are  chosen.  If  for 
any  rational  values  of  x,  integral  or  not,  gx  be  a  row  of  integers,  and  we  put 
x  =  y  -4-  L,  where  y  has  all  its  elements  positive  (or  zero)  and  less  than  unity, 
and  L  is  a  row  of  integers  (including  zero),  then  gx  =  gy  +  gL  =  gy  +  M , 
where  M  is  a  row  of  integers ;  in  this  case  the  row  gx  will  be  said  to  be  con 
gruent  to  gy  for  modulus  g.  The  result  to  be  utilised*  is,  that  the  number 
of  incongruent  rows  gx,  namely,  the  number  of  integers  which  can  be  repre 
sented  in  the  form  gx  while  each  element  of  x  is  zero  or  positive  and  less  than 
unity,  is  finite.  It  is  in  fact  equal  to  the  absolute  value  of  the  determinant  of 


9- 

For  instance  when  c 

^  is     gu  glz 

there 

are  gngyz-gl 

2^2!  integer  pair 

which  can  be  written  gnx1+gl2x2,  g^^  +  g^, 
less  than  unity.     The  reader  may  verify,  for 
the  9  ways  are  given  (cf.  p.  637,  Footnote)  by 

vz,  for  (rational)  values  of  xl}  a 

6  3 

instance,  that  when  q  = 
I  2 

1 

234 

5 

6789 

T       T                         Of 
1  ?       2                        ">     ^ 

)      4      4.       5       2 
¥'9       ¥»    IT 

i»* 

2      8 
f  '    ¥ 

i  t    i 

72285 

?    i?>  a     ¥»  ¥ 

fi-r   4-  ^T      T    -L  9/r        ft     f 
v^i*/i    i^  tJiX/g  j  «*^i    i^  ^*^2       "j     *- 

)    2,  1    4,  1 

3,  1 

4,  2 

5,  1    5, 

2    6,  2    7,  2 

To  prove  the  statement  in  general  let  t  be  the  number  required,  of  integers 
representable  in  the  form  gx,  when  x  <  1.  Consider  how  many  integers 
could  be  obtained  in  the  form  gX  when  X  is  restricted  only  to  have  all  its 
elements  less  than  (a  positive  number)  N.  Corresponding  to  any  one  of  the 
t  integers  obtained  in  the  former  case  we  can  now  obtain  N—l  others  by 
increasing  only  one  of  the  elements  of  x  in  turn  by  1,  2,  ...,  N—  1.  This 
can  be  done  independently  for  each  element  of  x.  Hence  the  number 
of  integers  gX  is  tN"  where  a,  here  to  be  taken  =  2p,  is  the  number  of 

elements  in  x.    Let  one  of  these  integers  be  called  M.     Then  g  -^  =  -^r  or  say 

M 

gx  =  jj.,  wherein  x  is  less  than  unity.     Now  when  N  is  very  great,  the 


p.  189 


Cf.  Appendix  ii,  §  418,  and  the  references  there  given,  and  Frobenius,  Crelle,  xcvn.  (1884), 


590  EXPRESSION   OF   A   JACOBIAN   FUNCTION  [357 

M 

variation  of  z  =  -^ ,  as  M  changes,  approaches  to  that  of  a  continuous  quan 
tity,  and  the  number  of  its  values,  being  the  same  as  the  number  of  values 
of  M ,  is 


where  zlt  ...,  za  vary  from  zero  to  all  values  which  give  to  x,  in  the  equations 
gas  =  2,  a  value  less  than  unity.     Now  this  integral  is 


l....<, 

0  V*l>  •••!  x<r) 

Since  this  is  equal  to  tN",  it  follows  that  t  is  equal  to  \g\,  as  was  stated. 

358.  Supposing  then  that  the  matrix  g,  with  2p  rows  and  columns  each 
consisting  of  integers,  has  been  determined  so  that  k  =  ab—I>a  =  geg,  we 
consider  the  expression  of  the  Jacobian  function  when  cr  =  2p.  The  deter 
minant  of  k  not  being  zero,  the  determinant  of  g  is  not  zero. 

Put  K=ag~l,  so  that  K  is  a  matrix  of  p  rows  and  2p  columns,  and 
a  =  Kg  ;  put  similarly  b  =  Lg  ;  also,  take  a  row  of  2p  quantities  denoted  by 
G,  such  that  c  =  gC  +  J  [g],  where  c  is  the  parameter  (§  351)  of  the  Jacobian 
function,  and  [g]  is  a  row  of  2p  quantities  of  which  one  element  is 


take  x,  x',  X,  X',  rows  of  2p  quantities  such  that 

X  =  gx,  X'  =  gx',  so  that  ax  =  Kgx  =  KX,  bx  =  LX,  ax'  =  KX',  bx  =  LX' ; 

then  as 

kx'x,  =  ax .  bx'  —  ax' .  bx,  =  (KL  —  LK)  X'X, 

is  also  equal  to 

gegx'x  =  egx' .  gx  =  eX'X, 
we  have 

so  that 

i, ...,  p 

KxLx  —  Kx'Lx  =  (KL  —  LK)  x'x  —  ex'x  =    S    (ittaffff  —  xj  ^J+P)  '•> 

i,j 

further,  as  ikxx1  is  positive  for  ax  =  0,  we  have 

ieXX\  =  positive  when  KX  =  0,  (D) ; 

jr 

thus,  if  A  denote  the  matrix     r    ,  we  have,  from  the  equation  (C), 

Li 

and,  if  z  be  a  row  of  p  arbitrary  quantities,  and  Z  be  a  row  of  2p  quantities 


358]  BY  MEANS  OF  THETA  FUNCTIONS.  591 

such  that  KX=0,  LX  =  z,  so  that  Kz  =  KLX  =  (KL  -  LK)  X  =  eX,  and 
therefore  eKz  =  -  X,  K&  =  eXlt  we  have 

iKleKzz1  =  positive,  for  arbitrary  z  other  than  zero,  (F)  ; 

for 

iKleKzzl  =  —  iKlXzl  =  -  i 


If  we  now  change  the  notation  by  writing  K=  |2o>,  2o>'|,  2mL  =  \2ij,  2i)'\, 
and  introduce  the  matrices  a,  b,  h  of  p  rows  and  columns  defined  by 

a=  ^r)o)~l,  h  =  ^7rio)~l,  b  = 


it  being  assumed,  in  accordance  with  Remark  iv.  (§  355)  that  the  determinant 
of  the  matrix  w  is  not  zero,  then  the  equation  (E)  shews  (cf.  Ex.  viii.,  §  356) 
that  the  matrices  a,  b  are  symmetrical,  and  that  rf  =  ?7a>~1a>'  —  ^iriS  l,  so  that 
we  can  also  write 

r)  =  2a&>,     t]  =  2ao>'  —  h',     2hw  =  iri,     2h&>'  =  b  ; 
also,  by  actual  expansion, 


-  _          1 

b]  &>  =  --  &>!  [bj  +  b] 

7T 


WjCft),  if  b  =  c  +  * 

7T 


thus 

_  2 

iKleKzzl  =  --  ctj,  where  t  =  wz,  z  and  t  being  rows  of  p  arbitrary  quantities  ; 

7T 

and  therefore,  by  the  equation  (F),  for  real  values  of  n1}  ...,  np  other  than 
zero,  the  quadratic  form  bn2  has  its  real  part  essentially  negative. 
Hence  we  can  define  a  theta  function  by  the  equation 


|  u  .  '   )  «•  2eau2+2hM(w+V 

V     '    —  7/         n 


wherein  7,  7'  are  rows  of  p  quantities  given  by  G  =  (y',  7),  that  is,  Cr  =  yr', 
Gp+r  =  7r>  for  r  <  p  +  1.  Denoting  this  function  by  ^  (u  ;  C)  and  taking  /*  for 
a  row  of  2p  integers,  the  function  is  immediately  seen  (§  190,  Chap.  X.)  to 
satisfy  the  equation 


^^^(u-  C), 

which  is  the  definition  equation  for  a  Jacobian  function  of  periods  K,  L  and 
parameter  (7,  for  which  the  matrix  k  is  e. 

Further,  if  p  be  a  matrix  of  integers  with  2p  rows  and  columns,  such  that 
/Ze/x  =  e,  and  (Ex.  ii.,  §  357)  we  replace  g  by  fjr^g,  the  matrices  K,  L  are 
replaced  by  Kp  and  Z/A.  Thus  instead  of  the  theta  function  §(u;  C) 
we  obtain  a  linear  transformation  of  this  theta  function  (cf.  §  322  Chap 
XVIII.). 


592  EXPRESSION   OF   A  JACOBIAN   FUNCTION  [359 

359.     Proceeding  further  to  obtain  the  expression  for  the  general  value 
of  the  Jacobian  function  <£,  let  $  (u  ;  v)  denote 


d>  (u  +  Kv)  e~ZlriLv  (U 

where  Vi  =  ni}  Vi+p  =  ni,  for  i<p  +  l.      Then,  since   a  =  Kg,  and  therefore 
aN  =  KgN,  we  have 

0  (u  +  aN,  v)  =  <f)  (u  +  KgN,  v)  =  <j>  (u  +  Kp,  v),  (I), 

where  /j,  denotes  the  row  gN,  so  that  aN=Kp,  N  being  a  column  of  2jt> 
integers  and  therefore  p  a  column  of  integers  ;  thus  <£  (u  +  aN,  v)  is  equal  to 

0  (U  +  aN+  Kv)  e~^iLv  (*+*/*+**")  -2"iCv+ninn'  =  fy  (u 

where 


u  +  K/j,  +  %Kv)  —  2-rriCv  +  winn', 

by  the  properties  of  (f>,  N  being  a  column  of  integers  ;  thus  <f>(u  +  aN,  v)  is 
equal  to 

<x<0 

*  /..      \a2TribN(u  +  ^aN)  +  2wicN+n   S    kaBNaNs  +  2Tri(bN  .Kv  -  Lv  .K/j.) 

Q)  I  i-Cj   l/  }  c/  • 

Now  bN=LgN  =  L/j,,  therefore 

IN  .  Kv  —  Lv  .  Kp  =  (KL  —  LK}  pv  =  epv  =  mri  —  m'n, 


where  ^  =  mf,  m+p  =  m/,  etc.  for  i<p  +  l.     If  then  we  take  v,  as  well  as  p, 
to  consist  of  integers,  it  will  follow  that 


and  therefore  that 

$  (u  +  aN)  _  <f>(u  +  aN,  v)  _  ^ibN  (u  +  &N)  +  z-wicN  +  ^  2 
<f>  (u)  (/>  (u,  v) 

Next 


(>    U, 

and  this 

=  <f)(u  +  K/J,,  v)  eM, 
where 

M  =  27riLv  (u  +  K/J,  +  ^Kv)  +  Z-rriCv  -  -rrinn'  -  ZTTI  (Lp  +  Lv)  (u 

—  ZTTI  (Op  +  Cv)  +  iri  (m  +  m)  (n  +  n')  ; 
therefore 

<f>  (U  +  Kfl,  v)    _frriLn  (u 

(f>  (U,  ft  +  v 

iinni'+irinri—iri  (m+m')  (n+»i') 


359]  BY  MEANS  OF  THETA  FUNCTIONS.  593 

of  which  the  exponent  of  the  right  side  is 
iri  [(KL  -  LK)  pv  -  mri  -  m'n]  =  TTI  \rnri  -  m'n  -  (mri  +  m'n)]  =  -  Zirim'n, 

so  that,  since  /*,  v  consist  of  integers,  the  right  side  is  unity. 
Hence  we  have 

(ft  (U  -f  KfJ,,  V)  _  griLli  (u+lKrt+tonCn-Trimm^ 

<ft  (u,  fi  +  v) 
It  is  to  be  carefully  noticed  that  this  equation  does  not  require  /A  =  0  (mod.  g). 

a<0 

We  suppose  now  that  p=0  (mod.  g).    Then  cN+$  2  ka^NaN^  =  Cfji,-^mm' 
(mod.  unity)  and  L(j,  =  bN,  K^  =  aN,  as  will  be  proved  immediately  (§  360)  ; 


thus 

'  a 


<f>  (u)  (f)  (u,  v)       ~  <j>(u,  p  +  v} 

and  therefore  $  (u,  ^  +  i>)  =  <£  (u,  v)  for  integer  values  v  and  any  integer 
values  p  that  can  be  written  in  the  form  gN,  for  integer  N  ';  namely  (f>(u,  v) 
is  unaltered  by  adding  to  v  any  set  of  integers  congruent  to  zero  for  the 
matrix  modulus  g. 

The  set  of  g  integers  gr,  wherein  r  has  all  rational  fractional  values  less 
than  unity  will  now  be  denoted  by  v,  each  value  of  v  denoting  a  column  of 
2p  integers  —  in  particular  r  =  0  corresponds  to  a  set  of  integers  =  p  (mod.  g}. 
And  v  shall  denote  a  special  one  of  the  sets  of  integers  which  are  similarly  a 
representative  incongruent  system  for  the  transposed  matrix  modulus  g,  such 
that  v  =gr,  the  quantities  r'  being  a  set  of  fractions  less  than  1.  With  the 
assigned  values  for  v,  let 

^(w)  =  2e-27rir/v0(w,  v); 

V 

then 

ijr  (u  +  K\)  =  Se-2™1'"  <f>  (u  +K\,  v}  =  Ze-™'11  &™LK  <«+***>  +ar<cx-»i«'  ^  (M>  x  +  v) 

for  any  set   of  integers   X,  as   has   been   shewn   (\   being   such   that,    for 


If  now  v  +  \  =  p,  so  that  p  also  describes,  with  v,  a  set  of  integers 
incongruent  in  regard  to  modulus  g,  those  for  which  the  necessary  fractions 
s,  in  p  =  gs,  are  >  1  being  replaced,  by  the  theorem  proved  *,  by  others  for 
which  the  necessary  fractions  are  <  1,  so  that  the  range  of  values  for  p  is 
precisely  that  for  v,  then  we  have 


u 

—  g2irl'r'X+2jrt'l/X  (M+iX'A)+2irtC'A—  iri'M'  ^g—  SirirV 

V 

riiA.  (M+JA'A)  +2iriCA-irtf<'         /\ 


*  That  0(w,  y)  is  unaltered  when  to  »/  is  added  a  column  =0  (mod.  g). 

B.  38 


594  EXPRESSION    OF   A   JACOBIAN    FUNCTION  [359 

Hence,  by  the  result  of  §  284,  Chap.  XV.,  we  have 

1r(u)  =  A,*(u,  C+r'), 

the  theta  function  depending  on  the  a,  b,  h  derived  in  this  chapter  (§  358). 
Now  let  v  describe  a  set  of  incongruent  values  for  the  modulus  g  ;  then 

*  (u,  C  +  r')=  ^  0)  =  22e-2™'"  <£  (u,  v)  ; 


v' 

and  since  v  =  gr,  we  have  v'r  =  gr'r  =  grr  =  vr  ;  thus 

Vg-2jnVV  _  ^  /g—  2irwV\  _  ^  (Q—  2Trirl\v\  /g—  2«r2y2  _  _  _  /g—  lTrinp\v'-tp  ; 
v'  v'  v' 

this  sum  can  be  evaluated  : 

when  v  =  0  (mod.  g),  or  the  numbers  r  are  zero,  its  value  is  equal  to  the 
number  of  incongruent  columns  for  modulus  g,  =  \g\.     Since  k  =  geg,  we 

have  \k\  =  (|#|)2,  so  that  \g  =  J~k\. 

when  v  ^0  (mod.  g),  so  that  some  of  rl}  ...,  r2p  are  fractional,  its  value  is 
zero,  as  is  easy  to  prove  (see  below,  §  360). 

Hence  we  have  the  following  fundamental  equation  : 

Vpfcf  (j>  (u)  =  2As*  (u,  C  +  v'\ 

v' 

which  was  the  expression  sought. 

Thus  betiveen  V|  k  \  +  1  functions  <f>  with  the  same  periods  and  parameters 
there  exists  a  homogeneous  linear  relation  with  constant  coefficients*. 

Ex.  i.  Prove  that  a  product  of  n  functions  ^  is  a  function  $  for  which  Vl^"!  is  changed 
into  nP  *J\k  \.  In  fact  the  periods  are  na,  nb. 

Ex.  ii.  Prove  that  the  number  of  homogeneous  products  of  n  factors  selected  from 
jo  +  2  functions  <£  of  the  same  periods  and  parameters  is  greater  than  np^\k\  when  n 
is  large  enough.  And  infer  that  there  exists  a  homogeneous  polynomial  relation  con 
necting  any  p  +  2,  functions  0  of  the  same  periods  and  parameters.  (Of.  Chap.  XV.,  §  284, 
Ex.  v.) 

360.     We  now  prove  the  two  results  assumed. 

(a)     If  /j,  =  0  (mod.  g)  or  ^  =  gN,  where  N  are  integers,  then 

a<|3 

cN  +  \  2  k^N+Np  =  Cfji-  %mm      (mod.  unity). 
For 

2p  p 

k«e  =  fag)*?  =  S  (g\y(eg}yt  =  2  (g)ay  2 

y  y=l  A=l 

P  P  P 

=  2,gyaz<  [ey\gw  +  ey,\+pg*+p,fi]  +  ^ 

y=l         A=l  y= 


*  Weierstrass,  Berl.  Monatsber.,  1869;   Frobenius,   Crelle,  xcvn.  (1884);    Picard,  Poincar^, 
Compt.  Rendus,  xcvn.  (1883),  p.  1284. 


360]  BY  MEANS  OF  THETA  FUNCTIONS.  595 

therefore 


a</3  p  a</3 

2  kaftNaN  =  2  2 


=  22  [ffy+p,aN..gy,itNfi+ffv,aNa.ffv+p,pNe],     (mod.  2), 
y-i 

a</3  a</3  \ 


v=i 

=  2  2?,gy+ptaNa  .  $ry,^  ,  (mod.  2), 

y-i 

where  the  22  indicates  that  the  summation  extends  to  every  pair  a, 
except  those  for  which  a  =  ft  ;   thus 


P 
=   *  E0*A 

y-i 


=  2  /iy  .  /iy+p  =  mm',  (mod.  2)  ; 

•     y=l 

therefore,  since  %Na2  =  ^Na  (mod.  unity),  and  therefore 


u  y=1 

we  have 


N  =  {gC  +  ±[g]}  N  +  ±mm'  -  ±\g\  N, 

(mod.  1), 
=  gN  .  C  +  %mm'  =  fiC  +  \mm!  =Cjj,-  ^mm',  as  required. 

(6)     If  r1}  ......  ,  r^  be  any  set  of  rational  fractions  all  less  than  unity 

and  not  all  zero  and  such  that  the  row  gr  =  v  consists  of  integers,  and 
(v\,  ......  ,  Vsp),  =  v',  be  every  integer  row  in  turn  which  can  be  represented  in 

the  form  gr'  for  values  of  /  less  than  unity,  then 


is  zero.     Since,  as  remarked  (§  359),  the  sum  can  also  be  written 


2  (e~ 

r' 


wherein  i/,,  ...,  v^  are  integers,  the  sum  is  unaffected  by  the  addition  of  any 
integers  to  any  one  or  more  of  the  representants  r\,  ....  r'ap,  namely  it  has 
the  same  value  for  all  sets,  v,  of  incongruent  columns  (for  the  modulus  g). 
If  to  each  of  any  set  of  incongruent  columns  v  we  add  the  column 
(0,  ...,  0,  \i,  0,  ...,0),  all  of  whose  elements  are  zero  except  that  occupying 
the  i-th  place,  which  is  an  integer,  we  shall  obtain  another  set  of  in- 
congruent  columns. 

38—2 


596 


EXAMPLE    OF   THE    EXPRESSION 


[360 


Suppose  then  in  the  above  sum  TI  is  fractional.  Add  to  every  one  of 
the  incongruent  sets  v  the  column  (0,  0,  ...,  1,  0,  ...,  0),  of  which  every 
element  except  the  i-ih  is  zero.  In  the  summation  everything  is  unaffected 
except  the  powers  of  e~2lfir^,  which  are  multiplied  by  e~2nir*.  Hence  the 
sum  is  unaffected  when  multiplied  by  e~Znir*,  and  must  therefore  be  zero. 

We  put  down  the  figures  for  a  simple  case  given  by 

4  5 


then  gr=(4rl  +  5rz,  ?'1  +  2r2)  and  the  equations  gr  =  v  give 


thus  the  values  of  rlt  r2  and  vlt  v2  are  given  by  the  table 


ri,     ra 

0,  0 

.i..i 

1,1 

"n  "2 

0,  0 

3,   1 

6,  2 

Similarly  gr'  =  (kr\+r'z,  5'''i  +  2r'2),  and  the  equations  gr'  =  v  give 
thus  the  values  of  r\,  r'2  and  v\,  i>'2  are  given  by  the  table 


Thus  the  sum  in  question  is 


r'     r' 

0,  0 

i,  I 

§,  \ 

V'D  "'2 

0,  0 

2,  3 

3,  4 

•/ 

3 


For  ?*j = Ta  =  v-,  •• 
these  terms  are 


or  zero. 

For  (fj,  /•2)  = 


these  terms  are  each  unity  ;  for 
(»"i,  »-2)  =  (i»  *),     ("i»  "2)  =  (3, 


—  < 

3 


i=l+e     3     -+e     s 
D>  ("D  "2)  =  (^j  2),  these  terms  are 

_2™  2_™(2) 


361.     We  give  now  an  example  of  the  expression  of  <£  functions. 
Take  the  case  in  which  p  =  l,  and 

0    -3 
3       0 


361]  OF   A  JACOBIAN    FUNCTION.  597 

the  conditions  ab  —  ba  =  k,  and  geg  =  k,  if  a  =  (a,  a),  b  =  (b,  b'),  become 

ab'  -a'b  =  -  3,       g^g*  -  9u(/^  =  -  3 ; 
taking  for  instance 

4     5 

1     2    ' 

we  have,  if  x  =  (x,  x'),  xl  =  (xl)  &•/),  and  ax  +  ax  =  0,  the  equation 
.,  9m/     '       '    \-      3tV#/ ,  ,  ,   __  QX'XI        ,       , 

i/K/XJU-^  ~—  Ot-  ( JuJU-^   *"""  CG  &\)  ^~  ~~^  '     \CL  CL-\  "™~  CL'd-\   )  •— —  (  Ct/j    *~*  OL  yO  ) 

tZCvj  CLCt~\ 

where  a  =  a.  +  i/3,  a  —  a.'  +  ift'.     Thus,  beside  ab'  —  ab  =  -  3,  we  must  have 
a/3'  >  a'ft.     The  quantities  a,  b,  a,  b'  are  otherwise  arbitrary. 

The  equations  a  =  Kg,  b  =  Lg  give  (a,  a'}  =  (4-K  +  K',  oK  +  *2K') ;  there 
fore 

3JT  =  2a  -  a'  ,     3L  =  26  -  b'  , 

further  the  equation  c  =  gC  +  %  [g]  gives 


4    1 


,  C")  +  £  (4,  10)  =  (46'  +  (7  +  2,  5C'  4-  2C"  +  5), 


.5    2 
so  that 

3a=2c-c/+l,     W  =  4c' -  5c  -  10. 

Also,  from  K=\'2(o,  2o/ 1 ,  2-iriL  =  ,  2?;,  2?;'  | ,  with 


we  obtain 

a  =  7rt(26-6')/(2a-a'),     b  =  7ri(4a'-  5a)/(2a-a'),     h  =  3iri/(2a  -  a'). 

If  then  S-  (u  ;  (7)  denote  the  theta  function,  with  characteristic  [     n,  }  , 

\-C  J' 
given  by 

^  (u  ;   (7)  =  2eaM2+2hM(w+C)+b(«+C')!'  ~2*iC'  (n+C) 


then  the  Jacobian  function,  with  a,  b  as  periods,  and  c  as  parameter,  is  given 

by 


where,  in  the  three  terms  of  the  right  hand,  r'  is  in  turn  equal  to  i° 
/1/3N     /2/3N 

\2/3j  '  u/3;  • 

The  function  <f>(u)  may  in  fact  be  considered  as  a  theta  function  of  the 
third  order  ;  its  various  expressions,  obtainable  by  taking  different  forms  for 
the  matrix  g,  are  transformations  of  one  another,  in  the  sense  of  Chap.  XVIII 


and  XX. 


598  THE   CASE   WHEN   a  <  2p.  [362 

362.  The  theory  of  the  expression  of  a  Jacobian  function  which  has 
been  given  is  for  the  case  when  a-  =  2p.  Suppose  cr  <  *2p,  and  that  we  have 
two  matrices  a,  b,  each  of  p  rows  and  a-  columns,  such  that  ab  —  ba,  =  k,  is  a 
skew  symmetrical  matrix  of  integers,  for  which  ikxx^  is  a  positive  form  for 
all  values  satisfying  ax  =  0,  other  than  those  for  which  also  a^x  =  0,  or  x  =  0  ; 
then  it  is  possible*  to  determine  other  2p  —  a  columns  of  quantities,  and 
thence  to  construct  matrices,  A,  B,  of  2p  columns  (whereof  the  first  <r 
columns  are  those  of  a,  b),  such  that  AB  —  BA  =  K  is  a  skew  symmetrical 
matrix  of  integers  for  which  iKxxl  is  positive  when  Ax=0,  except  when 
x=  0  or  A-^x-=  0. 

There  will  then  correspond  to  the  set  A,  B  a  function  <I>,  involving  ^\K\ 
arbitrary  coefficients,  such  that,  for  integral  n, 


The  function  <£  (u),  which  is  subject  only  to  the  condition  that 


is  then  obtained  by  regarding  <£  (u)  as  a  particular  case  of  <I>  (u),  in  which 
the  added  columns  in  A,  B  are  arbitrary  except  that  they  must  be  such  that 
the  necessary  conditions  for  A,  B  are  satisfied. 

For   further  development    the  reader  should  consult   Frobenius,  Crelle, 
xcvii.  (1884),  pp.  16,  188,  and  Crelle,  cv.  (1889),  p.  35. 

*  Frobenius,  Crelle,  xcvn.   (1884),  p.  24. 


363] 


CHAPTER   XX. 

TRANSFORMATION  OF  THETA  FUNCTIONS. 

363.  IT  has  been  shewn  in  Chapter  XVIII.  that  a  theta  function  of  the 
first  order,  in  the  arguments  u,  with  characteristic  (Q,  Q'),  say  S-  (u,  Q),  may 
be  regarded  as  a  theta  function  of  the  r-th  order  in  the  arguments  w,  with 
characteristic  (K,  K'),  provided  certain  relations,  (I),  (II),  of  §  322,  p.  532,  are 
satisfied.  Let  this  theta  function  in  w  be  denoted  by  II  (w,  K).  We  confine 
ourselves  in  this  chapter,  unless  the  contrary  be  stated,  to  the  case  when 
(Q>  Q')  is  a  half-integer  characteristic.  Then  the  function  *b(u,  Q)  is  odd  or 
even ;  therefore,  since  u  =  Mw,  the  function  II  (w,  K}  is  an  odd  or  even 
function  of  the  arguments  w.  Now  we  have  shewn,  in  Chap.  XV.  (§  287), 
that  every  such  odd,  or  even,  theta  function  of  order  r,  is  expressible  as  a 
linear  function  of  functions  of  the  form 

•tyr(w\  K,  K'  +  //,)  =  S-    rw  ;  2u,  2?V,  2f/r,  2£'  **  +  ^'r 
I  K        J 

(K'  4-  LL\ 
-rw\  2v,  2n/,  2£/r,  2f  v         ™ 

K 

where  e  is  +  1,  according  as  the  function  is  even  or  odd.  The  most  important 
result  of  the  present  chapter  is  that  the  functions  tyr  (w ;  K,  K'  +  p)  which 
occur  can  be  expressed  as  integral  polynomials  of  the  r-th  degree  in  2*>  theta 

(n'\ 
w ;    2v,  2v',  2£  2%'        ) ,  whose  characteristics  are  those  of  a 
:  It  J 

Gopel  system  of  half-integer  characteristics  (Chap.  XVII.,  §  297) ;  the  earlier 
part  (§§  364 — 370)  of  the  chapter  is  devoted  to  proving  this  theorem. 

The  theory  is  different  according  as  r  is  odd  or  even.  When  r  is  odd, 
e  is  ewi]Q],  and  we  have  shewn  (§  327  Chap.  XVIII.)  that,  for  odd  values  of  r, 
\Q\  =  \K\,  (mod.  2) ;  the  theory  deals  then  only  with  functions 

* 

\lrr  (w  ;  K,  K'  +  //.) 


600  GENERAL   STATEMENT.  [363 


in  which  e  =  elrfl-K'1.  When  r  is  even,  e,  though  still  equal  to  e77*^1,  may  or 
may  not  be  equal  to  e7™1  Kl,  according  to  the  integer  matrix  which  determines 
the  transformation  ;  but  in  this  case,  also,  the  value  of  e  in  the  functions 
tyr(iu;  K,  K'  +  /LI)  which  occur  is  determinate. 

The  proof  of  the  theorem  is  furnished  by  obtaining  actual  expressions  for 
the  functions  ^rr  (w  ;  K,  K'  +  /*)  as  integral  polynomials  of  the  r-th  degree  in 

/  R'\ 

the  2?  functions  $•  I  w  ;  2v,  2t/,  2£  2£"  j  '     )  ;  the  coefficients  arising  in  these 
\  |  -R  / 

polynomials  are  theta  functions  whose  arguments  are  r-th  parts  of  periods, 
of  the  form  (2vm  +  2i/w')/r.  The  completion  of  the  theory  of  the  trans 
formation  requires  that  these  coefficients  should  be  expressed  in  terms  of 
constants  depending  on  theta  functions  with  half  integer  characteristics 
(§  373). 

Further  the  theory  requires  that  the  coefficients  in  the  expression  of  the 
function  II  (w  ;  K}  by  the  functions  ^,,  (w  ;  K,  K'  +  /A)  should  be  assigned 
in  general.  In  simple  cases  this  is  often  an  easy  matter.  The  general  case 
is  reduced  to  simpler  cases  by  regarding  the  general  transformation  of  the  r-th 
order  as  arising  from  certain  standard  transformations  for  which  there  is  no 
difficulty  as  to  the  coefficients,  by  the  juxtaposition  of  linear  transformations 
(||  371—2)*. 

364.  It  follows  from  §  332,  Chap.  XVIII.  that  any  transformation  may 
be  obtained  by  composition  of  transformations  for  which  the  order  r  is  a 
prime  number.  It  is  therefore  sufficient  theoretically  to  consider  the  two 
cases  when  r  =  2,  and  when  r  is  an  odd  prime  number.  We  begin  with  the 
former  case,  and  shew  that  the  transformed  theta  function  can  be  expressed 
as  a  quadric  polynomial  in  2^  theta  functions  belonging  to  a  special  Gb'pel 
system.  A  more  general  expression  is  given  later  (§  370). 

*  For  the  transformation  of  theta  functions,  and  of  Abelian  functions,  the  following  may  be 
consulted.  Jacobi,  Crelle,  vm.  (1832),  p.  416  ;  Eichelot,  Crelle,  xn.  (1834),  p.  181,  and  Crelle, 
xvi.  (1837),  p.  221  ;  Eosenhain,  Crelle,  XL.  (1850),  p.  338,  and  Mem.  par  divers  Savants,  t.  xi. 
(1851),  pp.  396,  402;  Hermite,  Liouville,  Ser.  2,  t.  in.  (1858),  p.  26,  and  Comptes  Rendus,  t.  XL. 
(1855);  Konigsberger,  Crelle,  LXIV.  (1865),  p.  17,  Crelle,  LXV.  (1866),  p.  335,  Crelle,  LXVII.  (1867), 
p.  58;  Weber,  Crelle,  LXXIV.  (1872),  p.  69,  and  Annali  di  Mat.  Ser.  2,  t.  ix.  (1878);  Thomae, 
Ztschr.  f.  Math.  u.  Phys.,  t.  xn.  (1867),  and  Crelle,  LXXV.  (1872),  p.  224  ;  Kronecker,  Berlin. 
Monatsber.,  1880,  pp.  686,  854  ;  H.  J.  S.  Smith,  Report  on  the  Theory  of  Numbers,  British  Associa 
tion  Reports,  1865,  Part  vi.,  §  125  (cf.  Weber,  Acta  Math.,  vi.  (1885),  p.  342;  Weber,  Elliptische 
Functionen  (1891),  p.  103;  Dirichlet,  in  Riemann's  WerJce  (1876),  p.  438;  Cauchy,  Liouville,  v. 
(1841),  and  Exer.  de  Math.,  n.,  p.  118;  Gauss,  Werke  (1863),  t.  n.,  p.  11  (1808),  etc.;  Kronecker, 
Berlin.  Sitzungsber.  1883  ;  Frobenius,  Crelle,  LXXXIX.  (1880),  p.  40,  Crelle,  xcvn.  (1884),  pp.  16, 
188,  Crelle,  cv.  (1889),  p.  35  ;  Wiltheiss,  Crelle,  xcvi.  (1884),  p.  21  ;  the  books  of  Krause,  Die 
Transformation  der  Hyperelliptischen  Functionen  (1886),  (and  the  bibliography  there  given), 
Theorie  der  Doppeltperiodischen  Functionen  (1895)  ;  Prym  u.  Krazer,  Neue  Grundlagen  einer 
Theorie  der  allgemeinen  Thetafunctionen  (1892),  Zweiter  Teil.  See  also  references  given  in 
Chap.  XXI.,  of  the  present  volume,  and  in  Appendix  n. 


*C\BRT^ 

OF   TTTF 

UNIVERSITY 


364]  TRANSFORMATION   OF   THE   SECOND   ORDER.  601 

By  means  of  the  equations  u  =  Mw,  a  function  S-  fn ;  2w,  2<w',  2?;,  2rj'       } , 

with    half-integer    characteristic    (      ] ,   becomes    a    theta    function   in   lu, 

\Q  I 

n  (w ;  K,  K'},  of  order  2,  with  the  associated  constants  2u,  2i/,  2£  2^'  and 
the  characteristic  (K,  K'),  where  (§  324,  Chap.  XVIII.) 

•  2o//3', 


=  &&     a/3'  -  a'yS  =  /8'a  -  y8a'  =  2  ; 


and 


this  theta  function  in  w,  U(w;  K,  K'),  can  by  §  287,  p.  463,  be  expressed  as 
a  linear  aggregate  of  terms  of  the  form 


;  2u,  2n/,  2 


-  rw 


',  2(r/r, 


r  being  equal  to  2  ;  here  e,  =  eMQQ'  ,  is  +  1,  according  as  the  original  function, 
that  is,  according  as  the  function  II  (w  ;  K,  K'},  is  even  or  odd.  For  brevity 
we  put  w  =  2vW,  VT'  =  V,  and  denoting  by  @  (W,  r)  the  series 
we  consider  the  function 


.8 


[-rF;  »V  (A"+f/r], 


which  is  equal  to  e-Mv~lvfltyr(w  ;  -ff",  K'  +  p}.     Throughout  the  chapter  the 

/      K'\        f      I  ^'\ 
symbols  ^  (  w        }  ,  ®  (W  •      }  denote  respectively 

\        K.  /  \       I  K  / 


;  2u, 


/o'\     /r'\ 
Taking  the  final  formula  of  §  291,  p.  472,  replacing  co,  •',  1^,  9,  (     ),  I    J 

respectively  by  v,  v,  f,  5",  -|(a  )  ,  %{    }  +  (  K  }  ,  multiplying  both  sides  of  the 

\ct  j       \a  /      \  K  I 


equation  by  e«a(M-tf'-<O;  where  ft  is  a  row  of  integers  each  either  0  or  1,  and 
adding  the  %'  equations  obtainable  by  giving  a  all  values  in  which  each  of  its 
elements  is  0  or  1,  we  obtain 


602 


EXPRESSION    OF   THE   TRANSFORMED    FUNCTION 


[864 


V 


•IT' 


'  +  *') 
K 


and  hence,  replacing  V,  U  respectively  by  W,  0, 


2F"; 


i-*'} 


This  may  be  regarded  as  the  fundamental  equation  for  quadric  transformation  ; 
we  consider  various  cases  of  it. 

(i)     When  (K,  K')  is  the  zero  characteristic  we  obtain 


;  2r' 


: 


the  right-hand  side  being  independent  of  a',  which  for  simplicity  may  be 
put  =  0. 

We  can  infer  that  in  any  quadric  transformation,  when  the  transformed 
function  has  zero  characteristic,  it  can  be  expressed  as  a  linear  aggregate  of  the 

,  in  which  «'  is  an  arbitrary  row  of  integers  (each  0 


z^  squares  5r  I  w 

or  1)  and  a  has  all  possible  values  in  which  its  elements  are  either  0  or  1. 
(ii)     When  JK'  =  Q,  K=^n  is  not  zero,  we  obtain 


where  on  the  right  side  only  2^-1  terms  are  to  be  taken  in  the  summation  in 
regard  to  a,  two  values  of  a  whose  difference  is  a  row  of  elements  congruent 

(mod.  2)  to  the  elements  of  n  not  being  both  admitted.     When  jH     )  is  an 


even  characteristic  we  may  put  a'  =  0 ;  when  Jj       is  an  odd  characteristic  we 


may  put  a'  =  /i. 

In  this  case,  as  before,  only  2^  theta  functions  enter  on  the  right  hand, 
and  their  characteristics  form  a  special  Gopel  system. 

The  cases  (i)  and  (ii)  give  the  transformation  of  any  theta  function  when 
the  matrix,  of  2p  rows  and  columns,  associated  with  the  transformation*  is 


For  the  notation,  cf.  Chap.  XVIII.,  §§  322,  324.. 


365]  BY   MEANS   OF   A   CERTAIN   GOPEL   SYSTEM.  603 

/20 

(         .     It  can  be  shewn  that  by  adjunction  of  linear  transformations  every 

quadric  transformation  is  reducible  to  this  case  (cf.  §  415  below);  so  that 
theoretically  no  further  formulae  are  required.  As  it  may  often  be  a  matter 
of  difficulty  to  obtain  the  linear  transformations  necessary  to  reduce  any  given 
quadric  transformation  to  this  one,  it  is  proper  to  give  the  formulae  for  the 
functions 

2r'   *"^1  +«6  F-2TT    2r' 


by  this  means  the  problem  is  reduced  to  finding  the  coefficients  in  the 
expression  of  any  theta  function  in  w,  of  the  second  order,  in  terms  of 
functions  W2(W;  K,  K'  +  yu.)  (see  §  372  below).  Hence  we  add  the  following 
case. 

(iii)     When  K'  is  not  zero,  we  deduce,  by  changing  the  sign  of  W  in  the 
fundamental  formula,  the  equation 


; 


2r'  2(JF;  K, 


; 


where,  putting  K=  |&,  K'  =  ^lc,  we  have  Ca  =  1  +  eeniklk'+a'}+niak'  .  When  e  is 
+  1,  there  are  2f~l  values  of  a  for  which  atf  =  k(k'  +  a')  +  1  (§  295,  Chap.  XVII.); 
for  these  values  Ga  =  0  ;  when  e  =  -l,  there  are  2?-1  values  of  a  for  which 
ok'  =  k  (kr  +  a')  ;  for  these  values  Ca  =  0.  In  either  case  it  follows  that  the 
right  side  of  the  equation  contains  only  2?~l  terms,  and  contains  only  2^ 
theta  functions  whose  characteristics  are  a  special  Gopel  system. 

It  is  easy  to  see  that  the  results  of  cases  (ii)  and  (iii)  can  be  summarised 
as  follows:  when  the  characteristic  (K,  K')  is  not  zero  the  transformed  function 
is  a  linear  aggregate  of  2*-1  products  of  the  form  ^  [w  ;  A,  P{]  ^  [w  ;  A,  K,  P,:] 

wherein  the  2"-1  characteristics  P{  are  of  the  form  |  fj  ,  K=(K   },  and 

\a/  V—  K) 

A,  K  are  such  that*  e"*i  *i  +»*  i  A  *i  =  e. 

These  results  are  in  accordance  with  §  288,  Chap.  XV.  ;  there  being 
2P-i  (1  +  e)  linearly  independent  theta  functions  of  the  second  order  with 
zero  characteristic  and  of  character  e,  namely  2*>  such  even  functions  and  no 
odd  functions,  and  there  being  2?-1  linearly  independent  theta  functions  of 
the  second  order  with  characteristic  other  than  zero. 

365.      Ex.   i.      When    p  =  l,    the    results    of    case    (i),   if    we    put   egh(W;   r')   for 
9  I  w  >  T'  k  (  _  f  )  I  ,  as  is  usual,  are 

800(2  w-  yj-^^^+oiiWO    eL(jV 
2000(20  -ae 

*  For  the  notation,  see  Chap.  XVII.,  §  294. 


604  TRANSFORMATION   OF  THE   SECOND   ORDER  [365 

and 


where  e  (2r')  denotes  e  (0  ;  2r').     If  then  we  introduce  the  notations 

VI    e^r')  e01(2r')       /X_e10(r')       /r>_e01(r') 

'         "''    VX-~         VX- 


4  v_ 

;  2r')'  ~  V  *  001  (2  TF;  2r')  '         *  ~         001  (2  W-  2r')' 

r') 
;  r')' 


=  -1  ^liJ^JL)  ./-      A  A!  Qio(JF;j-')  i/?-^6"^  r') 

VAe01(JF;  r')'          V>?-  V   X  601(Pf;  r')'          Vf~VX  e 


we  find  by  multiplying  the  equations  above  that 


and  therefore  that 
so  that  also 


while,  comparing  the  two  forms  for  0^  (2  IF;  2r'),  putting  1F=0,  we  obtain 

/  /         X  ,     1  —  X'        .   .  2  V^ 

giving   K* 


further  the  equations  for  600(2  W;  2/)  and  010(2TF;  2r')  give  the  results 


from  which  we  find 

r?  =  l-£,  C=1-X^;  thus  also  //  =  1-A-,  z  =  I-k'*x. 

Ex.  ii.     The  equations  of  case  (ii),  also  for  p  =  l,  give 

eol(2if;  ^^(^O^^O  20=e10(ir;.Qe 

yoi  V^r  ->  60i  (2r  ) 

From  these  we  have  by  division 


while  from  these  and  the  results  of  Ex.  1,  we  find 

]/  Vi^X^,   \/~z=  [i  -  (i  -  x')  ^l/Vr^W- 


t-.  iii.     When  p  =  1,  by  considering  the  change  in  the  value  of  the  function 

3*  (w]  —  P11 

^ 


when  ?y  is  increased  by  a  period,  we  immediately  find  that  it  is  a  theta  function  in  w  of 
the  second  order  with  characteristic  £  (j  •   hence  by  the  result  of  case  (iii)  above,  the 

function  is  a  constant  multiple  of  310  (w)  Sw  (w)  ;    determining  the  constant  by  putting 
iv  =0,  we  obtain  the  equation 

©oo(Oe10(r')[0'u(TF;  r')001(JF;  r')-e'ol(JF;  r)0n(IF;  r')] 
=  e'u  (r')  001  (r')  610  (  W',  r')  0oo  (  W;  r'), 


365]  IN   THE    ELLIPTIC   CASE. 

which  is  immediately  seen  to  be  equivalent  to 

e'u(r')  600(1-')  w=  ft  d£ 

©01  (O  e10  (r')        J  0 


605 


[We  may  obtain  the  theta  relation,  here  deduced,  from  the  addition  formula  of  Ex.  i., 
§  286,  p.  457  ;   taking  therein  m  =  $(     ^\  ,  a^=\  (  _  A  ,  «2  =  |  (  _  i)  '  W=G>  ?  =  ^  (Q)  ' 

r=p  =  %  (    )  ,  we  immediately  derive 

^10  (w)  Soo  («)  3U  (2»)  V  (0)  =  5oo  («0  310  («0  [$oi  0*  -  *>) 


if,  for  small  values  of  v,  this  equation  be  expanded  in  powers  of  v,  and  the  coefficients  of  v 
on  the  two  sides  be  put  equal,  there  results  the  equation  in  question.] 

Ex.  iv.  By  differentiating  the  second  result  of  Ex.  ii.,  putting  TP=0,  and  putting 
TF=0  in  the  first  result  of  the  same  example  and  in  the  second  value  for  600(2  W;  2i-')  in 
Ex.  i.,  we  obtain 


600  (2r')  601  (2r')  610  (2r')      6^  (r')  601  (r')  610  (r)  ' 

so  that  the  second  of  these  functions  is  unaltered  by  replacing  T  by  2'V,  n  being  as  large 
as  we  please.  Hence  we  immediately  find  from  the  series  for  the  functions,  by  putting 
T  =  oc  ,  that  each  of  these  fractions  is  equal  to  TT.  Hence  if  the  integral  occurring  in  the 
last  example  be  denoted  by  J  we  have  ,7=776^  (r)  W.  In  precisely  the  same  way  we  find 
7=2776^(21-')  W,  where  7  is  an  integral  differing  only  from  J  by  the  substitution  of  x  for  $ 
and  k  for  X.  Hence 


as  follows  from  the  first  result  of  Ex.  1. 

From  these  results  we  are  justified  in  writing  the  formula  of  Ex.  ii.  in  the  form 


'  T+X'~  dn(/,X) 

and  this  is  Landen's  first  transformation  for  Elliptic  functions. 

Ex.  v.     The  preceding  examples  deal,  in  the  case  p  =  1,  with  the  quadric  transformation 
associated  with  the  matrix  (        j  .     Prove  when  p  =  1  that  for  any  matrix  of  quadric 

transformation  the  transformed  theta  function  is  expressible  linearly  in  terms  of  one  or 
more  of  the  eight  functions 


6  = 


;  2r'), 


2  =  610(2TF;  2r'), 
6  (W;  2r' 


=  601  (2  W;  2r'), 


j  2r'), 


4)-  6  (2  IF;  2r' 


-^2  TF; 


67  =  6    2  TT; 

Prove  in  particular  that  the  functions  arising  for  the  transformation  associated  with 

the  matrix  (       )  are  expressed  as  follows  : 
\U  ^/ 

,    e,0(Tr;  ^-')=e4,    en(Tf;  £i-')=-tea; 


606  EXAMPLE    OF   THE    ELLIPTIC    CASE.  [365 

and  that  the  functions  arising  for  the  transformation  associated  with  the  matrix  (       )  are 

\U  2J 

expressed  as  follows  : 

©oo(^;  £r'-i)  =  e-ie2,     e01(TF;  £r'-|) 


_ 

ew(W;br'-to  =  e    ~^  ee,     eu(  W;  £r'-|)  =  e8  er. 

Obtain  from  the  formulae  of  the  text  the  expressions  of  the  functions  64,  05,  86,  07  of 
the  form 


),  e5=6'5e01(TF)en(TF),  ec=<70e01(TF)e10(TF),  er=C'7 

where  6'4,  C5,  Ce,  C"r  are  constants. 

Ex.  vi.     The  reason  why  the  matrices  (A1),  (A0),  (no)  are  selected  in  Ex.  v.  will 

\u  i/     \u  //     \u  zj 

appear  subsequently  (§  415)  ;  the  matrix  (        )  gives  the  transformation  which  is  supple- 

U  / 


mentary  to  that  given  by  L     J  ;  it  gives  results  leading  to  the  equation 
sn  [(1  +k)  u,  2 


by  combination  of  these  results  with  those  for  the  matrix  (        j  we  obtain  the  multiplica 

tion  formula 

0n(2TF;  r')  =  ^en(TF;  r')e01(Pf;  r')e10(^;  r')6oo(TF;  r'), 

where  ^  is  a  constant  (cf.  Ex.  vii.,  §  317,  Chap.  XVII.  and  §  332,  Chap.  XVIIL). 
The  matrix  associated  with  any  quadric  transformation  can  be  put  into  the  form 


where  fl,  Q'  are  matrices  of  linear  transformations  ;  for  instance  we  have 

0  -  1\  /2  0\  /     0  1\  _  /I  0 
Oj  (o  l)  V-l  0/~  \02 

with  the  corresponding  equations 

U=rW^      TF1  =  2TF2,      >F2=-r2PF3;         r^-l/r,     r2  =  r1/2,     rs=-l/r2, 
from  which  we  have,  for  instance, 


-  901  (2  TF2  ;  2r2) 

=  e~  -      EQm(  TF2  ;  r2)  G01  (  T<F2  ;  r2)  =  ^e^  (  TF3  ;  r3)  010  (  TF3  ;  r3), 

(E,  F  being  constants)  whereby  the  transformation  formula  for  010  (  TF3  ;  ^r3)  is  obtained 
from  those  for  610(2  TF;  2r'),  with  the  help  of  those  arising  for  linear  transformation. 

366.  We  pass  now  to  the  case  when  the  order  of  transformation  is  any 
odd  number,  dealing  with  the  matter  in  a  general  way.  Simplifications  that 
can  theoretically  be  always  introduced  by  means  of  linear  transformations  are 
considered  later  (§  372). 


360]  TRANSFORMATION    OF    ANY    ODD    ORDER.  607 

We  first  investigate  a  general  formula*  whereby  the  function 


can  be  expressed  in  terms  of  products  of  functions  with  associated  constants 
2v,  2t/,  2£,  2£'.  We  shall  then  afterwards  employ  the  formulae  developed  in 
Chap.  XVII.,  to  express  these  products  in  the  required  form. 

Let  a,  a-'  be  two  matrices  each  of  p  rows  and  m  columns,  whose  constitu 
ents  are  any  constants  ;  let  the  j-th  columns  of  these  be  denoted  respectively 
by  <r®  and  <r'&,  so  that  the  values  of  j  are  1,  2,  ...,  m;  let  T,  denote  the 
matrix  2v<7  +  2i/<r',  which  hasp  rows  and  m  columns,  and  let  the  j-th  column 

J 


of  this  matrix,  which  is  given  by  2i;o-(^  +  2wV^,  be  denoted  by  TVJ  ;  also, 
K,  K'  being  rows  of  any  p  real  rational  elements,  let  TK,  ZK  denote  the 
rows  2vK+  2v'K',  2£K+2£'K'  ;  and  use  the  abbreviation 
«•  (w  ;  K,  K')  =  ZK  (w  +  %TK)  -  TriKK'  ; 

finally,  let  s  =  (s(1),  ...,  s(w))  be  a  column  of  m  integers  whose  squares  have 
the  sum  r,  so  that 


then,  using  always  ^  (w)  for  ^  (w  ;  2v,  2i/,  2^,  2^)>  the  function 
Uw  =  e~  rw  lw  '  K^  K'W  3  ^ 


is,  m  w,  a  theta  function  of  order  r  with  associated  constants  2u,  2u',  2f,  2£' 
characteristic  (K,  K'}. 

For  when  the  arguments  w  are  increased  by  the  elements  of  the  row 
where  N,  N'  are  rows  of  p  integers,  the  function 


is  multiplied  by  a  factor  e*i,  where  tyj  is  equal  to 


that  is 


the  sum  of  the  m  values  of  ^-  is  given  by 


7  =  1 

*  Konigsberger,  Crelle,  LXIV.  (1865),  p.  28.     See  Eosenhain,  Crelle,  XL.  (1850),  p.  338,  and 
M£m.  par  divers  Savants,  t.  xi.  (1851),  p.  402. 


608  THE   FIRST   STEP   IN   THE  [366 

also,  when  w  is  increased  by  Ty,  the  function  —  rtx  [w  ;  K/r,  K'\r)  is  increased 
by  —  ZjrTA-;  thus  the  complete  resulting  factor  of  II  (w)  is 


of  which  (§  190,  p.  285)  the  exponent  is  equal  to 

m  (w  ;  N,  N'}  +  Ziri  (NK'  -  N'K)  ; 

thus  (§  284,  p.  448)  II  (w)  is  a  theta  function  in  w,  of  the  r-th  order  with 
(K,  K')  as  characteristic. 

Therefore  (§  284,  p.  452)  we  have  an  equation 

II  (w)  =  2  A^  \rw  ;  2v,  2rv',  2£/r,  2£'   ^'  + 
n  L  K 

where  yu,  is  a  row  of  p  integers  each  positive  (including  zero)  and  less  than  r, 
and  the  coefficients  A^  are  independent  of  w.  The  coefficients  A^  are  inde 
pendent  of  K,  K',  as  we  see  immediately  by  first  proving  the  equation  which 
arises  from  this  equation  by  putting  K  and  K'  zero,  and  then,  in  that  equation, 
replacing  w  by  w  +  ZvKjr  -f-  2v'K'/r. 

In  this  equation,  replace  K  by  K  +  h,  where  h  is  a  row  of  p  integers,  each 
positive  (including  zero)  and  less  than  r  ;  then,  using  the  equation  previously 
written  (§  190,  p.  286),  for  integral  M,  in  the  form 

*(u;  q  +  M}  =  e^iM(i^(u\  q\ 
we  find 


-  rat  [w  ;  (K+  h)jr,  K'/r]  -  2«  (K'  +  e)  ft/r  g  ^       (}) 

j=i 


rw ;  2v, 

K 

where  e  is  taken  to  be  any  row  of  p  integers  each  positive  (or  zero)  and  less 
than  r ;  ascribing  now  to  h  all  the  possible  r?  values,  and  using  the  fact  that 

h 

according  as  /*  —  e  =  0  or  ^  0,  (mod.  r),  we  infer,  by  addition,  the  equation 
C^    rw ;  2v,  2n/, 


v>  +  -  I  +  TJ 

h      j=i     |_       \  r 

where 

•^r  =  —  TOT  [w ;  {K  +  h)/r,  K'/r]  —  2jri  (K'  +  /A)  hfr, 

and  C^,  =  rPAp,  is  independent  of  w  and  of  the  characteristic  (K,  K'). 


367]  TRANSFORMATION   OF   ODD   ORDER.  609 

367.     We  put  down  now  two  cases  of  this  very  general  formula  :  — 

(a)     if  each  of  the  matrices  <r,  a-'  consist  of  zeros,  and  each  of  the  m 
integers  s(1),  ...,  s(m)  be  unity,  so  that  m  =  r,  we  obtain 


,  2n/,  2£/r,  2£' 

r'  K  '^  ~  ir  r   w  +  - 


r 

In  using  this  equation  we  shall  make  the  simplification  which  arises  by 
putting  w  =  2u  W,  v~lv  =  r,  and 

@  (  W,  r)  =  e-M-w  *  (w)  =  2e*riwr»+*T'»8; 

71 

then  the  equation  can  be  transformed  without  loss  of  generality,  by  means  of 
the  relations  connecting  the  matrices  v,  v,  f,  £'  (cf.  §  284,  p.  447),  to  the  form 


(I) 


(7  e-<twiK"\_W+WK'lr-\-lTnKK'lr®     rW,  TT 


where  Cy  is  independent  of  W  and  of  K  and  K'. 

This  equation  is  of  frequent  application  in  this  chapter  ;  it  is  of  a  different 
character  from  the  multiplication  formula  given  Chap.  XVII.,  §  317,  Ex.  vii., 
whereby  the  function  ©  (rW,  r')  was  expressed  by  functions  @(W,  r')  with 
different  characteristics  but  the  same  period,  r'. 

Ex.  \.     When  r  =  2,  p  =  2,  we  have 

F,  2r')=e2(Tru  wz-  r'j+e^i^+i,  TF2;  r')+  e2(iF15  ^2+i;  r') 


Ex.  ii.     If  X,  /LI,  /i  be  rows  of  p  integers  each  less  than  r,  prove  that  the  ratio 

2<r*n^/rer  T  |p+  J    X/rH     ^^^.p^  T  Tf+  AJ 

is  independent  of  W. 

(/3)  if  the  matrix  or'  consist  of  zeros,  and  if  each  of  the  m  integers 
sw,  ...,  s(m)  be  unity,  so  that  m  =  r,  and  if  the  matrix  <r,  of  p  rows  and  r 
columns,  have,  for  the  constituents  of  every  one  of  its  rows,  the  elements 


i  ? 

, 

r     r 


then   the   matrix    Tff  will  have,  for  the  constituents  of  its  i-ih  row,  the 
elements 


H.  39 


610  THE   FIRST    STEP.  [367 

where  fl;  is  the  sum  of  the  elements  of  the  i-ih  row  of  the  matrix  2i>, 

so  that 

p 

fit  =  2  2  vi  h  ; 

A  =  l 

also  the  *-th  of  the  p  elements  denoted  by  -  T^s  will  be 

(r-i)nri_r-i 

~ 


and  therefore  the  i-th  of  the  elements  of  T^  --  T0s  will  be 

r 


r  2r 

Thus,  denoting  the  row  (fllf  ...,  flp)  by  ft,  the  theorem  is 


A     ,-=i 

where  -^  has  the  same  value  as  in  §  366.     And  as  before  this  result  can  be 
written  without  loss  of  generality  in  the  form 


[rW,  rr'  / 


where  U  '=  W  —  (r  —  l)/2r  and,  for  any  value  of  u, 

<j)(u)  =  ®(u;  r)  0  (  u  +  -  ;  r'j  ......  6  f  w  +  7     -  ;  T'  J  ; 

the  number  of  different  terms  on  the  right  side  of  this  equation  is  r?~l  ; 
for  if  m  be  a  positive  integer  less  than  r,  the  two  values  of  h  expressed  by 
h  =  (hrl>  ...,  hp)  and  h  =  (h1',  ...,  hp'\  in  which  h^li^  +  m,  ...,  hp'  =  hp+m, 

s      i     \     •      ±1,  ^      f     ^fTT,h  +  ]K:  +  r^\ 

(mod.  r),  give  the  same  value  tor  <p  I  u  H  --  •  I  . 

Ex.  i.     For  j»  =  2,  r=2,  we  obtain 

')e(F1+J,  JT2  +  i;  r') 

+i,  TF2-i;  r'JeC^-i,  TT2  +  |;  r'). 


r.  ii.     For  jo  =  2,  r=3,  we  obtain,  omitting  the  period  r  on  the  right  side, 
r')  =  e(TT1,  ^0(1^-1,  Tf2-J)9  (W,+^,  TT2+i) 


368] 


THE   SECOND   STEP. 


611 


368.     We  consider  now  the  expression  of  the  function 

%(r;  K,K-  +  rt-»[rW;  rr'  (A"  +  ")/r]  +  e©  \-rW  ;  rr'  j  <""'  +  *> 

[•  jR'~l 
W  ;    T'  i         ,  in  the  case  when  ?*  is  odd.     We 

suppose  as  before  (K,  K')  to  be  a  half-integer  characteristic,  and  we  suppose 
e  =  e*i\K\^  so  ^hat  e  is  +  i  according  as  the  characteristic  (K,  K')  is  even  or 
odd*.  It  follows  from  §  327,  Chap.  XVIII.,  if  (K,  K')  has  arisen  by  trans 
formation  of  order  r  from  a  characteristic  (Q,  Q'),  that  e  is  also  equal  to  ewi  '  ^  ' 
and  is  +  1  according  as  the  function  is  even  or  odd. 

It  is  immediately  seen  that  equation  (I)  (§  367)  can  be  put  into  the  form 


h  r  J 

from  this  equation  by  changing  the  sign  of  W,  we  deduce  the  result 


where  we  have  replaced  ee~^irKK'  ,  =  ee-™-\K\  by  unity,  and  a  denotes  the 
expression  [h  -(r-l)  (K  +  r'K')]/r,  which  is  an  r-th  part  of  a  period.  We 
proceed  to  shew  that  the  function 


K 


i  (r-l)  K'WQr 


can  be  expressed  as  an  integral  polynomial  of  the  r-tli  degree  in  2^  functions 
©'•[I'F;  T'  APi],  where  APt  are  the  characteristics  of  any  Oopel  system  of 
half-integer  characteristics  whereof  (K,  K')  is  one  characteristic. 

From  the  formula  of  §  311,  p.  513,  putting  C=0,  A'  =  A,B  =  P  =%(q'}  , 

fP  \        /  P  \ 
and   replacing  U,   V,   W,   fVJ  €i,  (jM  e;  respectively  by  Tf,  a,  b,  €i,  e,-  we 

obtain,  if  Pa  = 


*  Thus,  when  2(K' +  /j.)-rm,  m  being  integral, 

e_e2iriK(rm-2p)_  ZwiKm_ 
as  in  §  287,  Chap.  XV.,  and 

tyr(W;  K,  K' +  u.)  reduces  to  29 


K'+u. 


39—2 


612  THE  SECOND  STEP  IN  THE  [368 

;  A) 


;  A  +  P.), 

>     )  *>       o. 

where 


X  (u,  v  ;  P,  e)  =  2e0e-W<?a  0  (M  ;  A  +  P  +  Pa)  ©  [>  ;  4  +  Pa]  ; 

the  function  x(u>  v>  A,  P,  e)  may  be  immediately  shewn  to  be  unaltered  by 
the  addition  of  an  integral  characteristic  to  the  characteristic  P0  of  one  of  its 
terms  ;  we  may  therefore  suppose  all  these  characteristics  to  be  reduced 
characteristics,  each  element  being  0  or  |. 

Hence  we  get 

;  A+Pa)®(W;  A  +  P.), 


and  hence  2^®3(TF+a;  A)  is  equal  to 

^H^ea@(W-  ^+Pa)2#22e/e-^'V?/3@(TF+3a;  A  +  P,L+Pft)®(W;A+Pp), 

e  a.  e'  |3 

where 

77  =  x  (g»  g  ;  °>  6)    77  =  y  (2a>  a  ;  -Pa.  6/)  . 

%(2a,0;0,e)'  X  (3a,  0  ;  P.,  e')' 

proceeding  in  this  way  we  obtain  2(r~1)i}  ©r  (  W+  a  ;  J.) 

2;  CM>,   (ni) 


where  each  of  P0i,  P02,  ...  becomes  in  turn  all  the  characteristics  of  the 
group  (P),  and  e1}  e2,  ...  relate  respectively  to  the  groups  described  by 
Pa,,  Pa.,,  •••,  and  further 


+  l)a,  0;  P0i  +  ...  +  P.^,  em], 
(m=l,  ...,  r-1), 

em  =  eay™@  (  If  ;  ^1  +  P.  J,     X^  =  -  ^TTI  (?'0l  +  ...  +  j'a^^)  ?am, 

(m=l,  ...,r-2). 

The  equation  (III)  expresses  ®r(W  +  a;  A)  as  an  integral  polynomial 
which  is  of  the  (r  -  l)th  degree  in  functions  ©  (  W  ;  J.  +  Pa),  whose  charac 
teristics  belong  to  the  Gopel  system  (AP),  arid  is  of  the  first  degree  in 
functions  ®  [W  +  ra;  A  +P0].  But  it  does  not  thence  follow  when  a  is  an 
r-th  part  of  a  period,  that  ®r(W  +  a;  A)  can  be  expressed  as  an  integral 
polynomial  of  the  r-th  degree  in  functions  @[TT;  .4+P0];  for  instance 
if  the  Gopel  system  be  taken  to  be  one  of  which  all  the  characteristics  are 
even  (§  299,  Chap.  XVII),  it  is  not  the  case  that  the  function  @3  (W  +  £), 


368]  TRANSFORM  ATION  OF  ODD  ORDER.  613 

which  is  neither  odd  nor  even,  or  the  function  ®3(W+  ^)  —  Ba(  W—  £),  which 
is  odd,  can  be  expressed  as  an  integral  polynomial  of  the  third  degree  in  the 
functions  of  this  Gopel  system  ;  differential  coefficients  of  these  functions 
will  enter  into  the  expression.  The  reason  is  found  in  the  fact  noticed  in 
§  308,  p.  510  ;  the  denominator  of  Hr^  may  vanish. 

Noticing  however,  when  P  is  any  characteristic  of  the  Gopel  group 
(P),  that  x(-u,-v;  P,  e)  =  e«i^i+«i^-Pi  x  (u,  v;  P,  e),  so  that  the  co 
efficients  Hm  are  unaltered  by  change  of  the  sign  of  a,  and  putting  the 

(K'\ 
„  J  ,  we  infer,  from  the  equation  (III),  that 


is  equal  to 

2^2  ......  2#r_1|>-2™<»--1>*'^%(TF  +  ra,  W;  P,  eM) 

e,  ai  «r_i 

+  e***W'irx(W-ra,  W  ;  P,  e^)], 

where  P  denotes  Pfli  +  .  .  .  4-  Par  2  ;  and  it  can  be  shewn  that  when  a  becomes 
equal  to  [h  -(r-l)(K  +  r'K')]/r,  the  limit  of  the  expression 

U=Hr_1  [e-^(r-vK'wx  (W+ra,  W;  P,  er_0  +  e^^K'wX  (W-ra,  a;  P,  er_0], 

if  it  is  not  a  quadratic  polynomial  in  functions  @(TT;  APa),  is  zero.  The 
consequence  of  this  will  be  that  ^r  [  W  ;  K,  K'  +  //,]  is  expressible  as  a 
polynomial  involving  only  the  functions  ®  (TF;  APa). 

For  the  fundamental  formula  of  §  309,  p.  510,  immediately  gives*,  for 
any  values  of  a,  b, 

x(W+a,  W  +  b;  P,  e)x(a  +  b,  0;  P,  e)  =  x(a,  b;  P,  €)x(W  +  a  +  b,  W;  P,  e), 
and  hence,  replacing  e,._j  simply  by  e,  the  expression  U  is  equal  to 
2eae-*"V9.  {e-'-o-D  K>W®  (W  +  a;  A  +PJ@[W  +  (r-l)a;  A  +  P  +  PJ 


where   P,  =i>   is   used   for  Pa+  ......  +  P       and  e1;  e2,...    for 


(er-i)ai  ••••  Replacing  ra  in  this  expression  by  the  period  h-(r-l)(K+r'K'), 
and  omitting  an  exponential  factor  depending  only  on  r,  h,  K,  K'  and  P,  it 
becomes 

@[W-a;  A  +  P  +  Pa] 


*  We  take  the  case  when  the  characteristics  B,  A  of  %  309  are  equal.  It  is  immediately 
obvious  from  the  equation  here  given  that  in  the  expressions  here  denoted  by  Hm  the  value  of  the 
half-integer  characteristic  A  is  immaterial. 


614  FORMULATION    OF   THE   GENERAL  THEOREM  [368 


A  being  as  before  taken  =  (  ^J  and  £  =  «.tf^»>  W«^fr-*>*'«»  ;  and  this 
is  immediately  shewn  to  be  the  same  as 

*\  A+Pa)S(W-a;  A  +  P  +  Ptt), 

where  ep  is  the  fourth  root  of  unity  associated  with  the  characteristic  P  of 
the  Gb'pel  group  (P),  which  is  to  be  taken  equal  to  1  in  case  P  =  0.     Thus 

/A\ 
the  expression  vanishes  when  fp  =  —  e*ni  '  p  '  (  „  J  .     Hence,  in  order  to  prove 

that   when  the  expression   U  is   not  a  quadratic  polynomial  in  functions 
©  (W  ;  APa),  it  is  zero,  it  is  sufficient  to  prove  that  the  only  case  in  which 

fA\ 

U  is  not  such  a  quadratic  polynomial  is  when  £P  =  —  e?ni  '  p  '  (  p  )  • 
Now  the  denominator  of  Hr^  is 

2e0e-^9'3«  0  [ra  ;  A  +  P  +  PJ  @  [0  ;  A  +  Pa], 

a 

where  P  still  denotes  Pai  +  .  .  .  +  Pa      and  ea  has  the  set  of  values  of  er_2  ; 
save  for  a  non-vanishing  exponential  factor  this  is  equal  to 


or 


according  as  P  =  0  or  not,  where,  in  the  second  form,  P^  is  to  describe  a 
group  of  %P~I  characteristics  such  that  the  combination  of  this  group  with 
the  group  (0,  P)  gives  the  Gb'pel  group  (P).  We  shall  assume  that,  when 

fA\ 
£P  is  not  equal  to  —  e*wi  '  p  '  (  p  j  ,  neither  of  these  expressions  vanishes  for 

general  values  of  the  periods  r. 

Since  the  function  *¥r  (  W  ;  K,  K'  +  /jJ)  is  certainly  finite,  we  do  not 
examine  the  finiteness  of  the  coefficients  Hm  when  m  is  less  than  r  —  1, 
these  coefficients  being  independent  of  W  ;  further,  in  a  Gopel  system  (AP), 
any  one  of  the  characteristics  APa  may  be  taken  as  the  characteristic  A  ; 
the  change  being  only  equivalent  to  adding  the  characteristic  P0  to  each 
characteristic  of  the  group  (P);  hence  (§  327,  Chap.  XVIII.),  our  investigation 

gives  the  following  result  :  —  Let  any  2?  functions  ^f(u',  2o>,  2o>',  2??,  277' 

whose  (half-integer)  characteristics  form  a  Gopel  system,  syzygetic  in  threes,  be 
transformed  by  any  transformation  of  odd  order;  let  (AP)  be  the  Gopel 


system  formed  by  the  transformed  characteristics  [       j  J  then  every  one  of  the 


369]  FOR  TRANSFORMATION    OF   ODD   ORDER.  615 

original  functions  is  an  integral  polynomial  of  order  r  in  the  %>  functions* 
*b(w  ;  2u,  2i/,  2£  2f  |  AP)  :  as  follows  from  §  288,  Chap.  XV.,  the  number  of 
terms  in  the  polynomial  is  at  most,  and  in  general,  \  (/*  +  1). 

For  the  cases  p  =  l,2,  3,  and  for  any  hyperelliptic  case,  it  is  not  necessary 
to  use  the  addition  formula  developed  in  Chap.  XVIII.  We  may  use  instead 
the  addition  formula  of  §  286,  Chap.  XV.  It  is  however  then  further  to  be 
shewn  that  only  2?  theta  functions  enter  in  the  final  formula.  For  the  case 
p=3  the  reader  may  consult  Weber,  Ann.  d.  Mat.  2a  Ser.,  t.  IX.  (1878), 
p.  126. 

369.     We  give  an  example  of  the  application  of  the  method  here  followed. 

Suppose  p  =  l,  r  =  3,  and  that  the  transformation  is  that  associated  with  the  matrix 


;  then  (§  324,  Chap.  XVIII.)  taking  l/=3,  the  function 
9[u;  2»,  2o>',  2,,,  2,/  |  !(_?)], 
or  SOI(M),  is  equal  to  501(3zc;  2v,  6v',  2f/3,  2f)  or  ^r)<1>"1">3(  W;  -£,  0).     Now  we  have, 


also  e^j  (  W+  a)  is  equal  to 


a  a, 

a,  0;  0,  e)  a  e/x(3«,  0;  ^  a,  e  )  ^    » 

if  we  take  the  Gopel  system  to  be  \  (       j  ,  £  L  J  ,  so  that  *V"i(i)j  tnis  is  e(lual  to 

e^(a)+fle;o(q)  e01  (2a)  e01  (a)  +«1'e10  (2a)  e10  (a) 

J,e01(2a)e01+fle10(2a)e10   '       >  t,      e01(3a)e01+fl'e10(3«)e10 

6l(>  (2a)  9()1  (a)  "  *'  1/e<)1  (2a)  QI°  (a)  ' 


,!„         oi— 

"I:e01(2a)e01+«1e10(2a)e10€l  e,      e10(3a)e01-iVe01(3a)e,0 

where  001  denotes  001  (0),  etc.,  and 


iV1'801(  ir+3a.)010(  IV). 
Now,  in  accordance  with  the  general  rules,  the  denominator  of  the  fraction 
610  (2a)  001  (a)  -  if/e01  (2a)  010  (a) 

e10  (3a)  e01  -  ifl'  e01  (3a)  e10 


vanishes  when  ./=  -^          e-^-2A')?l'+«2^s  namelyj  as  =i     _      =  ^,  when 

,,'=  _le«^+1),  and  a  =  (A  +  l)/3  ;  in  fact,  putting  o  = 


e10  (3a)  e01  -  W/GO!  (3a)  e10=  e'r£(t+1)  e10  (.r)  e01  -  iV 


*  The  expression  of  the  transformed  theta  function  in  terms  of  2?  =  4  theta  functions  is  given 
by  Hermite,  Compt.  Eendu*,  t.  XL.  (1855),  for  the  case  p  =  2.  For  the  general  hyperelliptic  case 
cf.  Konigsberger,  Crelle,  LXIV.  (1865),  p.  32. 


616  EXAMPLE   OF   THE   GENERAL   METHOD    FOR   ODD    ORDER.  [869 

for  small  values  of  .r,  when  iel'  =  e1rl^  +  ',  because  the  differential  coefficients  of  the  even 
functions,  being  odd  functions,  vanish  for  zero  argument  ;  thus  the  denominator  of  the 
fraction  vanishes  to  the  second  order.  We  find  similarly,  for  ie1'  = 
that  the  numerator  of  this  fraction  is  equal  to 


in  the  same  case  also  we  find  that  the  expression  El  is  equal  to 

e«  <*+1>  [e'10  (  W)  e01  (  W)  -  e'01  (  W)  e10 

while  the  expression  010  (  W-  3a)  001  (  W)  —  ?'e/e01  (  W-  3a)  010  (  W)  is  equal  to  the  negative 
of  this.     Thus  the  function  ©^  (  W+a)  can  be  expressed  by  the  functions  010  (  TF),  001  (  W), 
and  their  differential  coefficients  of  the  first  order  ;  but  the  function  ©^  (  W+a)  +  0^  (  W—  a) 
can  be  expressed  by  the  functions  010  (  W),  Qol  (  W)  only. 
In  the  function  0^  (  W  +a)  +  0^  (  W-  a)  the  part 

s  010  (2a)  001  (a)  -  ^/001  (2cQ  010  (a)  £ 
e/       010  (3a)  ©01  -  tV  ©01  (3a)  010 

furnishes  only  the  single  term  for  which  ie{=  -em  (7t+1),  namely, 

h-±l\ 

T  •* 

GOI  (  W)  010  (  TF). 


e     -e 

*%  \      o      I  *T 

\    *   / 


U01  U10 

Ex.  i.     Prove  that  the  final  result  is  that  ?C0301  (u)  is  equal  to 


-  [ej,  (i)  e^  -  ©^  (i)  ©J0]  »a  (w) 
(j)  [©10  (j)  ©01  +  ©01  (j)  010]  n          2  3 


where  ©01,  ©10  denote  ©01  (0)  and  ©10  (0)  respectively. 
Ex.  ii.     Prove  that 


©in  (i)  ©n 

=2-— 


370.  General  formulae  for  the  quadric  transformation  are  also  obtainable. 
The  results  are  different,  as  has  been  seen,  according  as  the  characteristic 
(K,  K')  of  the  transformed  function  is  zero  (including  integral)  or  not.  The 
results  are  as  follows  :  — 

When  (K,  K')  is  zero,  the  transformed  function  can  be  expressed  as  a 
linear  aggregate  of  the  2^  functions  S-2  (w  A,  Pi),  whose  characteristics  are 
those  of  any  Gb'pel  system, 


370]  GENERAL  THEOREM  FOR  TRANSFORMATION  OF  THE  SECOND  ORDER.  617 

When  (K,  K')  is  not  zero,  the  transformed  function  can  be  expressed  as  a 
linear  aggregate  of  the  2*"1  products  ^  (w  \  A,  PI)  ^  (w  \  A,  K,  Pi),  in  which 
the  characteristics  Pi  are  those  of  any  Gopel  group  whereof  the  charac 
teristic  K,  =  (K,  K'),  is  one  constituent,  and  A  is  a  characteristic  such  that 
|  A,  K  |  =  |  K  |,  or  |  A,  K  \  =  \  K  \  +  1  (mod.  2),  according  as  the  function  to  be 
expressed  is  even  or  odd*. 

When  (K,  K')  is  zero,  the  equation  (I),  §  367,  putting  K  =  K'  =  /*  =  0, 
and  then  increasing  W  by  ^/u-r',  where  /A  is  a  row  of  quantities  each  either 
0  or  1,  gives 


2r' 


o  ) 


0 


hence,   from   the  fundamental   formula  of  §  309  (p.   510),  writing  therein 
v  =  0,u=W  +  a,b  =  a  =  h/2,  A  =$  (§  ,  Pt  =  $  (qi'}  ,  and 

\  W  \(±i/ 

we  obtain 

;  2r' 


i  _  i  _  Vf  .(S)2  /  W  .    T'  I  yj  PA 

2£©2  (0  ;  T  |  APt)  7?t     (     '      '       l)' 

i 

where  (7  is  independent  of  p.     It  is  assumed  that  the  sum  2£®2(0;  T'  4P;) 

i 

is  different  from  zero  for  each  of  the  2?  sets  of  values  of  the  fourth  roots  &. 
This  formula  suffices  to  express  any  theta  function  of  the  second  order  with 
zero  characteristic. 

When  (K,  K'}  is  other  than  zero,  by  putting  in  the  equation  (I),  §  367, 
r  =  2,  /i=0,  adding  %rh'  to  F,  where  h'  is  a  row  of  quantities  each  either 
0  or  1,  and  then  changing  the  sign  of  W,  we  obtain 

Ce-**(K+M  V2(W;  K,K'  +  h')  =  2  [e9^'^®'  (W  +  a)  +  ee-^'^&  (  W  -  a)], 

h 

where  X  =  K  +  h,  X'  =  K'  +  h',  and  C  is  the  same  constant  as  before,  indepen 
dent  of  W,  K,  K',  h',  and  a  =  ±\  +  £T'\',  the  period  T'  being  omitted  on  the 
right  side.  Hence,  taking  the  fundamental  formula  of  §  309  (p.  510),  putting 
therein  t>=0,  u=W+a,  b  =  a,  A=(),B=A,  and  then  writing  a-JX+|TV+4«, 
where  #  is  a  row  of  p  equal  quantities,  we  find,  provided  |  K,  Pf  |  =  0,  (mod.  2), 

When  (K,  K')  is  zero,  the  function  is  necessarily  even  (§  288,  p.  463),  and  therefore  |-fiT|=|Q| 
We  have  seen  (§  327,  Chap.  XVIII.)  that  this  is  always  true  when  r  is  odd.    When  r  is  2,  it  is  not 
always  so,  as  is  obvious  by  considering  the  transformation,  for  p  =  l,  in  which  a  =  2,  /3  =  0,  a'  =  0 
/3'  =  1,  and  ((?,<?')  =  (i,i);  then  we  find  (A',  K')  =  (J,  1)  ;  thus  |Q|  =  1,  \K\  =  2. 


G18      GENERAL  FORM  FOR  TRANSFORMATION  OF  SECOND  ORDER.     [370 

and  €==en\K\  +  ni\A,K\t  that  2*W2  (W ;   K,  K'  +  li)  is   equal  to  the  limit, 
when  a;  vanishes,  of  the  expression 

a;\A,K,  Pi) 

+  ®(W-x\A,K,Pi)}, 


U            y          (P*\     r 

where  c;  i  =  {  A  }  e 

\  ^i_  / 

i  (JlQ  -~~  Itf  Q-i  c  .     o  Y)  t  i 

•  1             Jl'    Cj.     (  1  1  M  1 

x-*"1-  / 

'  !  i  /''A     P  ^ 

2gi« 

1   —              2 

(0;  A,  Pi) 

i 

It  can  easily  be  proved  (cf.  §  308,  p.  510)  that  the  denominator  of  Ef 
vanishes,  for  x  =  0,  for  the  2^  sets  of  values  of  the  fourth  roots  &  in  which 
the  fourth  root  corresponding  to  the  characteristic  K  of  the  group  (P)  has 

(A\ 
)  ei*l*l,  and  that  the  corresponding  expressions 

L,  K,  Pi)  +  S(W-x\A,  K,Pt)} 


have  the  limit  zero  ;  the  summation  2  is  therefore  to  be  taken  only  to  extend 

i 

A. 


(.\ 
Kje^ilKl.     It  may 

however  happen  that  the  denominator  of  Ef  vanishes  for  other  sets  of  values 
of  the  fourth  roots  &,  when  a?=  0.  We  assume  that  for  such  sets  of  values 
the  sum  multiplying  Ef  in  the  expression  Uf  does  not  vanish  for  x  =  0  ;  by 
recurring  to  the  proof  of  the  formula  of  §  308,  it  is  immediately  seen  that 
this  is  equivalent  to  assuming  that  the  expression 

;  Pi) 


is  not  zero  for  general  values  of  the  arguments  U  for  any  set  of  values  of  the 
fourth  roots  e*  (cf.  (/S),  p.  514).  That  being  so,  the  value  of  Ef  when  its 
denominator  vanishes  for  a?  =  0,  can  always  be  obtained  from  the  limiting 
expression  given,  by  expanding  its  numerator  and  denominator  in  powers 
of  x. 

Ex.     Applying  the  formula  of  this  page  for  the  case  p  =  1  to  the  function 

eu(2TF;  2rO  =  i*a(TP;   -£,  1), 

for  which  (A',  £"')  =  (-£,  0)  and  A'  =  l,  we  immediately  find  that  the  Gopel  system  iu  terms 
of  which  the  function  can  be  expressed  is  (A,  APJ,  where  A  =£  (  Qj  ,  Pl  =  K=$  (  _v)  «  we 

/A\ 
are  to  exclude  the  value  of  the  expression  Uf  in  which  {  1  =  -  f_J  =  1  ;  the  value  of  Ef  for 

^=  —  1  is  easily  found  to  be 


872]         THE  PROBLEM  OF  THE  CONSTANT  COEFFICIENTS.          619 


of  which   both  numerator  and  denominator  vanish  for  #  =  0.     The  final  result  of  the 
formula  is 

Cen(2Tf;  2r')=-4eio(i;  ^e^i;  r')eu(JT;  r'}Qw(W-  r')/e'n  (0;  r')ej(J(0  ;  r'). 
Prove  this  result,  and  also 

<7eol(2Tf;  2r')  =  2e^(i;  r>)eM(W;  r')eoi(Tf;  0/6^(0;  r')  901  (0  ;  r'), 
and  (cf.  §  365)  obtain  the  formulae 


or 
A 


or       w 


K 


e,(i;  r'Hie^O;  r')e01(o;  r')[e^(0;  r')+e^(o;  r')], 
ej,(0j  20  =  4  [ej,(0;  0  +  6^(0:0], 

(7=  V2[eJ,(0;  0  +  8^(0;  r')]. 

371.  The  preceding  investigations  of  this  chapter  enable  us  to  specify  in 

all  cases  the  form  of  the  function  §(u:  2o>,  2&>'  2??,  2??'    ^  ) 

V  QJ 

when  expressed  in  terms  of  functions  ^  (w  ;  2i/,  2i/.  2(T, 

\ 

In  many  particular  cases  it  is  convenient  to  start  from  this  form  and 
determine  the  coefficients  in  the  expression  by  particular  methods.  But  it 
is  proper  to  give  a  general  method.  For  this  purpose  we  should  consider 

two  stages,  (i)  the  determination  of  the  coefficients  in  the  expression  of  the 

/    |  Q'\ 
function  ^  (u     L  J  by  means  of  functions  tyr  (w  ;  K,  K'  +  /&),  (ii)  the  determi- 

\  c    / 

nation  of  the  coefficients  in  the  expression  of  the  functions  i/rr  (w  ;  K,  K'  +  //,) 

(«*'\ 
w         \.     The  preceding  formulae  of  this  chapter 

enable  us  to  give  a  complete  determination  of  the  latter  coefficients  in  a 
particular  form,  namely,  in  terms  of  theta  functions  whose  arguments  are 
fractional  parts  of  the  periods  2v,  2v  ;  but  this  is  by  no  means  to  be  regarded 
as  the  final  form. 

372.  Dealing  first  with  the  coefficients  in  the  expression  of  the  function 
*\      Q)  b^  functions  $r(w,  K,K'  +  (JL),  there  is  one  case  in  which  no 
difficulty  arises,  namely,  when  the  transformation  is  that  associated  with  the 


matrix  ^  J  ;  then  S-  (u  I  Q  )  is  equal  to  S  (rw  ;  2v,  2rv',  2f/r,  2^'    K'^'\  , 
the  row  K'  being  in  fact  equal  to  rQ',  namely  *  (u   Q}  is  ^,.  (w  ;  K,  K'). 


620  THE   FIRST   STEP   IN   THE  [372 

Now  it  can  be  shewn*,  that  if  ftr  be  the  matrix  associated  with  any 
transformation  of  order  r,  and  r  be  a  prime  number,  or  a  number  without 
square  factors,  then  linear  transformations,  ft,  ft',  can  be  determined  such 

(T  0\ 
that  ft,.  =  ft  f        j  ft  .    Hence,  in  cases  in  which  the  matrices  ft,  ft'  have  been 

calculated,  it  is  sufficient,  first  to  carry  out  the  transformation  ft  upon  the 
given  function  Sfcfti  j;  then  to  use  the  formulae  for  the  transformation 

(r  0\ 
j  ,  whereby  the  original  function  appears  as  an  integral  polynomial  of 

order  r  in  2^  theta  functions  ;  and  finally  to  apply  the  transformation  ft'  to 
these  2f  theta  functions.  All  cases  in  which  the  order  of  transformation  is 
not  a  prime  number  may  be  reduced  to  successive  transformations  of  prime 
order  (§  332,  Chap.  XVITL). 

We  can  however  make  a  statement  of  greater  practical  use,  as  follows.    It 
is  shewn  in  the  Appendix  II.  (§§  415,  416)  that  the  matrix  associated  with 

any  transformation  of  order  r  can  be  put  into  the  form  ft  (        „,  j  ,  where  ft 

is  the  matrix  of  a  linear  transformation,  and  that,  in  whichever  of  the  possible 
ways  this  is  done,  the  determinant  of  the  matrix  B'  is  the  same  for  all.  In 
all  cases  in  which  this  has  been  done  the  required  coefficients  are  given  by 
the  equation 


•  ,, 

V|ft)|  | 

W+^'.Se-->->.  &  r      .  2v_  w>  2?/).  2?,  <A"+M)/r1  1 

H  K 


^  \M\\v\\R 

wherein,  (Q,  Q')  being  a  half-integer  characteristic,  e  is  an  eighth  root  of  unity, 
u  =  Mw,  \M\  is  the  determinant  of  the  matrix  M,  etc.,  /m  is  in  turn  every 
row  of  integers  each  positive  (or  zero)  and  less  than  r,  which  satisfies  the 

condition  that  the  p  quantities  -  B'/j,  are  integral,  and,  finally,  7  denotes  the 

symmetrical  matrix  BB',  while  d  denotes  the  row  of  integers  formed  by  the 
diagonal  elements  of  7.  It  is  shewn  in  the  Appendix  II.,  that  the  resulting 
range  of  values  for  p  is  independent  of  how  the  original  matrix  is  resolved 
into  the  form  in  question.  For  any  specified  form  of  the  linear  transformation 
ft  the  value  of  e  can  be  calculated  (as  in  Chap.  XVIII.,  §§  333—4);  if  e0 

*  Cf.  Appendix  II.;  and  for  details  in  regard  to  the  case^  =  3,  Weber,  Ann.  d.  Mat.,  Ser.  2a, 
t.  ix.  (1878—9).  We  have  shewn  (Chap.  XVIII.,  §  324,  Ex.  i.)  that  the  determinant  of  the 
matrix  of  transformation  is  ±?-P.  From  the  result  quoted  here  it  follows  that  that  determinant 
is  +7*. 


372]  DETERMINATION   OF   THE   COEFFICIENTS.  621 

denote  its  value  when  the  characteristic  (Q,  Q')  is  zero,  its  value  for  any  other 
characteristic  is  given  by 


where  H  =  ,  and  Q,'  =  pQ'  -  p'Q-^d(pp'),   -  Q,  =5=  Q'  -  <f'Q  -%d(<r<r'). 

To  prove  this  formula,  we  have  first  (§  335,  Chap.  XVIII.),  if  fl  = 


P 

the  equation 


=  *(u;  2(o,  2ft)', 


Q' 




\f\J\f, 


where   u  =  M1ul,  Mlwl  =  cap  +  w'p,  etc.     Writing  ul  =  2o)1U'l,  WI/  =  O)ITI,  we 
have 

j  (u^  5  2o)i   2(&i ,  2f]i,  2i)i 


and  the  equations  w.j  =  J/2w,  Jl/2i;  =  w^A,  M^v  =  ^B  +  w^B',  give,  if  w  =  2vW, 
v  =  vr\  and  in  virtue  of  AB'  —  r,  the  equations  Ul  =  A  W,  rr^  =  AT'  A  —  BA, 
while,  by  the  equation  r£=  M^A,  we  find  r}l(o1~1u12  =  r%u~lw*.  Now  it  is 

(o 
Ul  ;  X 

gives 

(  m  +  -  } 

\         r/ 

ym»  +  dm)  - 


r 


wherein  7  =  55',  and  cZ  denotes  the  row  of  diagonal  elements  of  7,  and  m,  p, 
are  obtained  by  putting  An—-  rm  +  p,  m  being  a  row  of  integers,  and  /*  a  row 
of  integers  each  less  than  r  and  positive  (including  zero)  ;  this  equation  is 

equivalent  to  n  —  B'm  =  -B'ij,;  corresponding  to  every  n  it  determines  an 
unique  m  and  an  unique  p  for  which  —  -  is  integral  ;  corresponding  to  any 

TV 

assigned  p,  for  which  -  is  integral,  and  an  assigned  m,  the  equation 
determines  an  unique  n.  Since  then  yw2  +  dm  is  an  even  integer,  and,  for 
the  terms  which  occur,  B  —  m  is  an  integer,  we  have 


Increasing,  in  this  equation,  U,  by  Ql  +  TjQ/,  we  hence  deduce 


;  T, 


e 


r 

[r!T; 


622  A    PARTICULAR   EXAMPLE   OF   THE   SECOND   STEP  [372 


where  K'  =  AQ,',  -  K  =  BQ1' -  B'Q1-^d(BB')i  so  that  (K,  K')  is  the 
characteristic  of  the  final  theta  function  of  w.  Since  now  the  matrix 
MvB'  =  M.M^B'  =  M^AB'  =  rMlwl ,  and  therefore  \M\  v\  B'\  =  rP\Ml  mi\, 

we  have,  by  multiplying  the  last  obtained  equation  by  e^i<ai  u>*  =  e%r&~lw2 ,  the 
formula  which  was  given  above. 

Ex.  i.     When  p  =  l,  the  transformation  associated  with  the  matrix  (        )  gives  rise  to 

\  J 

the  function  9(TF ;  \T}  ;  we  have 


©/  TI7  .      1  _'\ o  /Q  H7  •     Q—  '\    l_  £i   I    O  T'lT  .     O    ' 
^  rr    j    >rT  ^  —  O  ^O  rr    ^    Or  y  ~J~  v7  I   «5  rr    j    OT 

V 
Other  simple  examples  have  already  occurred  for  the  quadric  transformations  (§  365). 

Ex.  ii.     Prove  when  p  =  2,  by  considering  the  transformation  of  order  r  (r  odd)  for 
which 


,0,    */•        vo,  oy        vo  o. 

that 
6    it,— u.u<>.  ru9\  -  (T,,  —  2ur19  +  u2r.,.>  —  2X),  2r,9  — 2uT9,,  rrool 

'          ^«'  j^^,\H  I         li  I  HI  /7  \.£t  |~     ^^  7  i«J 

',  0)+S  2 


where  ^(OTI,  74)  denotes  B^J  rr 


+  e 


y .      (Wiltheiss, 


Crelle,  xcvi.  (1884),  pp.  21,  22.) 

373.     In  regard  now  to  the  question  of  the  coefficients  which  enter  in  the 

/      Kf" 
expression  of  the  functions  i/>y  (w  ;  K,  K'  +  /i)  by  means  of  functions  S-  (  w     r  )  , 

\        K  ) 

the  problem  that  arises  is  that  of  the  determination  of  these  coefficients  in 
terms  of  given  constants,  as  for  instance  the  zero  values  of  the  original  theta 
functions.  The  theory  of  this  determination  must  be  omitted  from  the 
present  volume.  In  the  case  when  the  order  of  the  transformation  is  odd 
these  coefficients  arise  in  this  chapter  expressed  in  terms  of  theta  functions, 

»M~  5    2t>,  2i/,  2£,  2^'J  ,  whose  arguments  are  ?'-th  parts  of  the 

periods  2i»,  2i/.  By  means  of  two  supplementary  transformations,  A,  7'A"1, 
(as  indicated  §  332,  Chap.  XVIII.),  or  by  means  of  the  formulae  of  Chap.  XVII. 
(as  indicated  in  Ex.  vii.,  §  317,  Chap.  XVII.),  we  can  obtain  equations  for 
functions  ^  (rw  ;  2u,  2i/,  2f,  2£")  as  integral  polynomials  of  degree  r2  in 
functions  S-(w;  2v,  2t/,  2£  2£").  By  means  of  these  equations  the  functions 

^•(—  -;    2u,   2i/,    2£,   2£'j    are   determined   in    terms   of  functions 

^  (0  ;  2u,  2i/,  2f,  2^')  ;  or  this  determination  may  arise  by  elimination  from 
the  original  equations  of  transformation,  without  use  of  the  multiplication 
equations.  There  remains  then  further  the  theory  of  the  relations  connecting 
the  functions  &(0;  2u,  2i/,  2£  2f)  and  the  functions  ^(0;  2eo,  2ft)',  277,  2?/), 
which  is  itself  a  matter  of  complexity. 


373]  IN   THE    EXPRESSION    OF   THE   CONSTANT   COEFFICIENTS.  623 

For  the  case/>=l,  the  reader  may  consult,  for  instance,  Weber,  Elliptische  Functionen 
(Braunschweig,  1891),  Krause,  Theorie  der  doppeltperiodischen  Functionen  (Erster  Band, 
Leipzig,  1895).  For  the  case  jo  =  2,  Krause,  Hyperelliptische  Functionen  (Leipzig,  1886), 
Konigsberger,  Crelle,  LXIV.,  LXV.,  LXVII.  For  the  form  of  the  general  results,  the  chapter, 
Die  Theilung,  of  Clebsch  u.  Gordan,  AbeUsche  Functionen  (Leipzig,  1866),  which  deals  with 
the  theta  functions  arising  on  a  Riemaun  surface,  may  be  consulted.  For  the  hyper- 
elliptic  case,  see  also  Jordan,  Traite"  des  Substitutions  (Paris,  1870),  p.  365,  and  Burkhardt, 
Math.  Annal.  xxxv.,  xxxvi.,  xxxvm.  (1890  —  1). 

In  particular  cases,  knowing  the  form  of  the  expression  of  the  functions 

3  (u  ;  2o>,  2«',  2r],  2rj') 

in  terms  of  functions  3  (w  ;  2v,  2i/,  2£,  2f),  we  are  able  to  determine  the  coefficients  by  the 
substitution  of  half-periods  coupled  with  expansion  of  the  functions  in  powers  of  the 
arguments.  See,  for  instance,  the  book  of  Krause  (Hyperelliptische  Functionen}  and 
Konigsberger,  as  above. 

Ex.  i.  In  case  p  =  2,  r  =  3,  the  function  05(3JF,  3r')  is  a  cubic  polynomial  of  the 
functions  06  (  W,  T'),  634  (  W,  T'),  0t  (  Wt  T'),  e02  (  W,  r'),  of  which  the  characteristics  are 

respectively  £L'  QJ,  $('  _   V  J/_      _\  $(      '  QJ  ;  these  form  a  Gopel  system. 

The  only  products  of  these  functions  which  are  theta  functions  of  the  third  order  and  of 
zero  characteristic  are  those  contained  in  the  equation 

©5  (3  W,  3r')  =  Atl  +  B<t>5$l4  +  CWl+D<t>^l2  +  E<p3t4>1^ 

where  $6  =  05(JF,  T'),  etc.;  this  equation  contains  the  right  number  £  (rp  +  1  )  =  5  of  terms 
on  the  right  side.  Putting  instead  of  the  arguments  W1,  TF2  respectively 


we  obtain  in  turn 

eM(3lF,  3r')=     A^ 
0,  (Sir,  3/)=  -A<fi 

eM(3Tr,  30=  -^L 

whereby  the  Gopel  system  of  functions  06  (3  W,  3r),  ©34  (3  W,  3r'),  6X  (3  W,  3r'),  e02  (3  IF,  3r') 
is  expressed  by  means  of  the  Gopel  system  <£5,  ^34,  <£j,  ^02. 

From  the  first  two  equations,  by  putting  the  arguments  zero,  we  obtain 

®/;efi-Q<ue<u 

t  _      65  3434         n  _ 

•**  ~~  4  4  9          — 

e5~634  95e34  (66  ~  934 

where  05  =  05(0  ;  3r'),  etc.,  and  0.  =  05(0  ;   T'),  etc.  ;  by  the  addition  of  other  even  half- 
periods  to  the  arguments,  for  instance,  those  associated  with  the  characteristics 


O,O'     -i, 

we  can  obtain  expressions  for  C,  D,  E  ;  these  substitutions  give  respectively 
0,3  (3  IK  ;  3r')  =  ^<# 
04  (311';  3r')  =  A<f 
0,,  (3  IF  ;  3r')  =  .1  0J., 


624  PARTICULAR   EXAMPLE.  [373 

putting  herein  W=0  we  obtain  in  succession  the  values  of  Z>,  C  and  E,  expressed  in  terms 
of  the  constants  previously  used,  05,  034,  65,  634  and  the  constants  023,  ©4,  012,  G^,  003, 
04J  eM,  012,  00,  62,  001.  Thus  the  zero  values  of  each  of  the  ten  even  functions  0(  W  \  r) 
enter  in  the  expression  of  the  coefficients  J,  B,  C,  D,  E  ;  there  remains  then  the  question 
of  the  expression  of  the  zero  values  of  the  ten  even  functions  in  terms  of  four  independent 
quantities  (cf.  Ex.  iv.,  §  317,  Chap.  XVII.),  and  the  question  of  the  relations  connecting 
the  constants  05,  ©34,  etc.,  and  the  constants  05,  034,  etc.  (cf.  the  following  example). 

Ex.  ii.     Denoting  001  (0  ;  3r')  001  (0  ;  r')  by  <701,  etc.,  shew  that  when  p  =  2  the  result  of 
Ex.  iii.,  §  292  (p.  477)  gives  the  equations 

^01  +  ^2  =  £5  +  ^34  ~  ^12  ~  ^0  J 
^4  +  ^03  =  ^5  ~  ^34  +  ^12  ~~  ^0> 
^23  +  ^14  =  ^5  ~  ^34  ~  ^12  +  ^OJ 

these  being  the  only  equations  derivable  from  that  result.  By  these  equations,  in  virtue  of 
the  relations  connecting  the  ten  constants  0  (0  ;  r'),  and  the  relations  connecting  the  ten 
constants  0  (0  ;  3r'),  (for  the  various  even  characteristics),  the  three  ratios 

634(0;  3r')/05  (0,  3r'),    012(0;  3r')/e5(0;  3r'),    00  (0  ;  3r')/66  (0  ;  3r') 
are  determinate  in  terms  of  the  three 

034  (0  ;  r')/e5  (0  ;  T'),    012  (0,  r')/05  (0  ;  r'),    00  (0  ;  r')/66  (0  ;  r'). 
By  addition  of  these  equations  we  obtain 

^01  +  ^2  +  ^4  +  ^03  +  ^23  +  ^14  +  ^34  +  ^12  +  ^0  =  ^  Cfi  • 

Obtain  similarly  from  the  result  of  Ex.  iii.,  §  292,  for  any  value  of  p,  the  equation 
20^0;  3r'    i(j')]e[°;  '    i(j')]  =  (2p-l)e(0;  3r')  6  (0  ;  r'), 

where  the  summation  on  the  left  extends  to  all  even  characteristics  except  the  zero 
characteristic  ;  for  instance,  when  p  —  I,  this  is  the  equation 

001  (0  ;  3r')  001  (0  ;  r'}  +  610  (0  ;  3r')  610  (0  ;  T')  =  Qw  (0  ;  3r')  0^  (0  ;  r'), 

namely  (cf.  Ex.  i.,  §  365  of  this  chapter)  it  is  the  modular  equation  for  transformation  of 
the  third  order  which  is  generally  written  in  the  form  (Cayley,  Elliptic  Functions,  1876, 
p.  188), 


As  here  in  the  case  j»  =  2,  so  for  any  value  of  p,  we  obtain,  from  the  result  of  Ex.  iii., 
§  292,  2P—  1  modular  equations  for  the  cubic  transformation. 

Ex.  iii.     From  the  formula  of  §  364  we  obtain  modular  equations  for  the  quadric 
transformation,  in  the  form 


where  s  is  a  row  of  p  quantities  each  either  0  or  1,  so  that  the  right  side  contains  2"  terms, 
and  k,  k',  s'  are  any  rows  of  p  quantities  each  either  0  or  1. 

374.  In  the  fundamental  equations  of  transformation  we  have  considered 
only  the  case  when  the  matrices  a,  a',  /3,  /3'  are  matrices  of  integers  ;  the 
analytical  theory  can  be  formulated  in  a  more  general  way,  as  follows;  the 
argument  is  an  application  of  the  results  of  Chap.  XIX. 


374]        GENERALISED    FORM   OF   THE   EQUATIONS   OF  TRANSFORMATION.         625 

Suppose  we  have  the  relations  expressed  (of.  Ex.  ii.,  §  324,  Chap.  XVIII.) 

by 

(  M,       0     )  (  2v,    2i/  )  =  (  2&),    2o>'  )  (  a  ,   /3   ), 
0  ,   rJf-1       I  2£    2£'  277,    277'        ,  a.',   0' 

where  r  is  a  positive  rational  number,  M  is  any  matrix  of  p  rows  and  columns, 
whose  determinant  does  not  vanish,  a,  /3,  a',  /3'  are  matrices  of  p  rows  and 
columns  whose  elements  are  rational  numbers  not  necessarily  integers,  &>,  w  '  , 
V),  ?;'  are  matrices  of  p  rows  and  columns  satisfying  the  equations  (B),  §  140 
(Chap.  VII.),  and  v,  v',  f,  £"  are  similar  matrices  satisfying  similar  conditions  ; 
then,  as  necessarily  follows,  the  matrices  a,  @,  a',  $'  satisfy  the  relation 
(viii)  of  §  324  (Chap.  XVIII.). 

If  now  x,  y  be  any  matrices  of  p  rows  and  columns,  the  relations  supposed 
are  immediately  seen  to  be  equivalent  to 

(M,       0 
0  ,   rM~ 


we  suppose  that  x,  y  are  such  matrices  of  integers  that  ax,  fty,  ax,  ft'y  are 
matrices  of  integers,  and,  at  the  same  time,  such  that  rx  is  a  matrix  of  integers  ; 
such  matrices  x,  y  can  be  determined  in  an  infinite  number  of  ways. 

Let  u,  w  be  two  rows  of  p  arguments  connected  by  the  equations  u  =  Mw  ; 
when  the  arguments  w  are  simultaneously  increased  by  the  elements  of  the 
row  of  quantities  denoted  by  2vxm  +  2v'ymf,  in  which  m,  m'  are  rows  of  p 
integers,  the  arguments  u  are  increased  by  the  elements  of  the  row  2&>r?  +  2<»W, 
where  n  =  axm  +  &ym,  n  =  a'xm  +  ft'ym'  are  rows  of  integers.  The  resulting 
factor  of  the  function  *&(u;  2&>,  2o>',  2?7,  277')  is  eR,  where,  if  Ha  =  2r)a+  ZrfoL, 
etc.,  (cf.  (v),  §  324,  Chap.  XVIII.),  R  is  given  by 

R  =  Hn  (u  +  ^  Hn)  —  irinri 

=  (Haxm  +  Hpym')  (Mw  +  Mvxm  +  Mv'ym'}  —  -rrinn 
=  (MHaxm  +  MHpym'}  (w  +  vxm  +  vym)  —  Trinri 
=  r  (%%xm  +  2^'ym')  (w  +  vxm  +  vym'}  —  trinn  ; 

now,  since  J3'a  =  r  +  /3a,  and  because  ax,  fty,  OL'X,  ft'y,  rx  are  matrices  of 
integers,  we  have 

nn'  =  xa'axm?  +  (yJ3a'x  +  y^ax)  mm  +  yft'Pym"1 
=fm  +f'm'  +  ryxmm   (mod.  2), 

where  /,  /'  denote  respectively  the  rows  of  integers  formed  by  the  diagonal 
elements  of  the  symmetrical  matrices  XOL'OLX,  yP'fty  (cf.  §  327,  Chap.  XVIII.). 


Thus,  if  we  denote  ^  (u  ;  2<w,  2<o',  2?7,  277')  by  <f>  (w),  we  have 

(w  +  2vxm  +  2v'ym')  =  er{'^xm+*l>'ym'>  (w+vam+w'j/w')  +«'  (/»»+/•»»')  +Tn( 

B-  40 


628 


THE  TRANSFORMATION  OF  THETA  FUNCTIONS 


[374 


Further  if  a,  b  denote  the  matrices  of  Zp  columns  and  p  rows,  given 
respectively  by 

a  =  (2ws,  2v'y),    Zirib  =  (2r(fo  2r£'y), 
we  have 


fjr^  — 

%  —  (ab-  "0  = 


y  ? 


=  (  a;  (v  £-£«)«, 


0,    -x 
yoc,      0 
so  that  a&  —  6a  =  k,  say,  is  a  skew  symmetrical  matrix  of  integers  given  by 

ab  —  ba  =  k  =  (     0  ,  —rxy  ), 
ryx,      0 


and  we  have 

a</3 

2  &„    m 


=  —  ryxmm', 


Finally,  let  X,  /x  be  rows  of  £>  quantities,  the  rows  of  conjugate  complex 
quantities  being  denoted  by  X1;  /ml}  and  let  X,  p  be  taken  so  that  the  row  of 
quantities  a  (X,  p,)  consists  of  zeros,  or 

a  (X,  /ji)  =  2twX  +  %v'yp  =  0, 


so  that  af\  =  —  T'yfji,  where*  r  =v~lv',  is  a  symmetrical  matrix,  =  p'  +  ia-',  say, 
p'  and  cr'  being  matrices  of  real  quantities  ;  then  by 


we  have 
ik  (X, 


=  -  r 


in  which  v  =  yp,  ^  =  y^  ;  as  in  §  325,  Chap.  XVIII.,  since  r  is  positive,  the 
form  ra-'vv-i  is  necessarily  positive  except  for  zero  values  of  p. 

On  the  whole,  comparing  formula  (II),  §  354,  Chap.  XIX.,  the  function 
<f>(w)  satisfies  the  conditions  of  §§  351  —  2,  Chap.  XIX.,  necessary  for  a 
Jacobian  function  of  w  in  which  the  periods  and  characteristic  are  given  -f-  by 

i«?,  2v'y), 


e  = 


*  The  determinant  of  the  matrix  u  is  supposed  other  than  zero,  as  in  Chap.  XVIII.,  §  324. 

+  In  §  351,  Chap.  XIX.,  the  row  letters  have  a  elements  ;  in  the  present  case  a  is  equal  to  2p, 
and  it  is  convenient  to  represent  the  corresponding  row  letters  by  two  constituents,  each  of  p 
elements  ;  and  similarly  for  the  matrices  of  2p  columns  and  p  rows. 


374] 


IS   A   CASE   OF   THE   EXPRESSION   OF   JACOBIAN    FUNCTIONS. 


627 


To  this  function  we  now  apply  the  result  of  §  359,  Chap.  XIX.,  in  order  to 
express  it  by  theta  functions  of  w.     The  condition  for  the  matrix  of  integers 

there  denoted  by  g,  namely  geg  =  k,  is  satisfied  by  g  =  (     '     ) ,  for 

v "  >  y  i 

(  rx,   0  )  (  0,   -1  )  (  rx,   0  )  =  (  rx,  0  )  (    0,    -y   )  =  (    0  ,  -rxy)\ 


0,   y         1,0 


0,   y 


0,   y         rx,     0 


ryx,      0 


hence,  with  the  notation  of  §  358,  Chap.  XIX., 


0    ]=(2v/r,    2t/), 


o  ,  r1 
i 


-X' 


o    U 


0  ,  yr 

Hence,  as  our  final  result,  by  §  359,  Chap.  XIX.,  the  function  </>  (w),  or 
^  (u ;  2&),  2&)',  2?;,  277'),  can  be  expressed  as  a  sum  of  constant  multiples  of 
functions*  §  (w  ;  2v/r,  2i/,  2£  2f  )  m'«A  different  characteristics,  the  number  of 
such  terms  being  at  most  VjlTi  =  T*  #  |y|t  wAere  [#(,  |y|  de,lote  *Ae 
determinants  of  the  matrices  x,  y.  This  is  an  extension  of  the  result 
obtained  when  the  matrices  a,  j3,  a,  j3'  are  formed  with  integers  ;  as  in  that 


y\,  owing 


case  there  will  be  a  reduction  in  the  number  of  terms,  from  r* 
to  the  fact  that  the  function  </>  (w)  is  even.  A  similar  result  holds  whatever 
be  the  characteristic  of  the  function  ^  (u  ;  2<w,  2<o',  277,  277').  The  generalisa 
tion  is  obtained  quite  differently  by  Prym  and  Krazer,  Neue  Grundlagen 
einer  Theorie  der  allgemeinen  Thetafimctionen  (Leipzig,  1892),  Zweiter  Theil, 
which  should  be  consulted. 

Ex.     Denoting  by  E  the  matrix  of  p  rows  and  columns  of  which  the  elements  are  zero, 
other  than  those  in  the  diagonal,  which  are  each  unity,  and  taking  for  the  matrices  a,  /3, 

a',  /^  respectively  ^  E,  0,  0,  —  E,  where  m,  n  are  integers  without  common  factor,  we  have 
the  formula 


n 
« 2261— 

* 


ms/n\ 
nr/mj ' 


wherein  r,  s  are  rows  of  p  positive  integers,  in  which  every  element  of  r  is  0  or  numerically 
less  than  m,  and  every  element  of  s  is  0  or  numerically  less  than  n.  This  formula  includes 
that  of  §  284,  Ex.  iii.  (Chap.  XV.)  ;  it  is  a  particular  case  of  a  formula  given  by  Prym  and 
Krazer  (loc.  cit.,  p.  77). 

To  obtain  a  verification—  the  general  term  of  the  right  side  is  e*,  where 


40—2 


That  is,  functions  3  (rw,  2v,  2ri/,  2f/r,  2f  )  ;  cf.  §  284,  p.  448. 


628  THE   ALGEBRAICAL    APPLICATIONS   OF   THE   THEORY.  [374 

hence  26*  =  0  unless  N/m  is  integral  ;  when  N/m  is  integral,  =M,  say,  then  2e*  =  ?»pe*, 

r  r 

where 


K,  =nM+s,  obtaining  all  integral  values  when  M  takes  all  integral  values  and  s  takes  all 
integral  values  (including  zero)  which  are  numerically  less  than  n. 

375.  The  theory  of  the  transformation  of  theta  functions  may  be  said  to 
have  arisen  in  the  problem  of  the  algebraical  transformation  of  the  hyper- 
elliptic  theta  quotients  considered  in  Chap.  XL  of  this  volume.  To  practically 
utilise  the  results  of  this  chapter  for  that  problem  it  is  necessary  to  adopt 
conventions  sufficient  to  determine  the  constant  factors  occurring  in  the 
algebraic  expression  of  these  theta  quotients  (cf.  §§  212,  213),  and  to  define 
the  arguments  of  the  theta  functions  in  an  algebraical  way.  The  reader  is 
referred*  to  the  forthcoming  volumes  of  Weierstrass's  lectures. 

It  has  already  (§  174,  p.  248)  been  remarked  that  when  p>3  the  most 
general  theta  function  cannot  be  regarded  as  arising  from  a  Riemann 
surface  ;  for  the  algebraical  problems  then  arising  the  reader  is  referred 
to  the  recent  papers  of  Schottky  and  Frobenius  (Crelle,  Gil.  (1888),  and 
following)  and  to  the  book  of  Wirtinger,  Untersuchungen  uber  Thetafunctionen 
(Leipzig,  1895). 

*  Cf.  Rosenhain,  Mem.  p.  divers  Savants,  xi.  (1851),  p.  416  ft.;  Konigsberger,  Crelle,  LXIV. 
(1865),  etc. 


377] 


CHAPTER  XXI. 

COMPLEX  MULTIPLICATION  OF  THETA  FUNCTIONS.    CORRESPONDENCE  OF 
POINTS  ON  A  RIEMANN  SURFACE. 

376.  IN  the  present  chapter  some  account  is  given  of  two  theories ;  the 
former  is  a  particular  case  of  the  theory  of  transformation  of  theta  functions ; 
the  latter  is  intimately  related  with  the  theory  of  transformation  of  Riemann 
theta  functions.     Not  much  more  of  the  results  of  these  theories  is  given 
than  is  necessary  to  classify  the  references  which  are  given  to  the  literature. 

377.  In  the  transformation  of  the  function  ©  (u;  T),  to  a  function  of  the 
arguments  w,  with  period  r'  (§  324,  Chap.  XVIII.),  the  following  equations 
have  arisen 

u  =  Mw,    M=OL  +  TO.',    Mr'  =  j3  +  r/3'; 

there*  are  cases,  for  special  values  of  r,  in  which  T'  is  equal  to  r.  We 
investigate  necessary  conditions  for  this  to  be  so ;  and  we  prove,  under  a 
certain  hypothesis,  that  they  are  sufficient.  The  results  are  stated  in  terms 
of  the  matrix  of  integers  associated  with  the  transformation ;  we  do  not  enter 
into  the  investigation  of  the  values  of  r  to  which  the  results  lead.  We  limit 
ourselves  throughout  to  the  function  (B)  (u ;  r) ;  the  change  to  the  function 
^  (u ;  2o>,  2o)',  2?7,  2?/)  can  easily  be  made. 

Suppose  that,  corresponding  to  a  matrix  A  =  (  ,  ^  J ,  of  2p  rows  and 

\W,      fij  / 

columns,  for  which 

a/8  =  £a,     a'/8'  =  /S'a',     a£'  -  £*'  =  r  =  ffa.  -  a'/S, 

where  r  is  a  positive  integer,  there  exists  a  matrix  T  satisfying  the  equation 

(a  +  ra')  r  =  £  +  r/3', 

which  is  such  that,  for  real  values  of  nl}  ...,  np,  the  imaginary  part  of  the 
quadratic  form  rn2  is  positive. 

*  References  to  the  literature  for  the  case^  =  l  are  given  below  (§  383).  For  higher  values  of 
p,  see  Kronecker,  Berlin.  Monatsber.  1866,  p.  597,  or  Werke,  Bd.  i.  (Leipzig,  1895),  p.  146; 
Weber,  Ann.  d.  Mat.,  Ser.  2,  t.  ix.  (1878—9),  p.  140;  Frobenius,  Crelle,  xcv.  (1883),  p.  281, 
where  other  references  are  given ;  Wiltheiss,  Bestimmung  Abehcher  Funktionen  mit  zwei 
Argumenten  u.  B.  w.  Habilitationsschrift,  Halle,  1881  (E.  Karras),  and  Math.  Annal.  xxvi. 
(1886),  p.  130. 


630  STATEMENT   AND   PROOF  OF  THE   NECESSARY  [377 

In  that  case,  as  follows  from  Chap.  XX.,  the  function  ®  [(a  +  rot')  w ;  T], 
when  multiplied  by  a  certain  exponential  of  the  form  e?™*,  is  expressible  as  an 
integral  polynomial  of  the  r-th  degree  in  2p  functions  ®  [w ;  T]  ;  on  this 
account  we  say  that  there  exists  a  complex  multiplication*,  or  a  special 
transformation,  belonging  to  the  matrix  A.  The  equation  (a  +  TO?)T  =  /3+T/3' 
is  equivalent  to  (/•?'  —  TO!)  r  =  —  ft  +  TO.  ;  this  arises  from  the  supplementary 
matrix 


just  as  the  former  equation  arises  from  A  ;  we  put  M  =  a  +  TOE',  N  =  ft'  —  ra  ; 
we  denote  by  A  —  X  the  determinant  of  the  matrix  A  —  \E,  where  E  is  the 
matrix  unity  of  2p  rows  and  columns,  and  X  is  a  single  quantity  ;  similarly  we 
denote  by  M  —  X  the  determinant  of  the  matrix  M  —  XJE",  where  E'  is  the 
matrix  unity  of  p  rows  and  columns. 

Then  we  prove  first,  that  when  there  exists  such  a  complex  multiplication, 
to  every  root  of  the  equation  in  X  of  order  p  given  by  \  M  —  X  =0,  there 
corresponds  a  conjugate  complex  root  of  the  equation  N  —  X  |  =  0  ;  that  the  Zp 
roots  of  the  equation  A  —  X  =0  are  constituted  by  the  roots  of  the  two  equations 
|lf-X|  =  0,  N-\\  =  0,  or  A-X  =  M  —  \  \N-\\;  and  that  all  these 
roots  are  of  modulus  *Jr.  Hence  when  r  =  1,  they  can  be  shewn  to  be  all 
roots  of  unity. 

378.  The  equations  of  the  general  transformation,  of  order  r,  and  its  supplementary 
transformation,  namely 

M 
give 

hence,  if  r=r1+^r2,  where  rl  and  r.2  are  matrices  of  real  quantities,  and  similarly  r  —  i-/  +  tV2', 
we  have  by  equating  imaginary  parts 

(a  +  T^G')  T2'  =  r2  (&  ~  a'ri')  J 
therefore  the  two  matrices 


)  r/  +  tV2  aV2',     r2  ^V=  r2  (ft  —  a'r/)  —  zV2  aV2' 
are  conjugate  irnaginaries,  =f+ig  and/—  igt  say. 
Now  suppose  T'  =  T  ;  then  from 

MTZ  =/+  ifft    T2F=/-  iff, 

we  have,  if  X  be  any  single  quantity,  and  J/0  be  the  matrix  whose  elements  are  the 
conjugate  complexes  of  the  elements  of  J/, 

(J/0  -  X)  r2  =/-  ig  -  Xr2  =  r2  (N  -  X), 
and  hence,  as  |  r2  1  is  not  zero, 

|jr.-xf-|jr-u 

*  The  name  principale  Transformation  has  been  used  (Frobenius,  Crelle,  xcv.). 


378]  CONDITIONS   FOR   THE   MATRIX   OF   TRANSFORMATION.  631 

which  shews  that  to  any  root  of  the  equation  \M-\  \  =  0  there  corresponds  a  conjugate 
complex  root  of  the  equation  |  /V-X  |  =0.     Further  we  have,  if  r0  =  r1  —  iY2, 

/I    r  \  /a    0\  =  /J/    #r    \        /J/    0   \  /I 
VI  rj  U  07  "  Wo  JftfiJ      V  0    #o/  V 

and  writing  this  equation  in  the  form 

where 

1 

1 

it  easily  follows  that  the  determinant  of  the  matrix  t  is  not  zero,  and  that,  if  X  be  any 
single  quantity,  we  have 

so  that 

I    A        \    ,        I  \    I  Tf       \    I        I/"         \    I I    \f       \    I    I    AT"       "\ 

A  —  A     ^     Lt  —  A     ==     JJL  —  A         Jfl  Q  —  A     —  (  JJ1  —  A       |  XT  —  A 

Thus  the  roots  of  the  equation  |  A  -  X  '  =  0  are  constituted  by  the  roots  of  the  equations 


Further,  from  a  result   previously  obtained   (Chap.   XVIII.,  §   325,   Ex.),   when,  as 
here,  T'  =  T  and  2<u  =  l,  2v  =  l,  we  have 


also  as,  for  real  values  of  %,  ...,  np,  the  form  r2?i2  is  a  positive  form,  it  can  be  put  into  the 
shape  mj*  +  ......  +*£,  =Emz,  say,  ^  being  the  matrix  unity  of  p  rows  and  columns,  and 

m  being  a  row  of  quantities  given  by  m  =  Sn,  where  S  is  a  matrix  of  real  elements  ;  the 
equation  rinz  =  E.  Sn.  Sn  gives  Tz  =  tiES=X8  ;  for  distinctness  we  shall  write 

r2  =  AYf0, 
K=K0  =  S  being  conjugate  complex  matrices.     Take  now  a  matrix  R  =  KMK~l  ;  then 

K'1  -  K~  lMrMK~l  =  rK~     K~l  =  r  ; 


thus  if  X  be  a  root  of  j  M—\   =0,  and  therefore,  as  R-\  =  K  (M-\~)  K~l,  also  a  root  of 
R-\  |  =0,  and  if  2,  =z  +  iy,  be  a  row  of  p  quantities  such  that  Rz=\z=E\z,  where  E  is 
the  matrix  unity  of  p  rows  and  columns,  we  have 

SiRfyz  =  R0z0.  Rz  —  E\0z0  .  E\z  =  XX0  .  Ez0z 
or 


Therefore  as  Ez9z,  which  is  equal  to   2   (^m+y2m),  is  not  zero,  it  follows  that  XX0  =  r;  in 

m=l 

other  words,  all  the  roots  of  the  equations  ;  M—  X  =0,  |  A  -  X  |  =  0,  are  of  modulus  Jr. 

Suppose  now  that  r  =  l,  so  that  the  roots  of  the  equation  |  A  —  X  |  =  0  are  all  of  modulus 
unity  ;  then  we  prove  for  an  equation 


of  any  order,  wherein  the  coefficients  .1,  /?,  ...,  AV  are  rational  integers,  and  the  coefficient 
of  the  highest  power  of  x  is  unity,  that  if  all  the  roots  be  of  modulus  unity,  they  are  also 
roots  of  unity*  ;  so  that,  for  instance,  there  is  no  root  of  the  form  elV2. 

*  Kronecker,  Crelle,  LIII.  (1857),  p.  173;  Werke,  Bd.  i.  (1895),  p.  103. 


632  NECESSARY   CONDITIONS.  [378 

Let  the  roots  be  e1",  e^,  ...,  so  that 

A=  -  (cos  a+cos/3  +  ...),     #  =  cos 


then  A  lies  between  -  n  and  n,  and  B  lies  between  ±\n  (n  -  1),  etc.  ;  hence  there  can  only 
be  a  finite  number,  say  k,  of  equations  of  the  above  form,  whereof  all  the  roots  are  roots  of 
unity.  Thus,  if  xlt  ...,  xn  be  the  roots  of  our  equation,  so  that,  for  any  positive  integer  /*, 
the  roots  of  the  equation 


are  also  roots  of  unity,  it  follows  that,  of  the  equations 

^0*0  =  0,     ^2(a;)  =  0,  ...,     Ft  +  l(x)  =  0, 

there  must  be  two  at  least  which  are  identical.     Hence,  supposing  F  (x)  =  0,  F  (x)  =  0  to 
be  identical,  we  have  n  equations  of  the  form 

fX.  _      V  fl  _      V 

x\~xrj        •****%'  ••" 
Choosing  from  these  equations  the  cycle  given  by 

i~    r,'        r,        «,'""'        nti~    l' 
consisting,  suppose,  of  o-  equations,  we  infer  that 


and,  hence,  that  x±  is  a  (p*  —  v°")-th  root  of  unity. 
Ex.     Prove  that,  when  M=a  +  ra,  .¥r'  =  /3  +  7-/3', 

/ir\/«  0\    /jrowiyx 

Vl   Tj\J  ft)       VO   JfoAl   rj' 

and  deduce*,  if  A  =  f  a,  '    )  and 
\*  P  / 

'1      0 


that 

Hence,  when  T'  =  T,  if  s  be  a  row  of  2jt?  elements,  and  #  =  A?,  we  have 


which  expresses  a  self- transformation  of  the  quadratic  form  Hz2,  which  has  real  coefficients. 
Cf.  Hermite,  Compt.  Rendus,  XL.  (1855),  p.  785  ;  Laguerre,  Journ.  de  I'ec.  pol.,  t.  xxv., 
cah.  XLII.  (1867),  p.  215  ;  Frobenius,  Crelle,  xcv.  (1883),  p.  285. 

379.     Conversely,  let 


be  a  matrix  of  integers  of  2p  rows  and  columns,  such  that 

aa'  =  a'a,     J3/3'  =  J3'j3,     a/3'  -  a/3  =  r  =  yS'a - /ffa', 

*  Cf.  Chap.  XVHI.  §  325,  Ex. 


381]  SUFFICIENT   CONDITIONS   FOR   A   COMPLEX   MULTIPLICATION.  633 

where  r  is  a  positive  integer  ;  and  suppose  that  the  roots  of  the  equation 
|  A  —  \  =  0  are  all  complex  and  of  modulus  \Jr.  Under  the  special 
hypothesis*  that  the  roots  of  \  A  —  A,  =0  are  all  different,  we  prove  now  that 
a  matrix  r  can  be  determined  such  that  (i)  r  is  a  symmetrical  matrix,  (ii)  for 
real  values  of  nlt  ...,  np  the  imaginary  part  of  the  quadratic  form  rri*  is 
positive,  (iii)  the  equation 

(a  +  rat)  r  =  /3  +  r/3' 

is  satisfied.   Thus  every  such  matrix  A  gives  rise  to  a  complex  multiplication. 

380.  We  utilise  the  following  lemma,  of  which  we  give  the  proof  at  once.  —  If  A  be  a 
matrix  of  n  rows  and  columns,  such  that  the  determinant  |A  +  X  ,  wherein  X  is  a  single 
quantity,  vanishes  to  the  first  order  when  X  vanishes,  and  if  #,  y  be  rows  of  n  quantities 
other  than  zero,  such  that 

hx=0,     hy=Q, 

then  the  quantity  xy,  =x1yl  +  ......  +  xnyn,  is  not  zero. 

Denoting  the  row  x  by  £t,  its  elements  being  £n,  ...,  £ln,  determine  other  n(n-l) 
quantities  £i>;-  (i=2,  ...,  n  ;  _/=!,...,  n)  such  that  the  determinant  |£  |  does  not  vanish  ; 
similarly,  denoting  y  by  TJI}  determine  n(n-\)  further  quantities  i^y  such  that  the 
determinant  |  rj  \  does  not  vanish.  Then  consider  the  determinant  of  the  matrix  rj  (h  +  A)  £  ; 
the  (r,  s)-th  element  of  this  matrix  is 

2  rjr>  i  2  Ai,  >£«,.,•  +  X  2  77,.,  i£gj  i  =  2  £,,  y  2  /^  y^,-,  f  +  X  2  rjri  ^r>  iy 
i  j  i  .1  i  i 

(i=l,  ...,»;  _/=!,  ...,  «),  and  when  r=l  we  have 

2Ai 

1 

while  when  8  =  1,  we  have 

2^,>&,,-=Wi,1  +  ......  +/*i,»«i,n=(^)«=0; 

thus  the  (1,  l)-th  element  of  this  matrix  is  \xy,  and  every  other  element  in  the  first  row 
and  column  has  the  factor  X  ;  thus  the  determinant  of  the  matrix  is  of  the  form  X  [Axy  +  \B\. 
But  the  determinant  of  the  matrix  is  equal  to|A+X||£||?7|,  and  therefore  by  hypothesis 
vanishes  only  to  the  first  order  when  X  vanishes.  Thus  xy  is  not  zero. 

381.  Suppose  now  that  X,  X0,  /*,  ^0,  ...  are  the  roots  of  the  equation  |  A  —  A  |  =0,  where 
X  and  X0,  and  p  and  /*„,  etc.  are  conjugate  complexes.     It  is  possible  to  find  two  rows  x,  a/, 
each  of  p  quantities,  to  satisfy  the  equations 


x'  =  \x',  or,  say,  (A-A)(#,  tf')  =  0,  (i), 

and  similarly  two  rows  z,  /,  each  of  p  quantities,  to  satisfy  the  equations 

az  +  $z'  =  iLZ,     a'z  +  P'z'  =  nz',  (ii)  ; 

from  equations  (i),  if  o;0  be  the  conjugate  imaginary  to  x,  etc.,  it  follows,  since  XX0=r,  that 

V  T 

'  ' 


and  hence,  in  virtue  of  the  relations  satisfied  by  the  matrices  a,  /3,  a',  ft,  we  have 

£'.r0  -  j3.r0'  =  X.r0  ,     —  a'^0  +  ax0'  =  \x0'  , 
*  For  the  general  case,  see  Frobenius,  Crelle,  xcv.  (1883). 


OF  THF 

UNIVERSITY 


634  DETERMINATION    OF    A   COMPLEX    MULTIPLICATION  [381 

which  belong  to  the  supplementary  matrix  rA"1  just  as  the  equations  (i)  belong  to  the 
matrix  A  ;  for  our  purpose  however  they  are  more  conveniently  stated  by  saying  that 
t  =  x0',  t'=  —  x0,  satisfy  the  equations 

(A-A)(*,  0  =  0; 
hence  as  x,  x'  satisfy  the  equations 

(A-»(*,«0=0, 

it  follows  from  the  lemma  just  proved,  putting  n  =  2p,  that  tx  +  t'x'  is  not  zero  ;  in  other 
words  the  quantity 

is  not  zero.     Further  from  the  equations  (i),  (ii)  we  infer 

\H  (xz1  -  x'z]  =  (ax  +  Qz')  (a'z  +  /3Y)  -  (a'x  +  /3V)  (as  +  /3/)  ; 

and  by  the  equations  satisfied  by  the  matrices  a,  /3,  a',  ft  this  is  easily  found  to  be  the 
same  as 

(X/Li  -  r)  (xzf  -  x'z]  =  0  ; 

thus,  as  the  equation  X/z  =  r  would  be  the  same  as  X  =  X0  ,  we  have 

xz'  —  x'z=  0. 
Also  we  have 

az0  +  ftz0'  =  fi0z0,     a'z0  +  p'z0'  =  /i0  00'  ; 

thus  we  deduce,  as  in  the  case  just  taken,  that 

(Vo-^O^o'-AO^O; 

and  hence  as  X/*0  -  r,  =r  (X/^i  -  1),  is  not  zero,  we  have 

xz0'  —  x'z0  =  0. 

If  we  put  x=x1  +  -ixz,  x0=xl-ix2,  x'=xl'  +  ix2',  x§=x{-ix^,  the  quantity 
xx0'  —  X'XQ  =  —  2i  (x^  -  x^x^) 

is  seen  to  be  a  pure  imaginary  ;  if  in  equations  (i)  X  be  replaced  by  X0,  the  sign  of  xx^-x'x^ 
is  changed,  but  the  quantity  is  otherwise  unaltered  ;  since  then  the  equations  (i)  de 
termine  only  the  ratios  of  the  constituents  of  the  rows  x,  x',  we  may  suppose  the  sign  of 
the  imaginary  part  of  X  in  equations  (i),  and  the  resulting  values  of  the  constituents  of  x  and 
x',  to  be  so  taken  that 

uCtJGfr        3G  X{\  :=    —  —  '   * 

this  we  shall  suppose  to  be  done  ;  and  we  shall  suppose  that  the  conditions  for  the  (p—  1) 
similar  equations,  such  as 

zz0'-z'z0=  -2i, 

are  also  satisfied.     With  this  convention,  let  the  constituents  of  x  and  x1  be  denoted  by 

si,  i  >  •  •  •  >  si.  i»  s  i,  1  1  •  •  •  >  £  it  P  5 

similarly  let  the  constituents  of  the  rows  2,  &',  which  are  taken  corresponding  to  the  root  p, 
be  denoted  by 

S2,  1>   •••>  C2,P>    b2,  1>   •••»  ?2,P> 

and  so  on  for  all  the/>  roots  X,  p,  ....  Then  the  equations  xx0'  -  X'XQ  =  -2i,  zz0'  —  z'z0=  —2i, 
etc.,  are  all  expressed  by  the  statement  that  the  diagonal  elements  of  the  matrix 


are  each  equal  to  -  2i.     When  r  is  not  equal  to  s  (r,  s<p  +  l),  the  (1,  2)-th  element  of  this 
matrix  is 


382]  CORRESPONDING   TO    A   GIVEN    MATRIX   OF    PROPER   FORM.  635 

which  we  have  shewn  to  be  zero  ;   similarly  every  element  of  the  matrix,  other  than  a 
diagonal  element,  is  zero  ;  we  may  therefore  write 


Take  now  a  row  of  p  quantities,  £,  and  define  the  rows  X,  X'  by  the  equations 

X=lt,     X'=$t, 
so  that 

^0  =  bO^O)       ^0=fo'o> 

then 


hence  it  follows  that  the  determinant  of  the  matrix  %  is  not  zero,  since  otherwise  it  would 
be  possible  to  determine  t,  with  constituents  other  than  zero,  so  that  Jf'  =  0,  and  therefore 
also  JT0'=0  ;  as  this  would  involve  -2wy  =  0,  it  is  impossible. 

382.     If  now  the  matrix  T  be  determined  from  the  equations 

<u  +  TX'  =  0,     2  +  rz  =  0,  ...  , 

where  x,  x  are  determined,  as  explained,  from  a  proper  value  of  A,,  etc.,  or, 
what  is  the  same  thing,  if  r  be  defined  by 

r+fr-o, 

then 

fF-rf-r^-r^-rV-W; 

but  the  equations  of  the  form  xz  —  xz  =  Q  are  equivalent  to 

*F-ri=o; 

now,  since  the  determinant  |  £'  does  not  vanish,  a  row  of  quantities  t  can  be 
determined  so  that  X'  =  gt,  for  an  arbitrary  value  of  X'  ;  thus  for  this 
arbitrary  value  we  have 

(T-r)Z/2  =  0, 
and  therefore 

T  =  T, 

or  the  matrix  T  is  symmetrical. 

Further,  from  the  equation  £  +  £V  =  0,  we  have 

&'  -  rl.  =  rroio'  -  rr|o'=  r  (T,  -  T>  g/, 

and  hence,  if  r  =  p  +  to-,  since  ££,'  -  f  '|0  =  -  2t,  we  have 

I  =  f0io',  or  t0t  =  <rXQ'X', 

where  «  is  a  row  of  any  jt>  quantities  and  X'  =  £'t  ;  hence,  since  the  determi 
nant  g  does  not  vanish,  it  follows,  if  X'  be  any  row  of  p  quantities,  that 
<rX0'X'  is  positive  ;  in  particular  when  n1}  ...,np  are  real,  the  imaginary  part 
of  the  quadratic  form  r?i2  is  positive. 

Finally  from  the  equations 

ax  +  fix'  =  \x,     afx  +  fix  =  \x', 


636  EXAMPLE   OF   COMPLEX   MULTIPLICATION  [382 

putting  x  =  —  TX,  we  infer 

(/8  —  CUT)  x  —  —  \TX',     (/3'  —  a'r)  x  =  \x', 
and  therefore 

T  (/S'  -  err)  X  +(/3  —  ar)  a/  =  0, 
or 

[/8  +  r/3'  -  (a  +  TO?)  T]  #'  =  0, 

and  hence 

[£  +  r/3'  -  («  +  ra')  r]  £'  =  0, 

from  which,  as  |  f  '  j  is  not  zero,  we  obtain 

/3  +  r/3'  -  (OL  +  ra.')  T  =  0. 
We  have  therefore  completely  proved  the  theorem  stated. 

It  may  be  noticed,  as  follows  from  the  equation  £  +  fr=0,  that  we  may  form  a  theta 
function  with  associated  constants  given  by 

2o>  =  2£',     2co'=-2£; 
these  will  then  satisfy  the  equations 

co'co  —  aw'  =  0,      o>o>o  —  o>  O>Q  —  —  2*  ; 

the  former  equation  always  holds  ;   the  matrix  a>  can  be  determined  so  that  the  latter 
holds,  as  is  easy  to  see. 

Ex.     Prove  that  by  cogredient  linear  substitutions  of  the  form 

u'  =  cu,    w'  =  cw, 
we  can  reduce  the  equations  u  =  Mw  to  the  form 


where  p.lt  ...,  p.p  are  the  roots  of  |  M-\  =0. 

383.     For  an  example  we  may  take  the  case  p  =  l  ;  suppose  that  a,  ft,  a,  ft'  are  such 
integers  that  aft'  -  a'ft=r,  a  positive  integer,  and  that  the  roots  of  the  equation 


are  imaginary  ;  if  a'  =  0,  the  condition  thatr  should  not  be  a  rational  fraction  requires  that 

a  /n_/«o\ 

a'  ft')'  W' 


where  a?  =  r,  and  then  the  equation  for  T  is  satisfied  by  all  values  of  T  ;  this  case  is  that  of 
a  multiplication  by  the  rational  number  a,  and  we  may  omit  it  here  ;  when  a  is  not  zero 

we  have  _ 

2aV  =  -  (a  -  ft')  ±  \/(a 


and  therefore  (a+/3')2<4r;   this  of  itself  is  sufficient  to  ensure  that  the  roots  of  the 
equation 


are  unequal,  conjugate  imaginaries,  of  modulus  -Jr. 


FOR  THE   ELLIPTIC   FUNCTIONS. 


637 


383] 

If  then  r  be  any  given  positive  integer  and  h  be  a  positive  or  negative  integer 
numerically  less  than  2jr,  and  a,  a'  be  any  integers  such  that  (a2-£a  +  r)/a'  is  integral, 
=  -  ft  we  obtain  a  special  transformation  corresponding  to  the  matrix 


for  a  value  of  r  given  by 


a    h  — 


A-2a 


where  |  a'  |  is  the  absolute  value  of  a',  and  the  square  root  is  to  be  taken  positively  ;  the 
corresponding  value  of  M  is  a  +  ra'.     Hence  by  the  results  of  Chap.  XX.,  the  function 


when  multiplied  by  a  certain  exponential  of  the  form  exw*,  is  expressible  as  an  integral 
polynomial  of  order  r  in  two  functions  0  [w  ;  -     ""^  I  with  different  character 

istics. 

The  expression  for  the  elliptic  functions  is  obtainable  independently  as  in  the  general 
case  of  transformation.     When 

Mv  =  <»a  +  a>'a,     Mv  =  wj3  +  <o'|3',     ap>-a'@  =  r,     tl  =  Mw, 

if  to  any  two  integers  m,  m!  we  make  correspond  two  integers  n,  n'  and  two  integers  k,  V, 
each  positive  (or  zero)  and  less  than  r,  by  means  of  the  equations 

rn  +  k  =  mfi  -  m'fi,     rn'  +  k'=-  ma  +  m'a, 
or  the  equivalent  equations 


'  =  na'  +  rip'  +  -  (a' 


then  we  immediately  infer  from  the  equation 

^(w)  =  tt-2+22'[(tt  +  2m«  +  2?ftV)-2-(2 

m  m' 

by  using  n,  ri,  instead  of  m,  m',  as  summation  letters,  that 


2v, 


wherein  the  summation  refers  to  the  r-  1  sets  k,  k'  other  than  k  =  k'=Q,  for  which  (§  357, 

p.  589)  the  congruences 

ak  +  pk'  =  0,     a'k  +  pk'  =  0     (mod.  r) 
are  satisfied*. 

This  formula  is  immediately  applicable  to  the  case  when  there  is  a  complex  multiplica 
tion  ;  we  may  then  put 

2o)  =  2u=l,     2«'  =  2w'  =  T,     p  =  h-a,      -  ft  =  (a2  -  ha  +  r)/a',     r  =  (£-2a±zV4r-/i2)/2a', 

*  When  these  congruences  have  a  solution  (k0,  kQ'),  in  which  fr0,  /r0'  have  no  common  factor, 
i.e.  (Appendix  11.,  §  418)  when  a,  a',  /3,  ft'  have  no  common  factor,  the  remaining  solutions  are  of 
the  form  (XA-0,  \k0'),  where  \<r;  in  that  case  taking  integers  x,  x'  such  that  k0x'  -  k0'x  =  l,  it  is 
convenient  to  take  2vk0  +  2v'k0'  and  2vx  +  2v'x'  as  the  periods  of  the  functions  g)  on  the  right  side. 


638  EXAMPLE   OF  THE   ELLIPTIC   CASE.  [383 

and  M—(h±i^4r-h2)/2,    as  above,   where  A2<4r.     The  application   of   the    resulting 
equation  is  sufficiently  exemplified  by  the  case  of  r  —  2  given  below  (Exx.  ii.,  in.). 

In  the  particular  case  where  r=l,  the  condition  7i2<4r  shews  that  h  can  have  only  the 
values  0  or  +  1  or  -  1  ;  in  this  case  the  values  «,  n'  given  by 


,        ,,,,-,       s 
m  —  na  +  n  (h  —  a) 
a 

n   m   and    m'  are  integral; 
immediately  find 


are  integral  when   m   and    m'  are  integral;    hence  as    —  -  --  "  --  \-(k-a)T  =  MT,   we 


1 
=  6022' 


2         \° 
=     =  )  3V 
*-*2' 


7  --  u 

n  (ro+m'r)8 

Thus  when  h  =  Q  we  have  g3=0,  and  if  a,  a'  be  any  integers  such  that  (a2  +  l)/a'  is  integral, 
we  have  T=(  +  i—a)/a,  the  upper  or  lower  sign  being  taken  according  as  a  is  positive  or 
negative.  In  this  case  the  function  g>  (u)  satisfies  the  equation 

(iW=4($to) 
where 


When  h  =  l  we  have  ff2  =  0,  and  if  a,  a'  be  any  integers  such  that  (a2-a  +  l)/o'  is 
integral,  we  have  T  =  (l  —  2a  +  ^\/3)/a'  ;   in  this  case 


When  h  =  -  1,  we  have  <72  =  0,  and,  if  (a2  +  a  +  l)/a'be  integral,  then  r-  (  -  1  -  2a±t'V3)/a. 

Ex.  i.  Denoting  the  general  function  <@u  by  ljf>(«;  g%,  <73),  it  is  easy  to  prove  that  the 
arc  of  the  lemniscate  r2  =  a2  cos  2$  is  given  by  a2//-2  =  £>  (s/a  ;  4,  0)  ;  when  n  is  any  prime 
number  of  the  form  4&  +  1  the  problem  of  dividing  the  perimeter  of  the  curve  into  n  equal 
parts  is  reducible  to  the  solution  of  an  equation  of  order  k  —  when  n  is  a  prime  number 
of  the  form  2A  +  1,  the  problem  can  be  solved  by  the  ruler  and  compass  only.  (Fagnano, 
Produzioni  Matematiche,  (1716),  Vol.  u.  ;  Abel,  CEuvres,  1881,  t.  I.,  p.  362,  etc.)  It  is 
also  easy  to  prove  that  the  arc  of  the  curve  i^  —  a?  cos  30  is  given  by  a2/r2  =  $(s/a;  0,  4); 
when  n  is  a  prime  number  of  the  form  6^  +  1,  the  problem  of  dividing  the  perimeter  of 
this  curve  into  n  equal  parts  is  reducible  to  the  solution  of  an  equation  of  order  k  (Kiepert, 
Crelle,  LXXIV.  (1872),  etc.).  These  facts  are  consequences  of  the  linear  special  transforma 
tions  of  the  theta  functions  connected  with  the  curves. 

Ex.  ii.    In  case  r  —  2,  taking  a  =  4,  a'  =  9,  A  =  0,  we  have  T  =  (  —  l  +  i  ^2)/9,  and 


By  expanding  this  equation  in  powers  of  w,  and  equating  the  coefficients  of  w2,  we 
find  easily  that,  if  ft)  (r/2)  =  e,  then  g2  =  J^e2,  and  g3=  —  Je3;  hence  we  infer  that  by  means 
of  the  transformation 

o/:— r  I  ® 

—  ^$  —  •tT"g  /  ,N 

we  obtain 

dx 


r    ds      i 

h    \/8P-  15£  +  7  J 


which  can  be  directly  verified.      It  is  manifest  that  when  r  =  2,  h=Q,  we  are  led  to  this 
equation  for  all  values  of  a  and  a. 


CORRESPONDENCES   ON   A   RIEMANN   SURFACE.  639 

Ex.  iii.     Prove  that  if  m  =  \  (h  +  i  \/8  -  A2),  the  substitution 


,3m*-3     1 

m*£  =  x-\  --  T  —  -.  --  -= 
m4  +  4  x-\ 

gives  the  equation 

r  *e  _n  r  '.          dx 

Jl    \/(m4  +  4)£3-15£-(m4-ll)         ./*   V(»4  +4)  **-!»*-(«•  -11) 

This  includes  all  such  equations  obtainable  when  r  =  2.     Complex  multiplication  arises 
for  the  five  cases  /i  =  0,  h—  +  1,  h=  ±2. 

.Ek  iv.     When  r-3  and_p=l,  we  see  by  considering  the  matrix 

iwo  -iwi  i 


that  the  function  eia[(l+i  \/2)  w;  i\/2]  is  expressible  as  a  cubic  polynomial  in  the 
functions  80>1(w;  t'\/2),  elfi(w;  i\/2).  The  actual  form  of  this  polynomial  is  calculable 
by  the  formulae  of  Chap.  XXI.  (§§  366,  372),  by  applying  in  order  the  linear  substitutions 

C  1%)  '  (°   "  l}  and  then  the  cubic  transformation  (0  3)  •    Hence  deduce  that  k  =  *J2-l 

and 

sn[(l  +  i\/2)  TT]  =  (l+rV2)sn  TT[l-sn2  F/sn2y]/[l-^2sn2  JF.sn2y], 

where  y  =  2(K-  i'A'')/3,  K  being  (§  365,  Chap.  XXI.)  =7^,  and  iK'  =  rK. 

For  the  complex  multiplication  of  elliptic  functions  the  following  may  be  consulted  : 
Abel,  (Euvres,  t.  I.  (1881),  p.  379  ;  Jacobi,  Werke,  Bd.  I.,  p.  491  ;  Sohnke,  Crelle,  xvi. 
(1837),  p.  97  ;  Jordan,  Cours  d'  Analyse,  t.  II.  (1894),  p.  531  ;  Weber,  Elliptische  Functionen 
(1891),  Dritter  Theil  ;  Smith,  Report  on  the  Theory  of  Numbers,  British  Assoc.  Reports, 
1865,  Part  vi.  ;  Hermite,  Theorie  des  equations  modulaires  (1859);  Kronecker,  Berlin. 
Sitzungsber.  (1857,  1862,  1863,  1883,  etc.),  Crelle,  LVII.  (1860)  ;  Joubert,  Compt.  Rendus, 
t.  L.  (1860),  p.  774;  Pick,  Math.  Annal.  xxv.,  xxvi.  ;  Kiepert,  Math.  Annal.  xxvi.  (1886), 
xxxii.  (1888),  xxxvii.,  xxxix.  ;  Greenhill,  Proc.  Camb.  Phil.  Soc.  iv.,  v.  (1882—3),  Quart. 
Journal,  xxil.  (1887),  Proc.  Lond.  Math.  Soc.  xix.  (1888),  xxi.  (1890)  ;  Halphen,  Liouville, 
(1888);  Weber,  Ada  Math.  xi.  (1887),  Math.  Annal.  xxin.,  xxxin.  (1889),  XLIII.  (1893); 
Etc. 

384.  We  come  now  to  a  different  theory*,  leading  however  in  one  phase 
of  it,  to  the  fundamental  equations  which  arise  for  the  transformation  of 
theta  functions,  that  namely  of  the  correspondence  of  places  on  a  Riemann 
surface.  The  theory  has  a  geometrical  origin  ;  we  shall  therefore  speak 
either  of  a  Riemann  surface,  or  of  the  plane  curve  which  may  be  supposed  to 
be  represented  by  the  equation  associated  with  the  Riemann  surface,  accord 
ing  to  convenience.  The  nature  of  the  points  under  consideration  may 
be  illustrated  by  a  simple  example.  If  at  a  point  a;  of  a  curve  the  tangent 
be  drawn,  intersecting  the  curve  again  in  z1}  z.,,  ...,  £n_2)  we  may  say  that  to 
the  point  x,  regarded  as  a  variable  point,  there  correspond  the  n  —  2  points 

*  For  references  to  the  literature  of  the  geometrical  theory,  see  below,  §  387,  Ex.  iv.,  p.  647. 
The  theory  is  considered  from  the  point  of  view  of  the  theory  of  functions  by  Hurwitz,  Math. 
Annul,  xxvin.  (1887),  p.  561;  Math.  Annal.  xxxn.  (1888),  p.  290;  Math.  Annal.  XLI.  (1893), 
p.  403.  See  also,  Klein-Fricke,  Modulfunctionen,  Bd.  n.  (Leipzig,  1892),  p.  518,  and  Klein,  Ueber 
Rienuinn't  Theorie  (Leipzig,  1882),  p.  67.  For  (1,  1)  correspondence  in  particular  see  the  re 
ferences  given  in  §  393,  p.  634. 


640  STATEMENT  OF   NECESSARY   CONDITIONS  [384 

z-i,  .  ..,  zn-2-  To  any  point  z  of  the  curve,  regarded  as  arising  as  one  of  a  set 
z-i,  ...,  zn-2,  there  will  reciprocally  correspond  all  the  points,  xl,  x2,  ...,  x^^, 
which  are  points  of  contact  of  tangents  drawn  to  the  curve  from  z.  Such  a 
correspondence  is  described  as  an  (n  —  2,  m  —  2)  correspondence.  A  point  of 
the  curve  for  which  x  coincides  with  one  of  the  points  zlt  ...,  zn_2  correspond 
ing  to  it,  is  called  a  coincidence  ;  such  points  are  for  instance  the  inflexions 
of  the  curve. 

In  general  an  (r,  s)  correspondence  on  a  Riemann  surface  involves  that 
any  place  x  determines  uniquely  r  places  z1,...,zr,  while  any  place  z, 
regarded  as  arising  as  one  of  a  set  zlt  .  ..,  zr,  determines  uniquely  s  places 
x-i,  ...,  Xg.  The  investigation  of  the  possible  methods  of  this  determination  is 
part  of  the  problem. 

385.  Suppose  such  an  (r,  s)  correspondence  to  exist  ;  let  the  positions  of 
z  that  correspond  to  any  variable  position  of  x  be  denoted  by  zlt  ...,  zr,  and 
the  positions  of  x  that  correspond  to  any  variable  position  of  z  be  denoted  by 
x1,  ...,  xs;  and  denote  by  c1}  ...,  cr  the  positions  of  zlt  ...,  zr  when  x  is  at  the 
particular  place  a,  and  by  a1}  ...,  as  the  positions  of  #1;  ...,  XB  when  z  is  at 
the  particular  place  c  ;  denoting  linearly  independent  Riemann  normal  inte 
grals  of  the  first  kind  by  vlt  ...,  vp,  consider  the  sum 


as  a  function  of  x  ;  since  it  is  necessarily  finite  we  clearly  have  equations  of 
the  form 

,  r         x,  a  -mf         x,  a         Zj,  cl  zr,  cr  ,  •       ,  % 

Mi>lvl     +  ......  +Mi>pvp    =vt      +  ......  +vt     ,          (i  =  I,...,p\ 

where  Miil}  ...,Mijp  are  constants.  On  the  dissected  surface  the  omitted 
aggregate  of  periods  of  the  integral  vt  indicated  by  the  sign  =  is  self-deter 
minative  ;  if  the  paths  of  integration  be  not  restricted  from  crossing  the 
period  loops  the  sign  =  can  be  replaced  by  the  sign  of  equality  (cf. 
Chap.  VIII.  §  153,  158). 

If  now  x  describe  the  &th  period  loop  of  the  second  kind,  from  the  right 
to  the  left  side  of  the  kih  period  loop  of  the  first  kind,  the  places  zlt  ...,  zr 
will  describe  corresponding  curves  and  eventually  resume,  in  some  order,  the 
places  they  originally  occupied  ;  since,  on  the  dissected  Riemann  surface 
v*l>Cl  -i-  vf'  Ca  =  VJ"  Cl  +  v*i'C*  ,  we  may  suppose  each  of  them  actually  to  resume 
its  original  position  ;  hence  we  have  an  equation 


wherein  a^fc,  «';,&,  ...  are  integers  ;  similarly  by  taking  x  round  the  kth  period 
loop  of  the  first  kind  we  obtain 


385]  FOR   AN   (r,   s)   CORRESPONDENCE.  641 

we  have  therefore  1p-  equations  expressible  in  the  form 


wherein  a,  a',  /3,  /3'  are  matrices  of  integers,  of  p  rows  and  columns. 
Consider  next,  as  a  function  of  x,  the  integral 

/.'",(' 
vm 


wherein  z,  c  are,  primarily,  arbitrary  positions,  independent  of  x,  and  IIzj;CCi 
is  the  Riemann  normal  integral  of  the  third  kind.  The  subject  of  integration 
becomes  infinite  when  any  one  of  the  places  zl,  ...,  zr  coincides  with  z,  or,  in 
other  words,  when  z  is  among  the  places  corresponding  to  x,  and  this  happens 
when  x  is  at  any  one  of  the  places  xlt  ...,xg,  which  correspond  to  z\  the 
subject  of  integration  similarly  becomes  infinite  when  x  is  at  any  one  of  the 
places  a1}  ...,  ag,  which  correspond  to  the  particular  position  of  z  denoted  by  c  ; 
it  is  assumed  that  c  does  not  coincide  with  any  one  of  the  places  cl5  ...,  cr 
The  sum  of  the  values  obtained  when  the  integral  is  taken,  in  regard  to  a, 
round  the  infinities  xly  ...,  xs,  a1}  ...,  as,  is,  save  for  an  additive  aggregate* 
of  periods  of  the  integral  vm,  equal  to 


This  quantity  is  then  equal  to  the  value  obtained  when  x  is  taken  round 
the  period  loops  on  the  Riemann  surface.  Consider  first,  for  the  sake  of 
clearness,  the  contribution  arising  as  sc  describes  the  Mb.  period  loop  of  the 
second  kind ;  if  x  described  the  left  side  of  this  period  loop  in  the  negative 
direction,  from  the  right  to  the  left  side  of  the  Kh  period  loop  of  the  first 
kind,  the  aggregates  of  the  paths  described  by  z^...,zr  would,  in  the 
notation  just  previously  adopted,  be  equivalent  to  aA)it  negative  circuits  of 
the  \th  period  loop  of  the  second  kind,  and  a'Aj  k  positive  circuits  of  the  Xth 
period  loop  of  the  first  kind  (X  =  1,  . . . ,  p).  In  the  actual  contour  integration 
under  consideration  the  description  by  x  of  the  left  side  of  the  Kb.  period  loop 
of  the  second  kind  is  to  be  in  the  positive  direction ;  hence  the  contribution 
arising  fur  the  integral  as  x  describes  both  sides  of  the  Kh  period  loop  of  the 
second  kind  is 

s. 


-  2-TTlTm,  k  2  a\,  k  V 


?,c 
A 


similarly  the  contribution  as  x  describes  the  sides  of  the  kih  period  loop  of 
the  first  kind  is 


Which  vanishes  when  paths  can  be  drawn  on  the  dissected  surface  connecting  alt  ...,  a, 
respectively  to  arlt  ...,  x,,  so  that  simultaneous  positions  on  these  paths  are  simultaneous  posi 
tions  of  a-, ,  .  . ,  x. .  Cf .  Chap.  VIII.  §  153  ;  Chap.  IX.  §  165. 

B-  41 


642  ALGEBRAIC   EXPRESSION   OF   CORRESPONDENCES  [385 

where  Em>  k  =  0  unless  m  =  k,  and  Em>  m  =  1.     Taking  therefore  all  the  period 
loops  into  consideration,  that  is,  k  =  1,  ... ,  p,  we  obtain 


« 


where  JVm,  x  =  ft\,  m  -  S  Tm>  k  «'x,  t  • 

*=i 

so  that  #„,,  x  is  the  (m,  X)th  element  of  the  matrix 

N  =  ft'-rS  ; 
since  the  equations  if  =  a  +  ra',  Mr  =  /3  +  rfi'  give 

-y8+Ta  =  (^-Ta)T, 

we  have  also  _ 


TOt. 

z,  c 


These  equations  express  the  sum  v%  "'+...  +  C'  °'  in  terms  of  integrals  j 
manner  analogous  to  the  expression  originally  taken  for  C  '+...+  wt-  ' 
in  terms  of  integrals  t;Ja,_the  difference  being  the  substitution,  for  the  matrix 


n  a 


386.  The  theory  of  correspondence  of  points  of  a  Riemann  surface  now 
divides  into  two  parts  according  as  the  equation,  which  arises  by  elimination, 
either  of  the  matrix  M  or  the  matrix  N,  namely, 

T«'T  +  O.T  —  T/3'  —  /3  =  0, 

is  true  independently  of  the  matrix  r,  in  virtue  of  special  values  for  the 
matrices  a,  ft,  a',  /3',  or,  on  the  other  hand,  is  true  for  more  general  values  of 
these  matrices,  in  virtue  of  a  special  value  for  the  matrix  T. 

We  take  the  first  possibility  first  ;  it  is  manifest  that  for  any  value  of  r 
the  equation  is  satisfied  if 

o  =  -7#,  ft  =  0,  «'  =  0,  ft'  =  -vE, 

where  7  is  any  single  integer,  and  E  is  the  matrix  unity  of  p  rows  and 
columns  ;  conversely,  if  the  equations  are  to  hold  independently  of  the  value 
of  r,  we  must  have  the  n2  equations 


O,     f  a^r^ 


and,  for  general  values  of  T,  these  give 

0^  =  0,     «m,«  =  /S/A,x,     9tiii+-fr&-*i     A 
which  are  equivalent  to  the  results  taken  above. 


386]  EXISTING   ON   A  GENERAL   RIEMANN   SURFACE.  643 

With   these    values   we   have,  as   the   particular   forms   of  the   general 
equations  of  §  385, 

Zi,  C,  Zr,  Cr  X,  a  ~ 

Vi        +  ......  +  Vt         +yVi       =0, 

x,,a,  Xs,ag  z,c        f.  /.  -,  -. 

vnt      +  ......  +vm      +  yvm    =0.        (i,  m=l,  ...,p). 

Let  the  value  on  the  dissected  surface  of  the  left  side  of  the  first  of  these 
equivalences  be 

gi  +  giTi,i  +  ......  +  g  'P  Ti,  P  > 

where  glt  ...,  gp,  #/,  .  ..,  g'p  are  integers.     Consider  now  the  function 


,  Z] 


Zr,C 


+yll 


z'c 


wherein  z1}  ...,  zr  are  the  places  corresponding  to  x,  and  clt  ...,  cr  their 
positions  when  x  is  at  a,  and  z,  c  are  arbitrary  places.  In  virtue  of  the 
equations  just  obtained  it  is  a  rational  function  of  z,  and  rational  in  the 
place  c  (cf.  Chap.  VIII.  ,  §  158).  Regarded  as  a  function  of  x  it  is  also 
rational  ;  for  the  quotient  of  its  values  at  the  two  sides  of  a  period  loop 
of  the  second  kind,  which,  by  what  has  just  been  shewn,  must  be  rational  in 
z,  is,  by  the  properties  of  the  integral  of  the  third  kind,  necessarily  of  the 
form 


where  K1}  ...,  Kp  are  integers;  this  quotient,  as  a  function  of  z,  has  no 
infinities  ;  being  a  rational  function  of  z,  it  is  therefore  a  constant,  and 
therefore  unity,  since  it  reduces  to  unity  when  z  is  at  c  ;  hence  </>  (x,  z  ;  a,  c), 
as  a  function  of  x,  has  no  factors  at  the  period  loops  ;  as  it  can  have  no 
infinities  but  poles  it  is  therefore  a  rational  function  of  x;  it  is  similarly 
rational  in  a.  As  a  function  of  x  it  vanishes  when  one  of  zl}  ...,  zr  coincides 
with  z,  that  is,  when  x  coincides  with  one  of  xlt  ....  xs. 

We  have  therefore  the  result.  Associated  with  any  (r,  s)  correspondence 
which  can  exist  upon  a  perfectly  general  Riemann  surface,  it  is  possible  to 
construct  a  function  $  (x,  z;  a,  c),  rational  in  the  variable  places  x,  z  and  the 
fixed  places  a,  c,  which,  regarded  as  a  function  of  x  vanishes  to  the  first  order 
at  the  places  xly  ...,  xg,  which  correspond  to  z,  and  vanishes  to  order  7  {if  7  be 
positive),  at  the  place  z  ;  which,  as  a  function  of  x,  is  infinite  to  the  first  order 
when  x  coincides  with  any  one  of  the  places  aly  .  ..,  ag  which  correspond  to  c, 
and  is  infinite  to  order  7  (7  being  positive)  when  x  is  at  c;  which,  as  a  function 
of  z,  has  similarly  (for  7  positive)  the  zeros  zlt  ...,  zr,  xt  and  the  poles 
Ci,  ...,  cr,  a*.  An  analogous  statement  can  be  made  when  7  is  negative. 

Ex.  i.  Some  examples  may  be  given  to  illustrate  the  form  of  this  rational  function. 
On  a  plane  cubic  curve  we  do  in  fact  obtain  a  (1,  4)  correspondence,  for  which  -y  =  2, 
by  taking  for  the  point  zl  which  corresponds  to  .r,  the  point  in  which  the  tangent  at 

41—2 


644  EXAMPLES   OF   GENERAL   CORRESPONDENCES.  [386 

x  meets  the  curve  again,  and  therefore,  for  the  points  xv,  x^  x3,  x^  which  correspond  to  2, 
the  points  of  contact  of  tangents  to  the  curve  drawn  from  z.  The  value  y  =  2  is  obtained 
from  Abel's  theorem,  which  clearly  gives  the  equation 

z,,  c,  .  n  x,  a     - 
v        +2v      =0 

as  representative  of  the  fact  that  a  straight  line  meets  the  curve  twice  at  x  and  once  at  zt. 
Denote  the  equation  of  the  curve  in  the  ordinary  symbolical  way  by  AX3  —  Q  ;  then  the 
equation  AXZA1  =  0,  for  a  fixed  position  of  x,  represents  the  tangent  at  x  ;  and  for  a  fixed 
position  of  z,  represents  the  polar  conic  of  the  point  z,  which  vanishes  once  in  the  points  of 
contact,  #!,  #2,  #3,  #4,  of  tangents  drawn  from  z  and  vanishes  also  twice  at  z,  where  it 
touches  the  curve  ;  then  consider  the  function 

AX*A. 
~A*At.A*An* 

when  z,  a,  c  are  fixed,  this  function  of  x  vanishes  to  the  first  order  at  xlt  #2,  xs,  x±  and  to 
the  second  order  at  z,  and  is  infinite  to  the  first  order  at  the  places  ax,  a2,  a3,  a4  which 
correspond  to  c,  and  infinite  to  the  second  order  at  c  ;  when  z,  a,  c  are  fixed,  this  function 
of  z  vanishes  to  the  first  order  at  zlt  and  to  the  second  order  at  x,  and  is  infinite  to  the 
first  order  at  the  place  Cj  ,  which  corresponds  to  a,  and  infinite  to  the  second  order  at  a. 

Ex.  ii.  More  generally  for  any  plane  curve  of  order  n,  and  deficiency  p,  if  to  a  point  x 
we  make  correspond  the  r  =  n  —  2  points  zl  ,  .  .  .  ,  zn  _  2  ,  in  which  the  tangent  at  x  meets  the 
curve  again,  and  to  a  point  z  the  s  =  2n  +  2p  —  4  points  of  contact  &lt  ...,  xt  of  tangents 
drawn  to  the  curve  from  z  (so  that,  for  instance,  when  the  curve  has  K  cusps,  K  of  the 
points  a?j,  ...,  xt  will  be  the  same  for  all  positions  of  z\  we  shall  have  an  (r,  s)  corre 
spondence  for  which  y  =  2.  If  Aj.n  =  0  be  the  equation  of  the  curve,  the  function 


regarded  as  a  function  of  x,  for  fixed  positions  of  z,  a,  c  (of  which  a  and  c  are  not  to  be 
multiple  points),  has  for  zeros  the  places  xlt  ...,  xg,  z2,  for  poles  the  places  alt  ...,  a,,  c2, 
and  regarded  as  a  function  of  z,  has  for  zeros  the  places  zlt  ...,  zr,  x2,  and  for  poles  the 
places  Cj,  ...,  cr,  a2. 

Ex.  iii.  If  from  a  point  x  a  tangent  be  drawn  to  a  plane  curve,  and  the  corresponding 
points  be  the  points  other  than  the  point  of  contact,  in  which  the  tangent  meets  the  curve 
again,  we  have 


where  z1  is  the  point  of  contact  of  one  of  the  tangents  drawn  from  x,  there  being  as  many 
such  equations  as  tangents  to  the  curve  from  x  ;  since  the  2n  +  2p  —  4  points  z1  lie  on  the 
first  polar  of  #,  it  follows  by  Abel's  theorem  that 

2j 
therefore 

/"c'  +  ......  + 

so  that  y  =  2/i  +  2jp-8.  As  a  function  of  z  the  function  <£  (#,  z  ;  a,  c)  has  therefore  the 
(n  —  3)  (2n  +  2p  —  4)  zeros  z1?  ...,  zr,  which  correspond  to  x,  as  well  as  the  zero  x,  of  the 
(2n  +  2p-8)th  order,  and  has  as  poles  the  places  cly  ...,  cr,  which  correspond  to  a,  as  well 
as  the  zero  a,  of  the  (2n  +  2p  -  8)th  order. 

For  instance  for  a  plane  quartic,  there  are  10  places  corresponding  to  x,  one  for  each  of 
the  tangents  that  can  be  drawn  from  x  to  the  curve  ;   the  function  $  (x,  z  ;  a,  c),  as  a 


387]  DETERMINATION    OF   THE    COINCIDENCES.  645 

function  of  z,  vanishes  to  the  first  order  at  each  of  these  ten  places,  and  vanishes  to  the 
sixth  order  at  x  ;  its  infinities  are  the  places  similarly  derived  from  the  fixed  position,  a, 
of  x.  We  can  build  up  this  function  in  the  manner  suggested  by  the  use  already  made  of 
Abel's  theorem  in  the  determination  of  the  value  of  y  ;  for  a  fixed  position  of  x,  let  T(z)  =  0 
be  the  equation,  in  the  variable  2,  for  the  ten  tangents  to  the  quartic  drawn  from  z  ;  let 
P  (z)  =  0  be  the  first  polar  of  x  ;  the  quotient 


vanishes  when  z  is  at  the  places  zlt  ...,  z10,  and  vanishes  when  z  is  at  x  to  order 
10-2(2)  =  6;  let  Ta(z\  Pa(z)  represent  what  T(z\  P(z)  become  when  x  is  at  a  ;  then 
the  function  of  z 

T(z) 


has  the  same  behaviour  as  has  the  function  0  (x,  z  ;  a,  c)  as  a  function  of  z.  From  this 
function,  by  multiplication  by  a  factor  involving  x  but  independent  of  2,  we  can  form  a 
symmetrical  expression  in  x  and  z  ;  this  will  be  the  function  <f>  (x,  z  ;  a,  c).  In  fact, 
denoting  the  equation  of  the  quartic  curve  by  ^1^  =  0,  and  expressing  the  fact  that  the  line 
joining  the  point  x  of  the  curve  to  the  point  £  not  on  the  curve  should  touch  the  curve, 
viz.,  by  equating  to  zero  the  discriminant  in  X  of  (Ax  +  \Atf-Ax*,  we  obtain  an  equation 
of  the  form 

^  [C6,  *"]  =  (AXA£?  [9  WAfF  -  IGAXA*  .  AJAJ, 

which  represents  the  tangents  to  the  curve  drawn  from  x.  Replacing  £  by  z,  a  point  on 
the  curve,  so  that  A,*  =  0,  we  have,  since  AXA  ,3=0  is  the  first  polar  of  x, 

T(z)/P*  W  =  9(AX*A*)*-16AXA*  .  AJA.  ; 
hence 


A(x  z-  a  c)  =  XX.. 

[9  (Au*A*r  -  \<>AaA?  .  AJA.]  [9  (AX*A*?  -  IQAXA*  .  Ax*Ae]  ' 

Ex.  iv.  If  a  (1,  1)  correspondence  exists,  the  rational  function  of  x,  denoted  by 
<f>  (x,  z  ;  a,  c),  is  of  order  y  +  1. 

387.  A  problem  of  great  geometrical  interest  is  to  determine  the  number 
of  positions  of  x,  in  which  x  coincides  with  one  of  the  places  zl}  ...,  zr,  which 
correspond  to  it.  This  is  called  the  number  of  coincidences. 

A  simple  way  to  determine  this  number  is  to  consider  the  rational  func 
tion  of  x  obtained  as  the  limit  when  z  =  a;,of  the  ratio  $(x,z\  a,  c)/(x  —  zf  ; 
putting 

$(x\  a,c)  =  Km  [<£  (x,  z  ;  a,  c)/(x  -  z)*], 


and  bearing  in  mind  that  if  t  be  the  infinitesimal  on  the  Riemann  surface, 
dx/dt  vanishes  to  the  first  order  at  every  finite  branch  place,  and  is  infinite  to 
the  second  order  at  every  infinite  place  of  the  surface,  we  immediately  find 
from  the  properties  of  the  function  ^>(xtz\  a,  c),  on  the  hypothesis  that  none 
of  the  branch  places  of  the  surface  are  at  infinity,  the  following  result  ;  the 
rational  function  of  x  denoted  by  <j>(x;  a,  c)  vanishes  to  the  first  order  at 
every  place  x  of  the  surface  at  which  x  coincides  with  one  of  the  places 


646  DEDUCTION    OF   THE    BITANGENTS  [387 

z1}  ...,  zr  which  correspond  to  it,  vanishes  also  to  order  2y  at  each  of  the  n 
infinite  places  of  the  surface,  and  is  infinite  to  order  7  at  each  of  the  branch 
places  of  the  surface  and  at  each  of  the  places  a,  c,  while  it  is  infinite  to  the 
first  order  at  each  of  the  places  cx,  ...,  cr  which  correspond  to  a,  and  at  each 
of  the  places  «1}  ...,  as  which  correspond  to  c  ;  hence,  denoting  the  number  of 
coincidences  by  C  we  have 

C  +  2ny  =  (2n  +  2p  -  2)  7  +  £7  +  r  +  s, 
so  that* 


The  same  result  is  obtained  when  there  are  branch  places  at  infinity. 
The  argument  has  assumed  7  to  be  positive  ;  a  similar  argument,  when  7  is 
negative,  leads  to  the  same  result. 

Ex.  i.     The  number,  i,  of  inflexions  of  a  plane  curve  of  order  n  and  deficiency  p  is 
given  (Ex.  ii.  §  386)  by 


where  h  is  the  number  of  coincidences  arising  other  than  inflexions,  as  for  instance  at  the 
multiple  points  of  the  curve.  In  determining  h  it  must  be  remembered  that  we  have  not 
excluded  the  possibility  of  there  being  fixed  positions  of  x  which  correspond  to  z  for  all 
positions  of  z  ;  for  instance  in  the  case  of  a  curve  with  cusps  all  these  cusps  have  been 
reckoned  among  the  places  &\,  ...,#„  which  correspond  to  z.  Therefore  for  a  curve  with 
K  cusps,  h  will  contain  a  term  2«  ;  for  a  curve  with  only  8  double  points  and  K  cusps,  the 
formula  is  the  well-known  one 

i—  «  =  3  (m  —  ri), 

where  m  is  the  class  of  the  curve,  equal  to  n(n  —  l)-28  —  3x. 

Ex.  ii.     Obtain  the  expression  of  the  function  <£  (x  ;  a,  c)  determined  by  the  limit 
{Af-*AJ(*-*?.Af-\A..AS-*A}^t 

where  Ax»  =  Q  =  A*=Aa»  =  Acn.     (Cf.  Ex.  ii.  §  386.) 

Ex.  iii.  The  number  of  double  tangents  of  a  curve  of  order  n  and  deficiency  p  may  be 
obtained  from  Ex.  iii.  §  386,  if  we  notice  that  a  double  tangent,  touching  at  P  and  Q,  will 
arise  both  when  P  is  a  coincidence,  and  when  Q  is  a  coincidence  ;  hence  if  T  be  the  number 
of  double  tangents,  and  h  the  number  of  coincidences  not  giving  rise  to  double  tangents, 
we  have 


where  tr  =  n-\-p  —  3.  For  instance  for  a  -curve  with  no  singular  points  other  than  8  double 
points  and  K  cusps,  there  will  be  a  contribution  to  h  equal  to  twice  the  number  of  those 
improper  double  tangents  which  are  constituted  by  the  tangents  to  the  curve  from  the 
cusps  and  the  lines  joining  the  cusps  in  pairs.  The  number  of  tangents,  t,  from  a  cusp  is 
given  (cf.  §  9,  Chap.  I.,  Ex.)  by 


-2,  or  i!  =  2/i-5- 
There  will  not  arise  any  such  contribution  corresponding  to  a  double  point,  since  the  two 

*  This  result  was  first  given  by  Cayley  ;  see,  for  references,  Ex.  iv.  below. 


387]  OF   AN    ALGEBRAIC    PLANE    CURVE.  647 

points  of  the  curve  that  there  correspond  are  different  places  (cf.  §  2,  Chap.  I.)  ;   hence 
we  have 


and  therefore  r  =  2<r  (a-  +  1)  -  4p  -  *t  -  1(*2  -  K)  ; 

substituting  the  values  for  <r,  p  and  t,  we  find  the  ordinary  formula  equivalent  to 


where  m  is  the  class  of  the  curve. 

Ex.  iv.  The  points  of  contact  of  the  double  tangents  of  a  quartic  curve  AX4  =  0  lie 
upon  a  curve  whose  equation  is  obtainable  by  determining  the  limit,  when  z=x,  of  the 
expression 

[9  (  Jz2  ^2)2  _  16  AxA?  .  A*A^(X  -  Zf. 

For  the  result,  cf.  Dersch,  Math.  Annal.  vn.  (1874),  p.  497. 

For  the  general  geometrical  theory  the  reader  will  consult  geometrical  treatises  ;  the 
following  references  may  be  given  here  ;  Clebsch-Lindemann-Benoist,  Lemons  sur  la  Geo 
metric  (Paris,  1879—1883),  t.  I.  p.  261,  t.  n.  p.  146,  t.  in.  p.  76  ;  Chasles,  Compt.  Rendus, 
t.  LVIII.  (1864)  ;  Chasles,  Compt.  Rendus,  t.  LXII.  (1866),  p.  584  ;  Cayley,  Compt.  Rendus, 
t.  LXII.  (1866),  p.  586,  and  London  Math.  Soc.  Proc.  t.  I.  (1865  —  6),  and  Phil.  Trans. 
CLVIII.  (1868)  (or  Coll.  Works,  v.  542  ;  vi.  9  ;  vi.  263)  ;  Brill,  Math.  Annal.  t.  vi.  (1873), 
and  t.  vn.  (1874).  See  also  Lindemann,  Crelle,  LXXXIV.  (1878);  Bobek,  Sitzber.  d.  Wiener 
Akad.,  xcin.  (ii.  Abth.),  (1886),  p.  899  ;  Brill,  Math.  Annal.  xxxi.  (1887),  xxxvi.  (1890)  ; 
Castelnuovo,  Rend.  Ace.  d.  Lincei,  1889;  Zeuthen,  Math.  Annal.  XL.  (1892),  and  the 
references  there  given. 

Ex.  v.     If  we  use  the  equation  (Chap.  X.  §  187) 


where  Q  is  an  odd  half-period,  equal  to  X  +  rX'  say,  X,  X'  being  each  rows  of  p  integers,  and 
form  the  rational  function  of  x  and  a, 


„.      .    7.        .    _,y 

R  (x,  a)  =  hmz=x  (  -  l)y  —  -  ,         - 

c=a  0  (#,  *  j  0,  C) 


[<t)(x,  z;  a,  c 

we  have 

l     1  IT,x,  a 


which  is  a  generalisation  of  the  equation  (i),  p.  427. 

The  function  R(x,  a)  vanishes  when  x  is  at  any  one  of  the  places  c1?  ...,  cr,  which 
correspond  to  a,  and  when  x  is  at  any  one  of  the  places  an  ...,  at  which  correspond  to  the 
position  a  of  the  place  c  ;  it  vanishes  also  2y  times  at  each  of  the  zeros  of  the  function 
e^.a-t-^Q).  It  is  infinite  C  times,  namely  when  x  has  any  of  the  positions  in  which  it 
coincides  with  one  of  the  places  2j,  ...,  zr  which  correspond  to  it.  In  the  particular  case 
of  Ex.  i.  p.  427,  the  function  R(x,a)  is  (#  -  a)2  Jf  (#),  and  the  equation  C=r  +  s  +  2py 
expresses  that  the  number  of  branch  places  (where  two  places  for  which  x  is  the  same 
coincide)  is  2  (n-  l)  +  2p. 

Ex.  vi.     Determine  the  periods  of  the  function  of  x  expressed  by 


648  EXISTENCE    OF    SPECIAL   CORRESPONDENCES.  [387 

where  zlt  ...,  zr  are  the  places  corresponding  to  x,  and  clt  ...,  cr  are  the  places  correspond 
ing  to  a. 

Ex.  vii.  If  there  be  upon  the  same  Riemann  surface  two  correspondences,  an  (r,  «) 
correspondence  and  an  (r',  a')  correspondence,  then  to  any  place  z  will  correspond,  in  virtue 
of  the  first  correspondence,  the  places  xlt  ...  ,  &•„  and  to  any  one  of  these  latter,  say  xit  will 
correspond,  in  virtue  of  the  second  correspondence,  say  z'itl,  ...,  z'i>r,  ;  conversely  to  any 
place  z'  will  correspond,  in  virtue  of  the  second  correspondence,  the  places  xlt  ...,  xs/,  and 
to  any  one  of  these  latter,  say  xt)  will  correspond,  in  virtue  of  the  first  correspondence, 
say  zitl,  ...,  zit,.  ;  we  have  therefore  an  (r's,  rs')  correspondence  of  the  points  (z,  z').  In 
virtue  of  the  equations 


we  have 


i=l  J=l 


Hence*  we  can  make  the  inference.  If  upon  the  same  Riemann  surface  there  be  two 
correspondences,  an  (r,  s)  correspondence  of  places  x,  z,  and  an  (/,  s')  correspondence  of  places 
of,  z1,  then  the  number  of  common  corresponding  pairs  of  these  two  correspondences,  for  which 
both  x,  x'  coincide,  and  also  z  and  z',  is 

r's  +  rs'  —  2yy'p. 

388.  We  have  so  far  considered  only  those  correspondences  f  which  can 
exist  on  any  Riemann  surface.  We  give  now  some  results  £  relating  to 
correspondences  which  can  only  exist  on  Riemann  surfaces  of  special  cha 
racter,  more  particularly  (1,  1)  correspondences. 

We  prove  first  that  any  (1,  s)  correspondence  is  associated  with  equations 
which  are  identical  in  form  with  those  which  have  arisen  in  considering  the 
special  transformation  of  theta  functions.  For  any  such  correspondence,  in 
which  to  any  place  x  corresponds  the  single  place  z,  and  to  any  position  of  z 
the  places  xly  ...,  #„,  we  have  shewn  that  we  have  the  equations  (i=  1,  ...,£>) 

vx;a,   M=a  +roc',    Mr=     ft+rff, 


hence 

£ 

'   »P 


z>  c  _    JUT        51      *«•  ft»  »*-         •c'      x>>  a» 


m=l 

P 

S  MI  & 
A=i 

r        ^.  c   . 


,      T  z>c 

+Li>pvp  , 


*  Provided  the  (r's,  rs')  correspondence  is  not  an  identity. 

t  Called  by  Hurwitz,  Werthigkeit-correspondenzen,  y  being  the  Werthigkeit. 

{  For  other  results,  see  Klein-Fricke,  Modulfunctionen,  Bd.  n.  (Leipzig,  1892),  pp.  540  if. 


389]  CONDITIONS   FOR   A   (1,    1)   CORRESPONDENCE.  649 

where  Li>m  is  the  (i,  m)th  element  of  the  matrix  L,  =  MN.     This  matrix  is 
therefore  equal  to  .9.     Now 

MN  =M(    J3'-Ta)  =     (a  +  ra)  ft'  -  (/8  +  r/3')  a  =      aft'-  /8o'  +  T(a'/8'-/8/a/), 
MNr  =  M  (-  J3  +  ra  )  =  -  (a  +  ra)  £  +  (/3  +  r/8')  a  =  -  (a)8  -/3o)+r(/3'a  -  a'^  ), 

which  we  may  write  in  the  form 


if  now  T  =  T1-MY2,  where  rlt  T2  are  matrices  of  real  quantities,  it  follows 
by  equating  to  zero  the  imaginary  part  in  the  equation 


that  T2£  =  0;  since  for  real  values  of  ?i1}  ...,  np  the  quadratic  form  r.2n2  is 
necessarily  positive,  the  determinant  of  the  matrix  r2  is  not  zero  ;  hence  we 
must  have  B  =  0  ;  hence  also  H  =  s  and  A  =  0  ;  or 

«£  =  £*,   <*'£'=  /3'a',   a/3'-/3a'  =  ffa-a.'/3  =  s; 

and  these  equations,  with  the  equation  (a  +  ra')  r  =  0  +  r/3',  are  identical 
in  form  with  those  already  discussed  in  this  chapter  (§§  377,  ff.). 

We  are  able  then  as  in  the  former  case  to  deduce  certain  conditions 
for  the  matrices  a,  /3,  a',  /9',  which  in  their  general  form  necessarily  involve 
special  values  for  the  matrix  T. 

389.  In  particular,  in  order  that  a  (1,  1)  correspondence*  may  exist, 
the  roots  of  the  equation  M  —  A,  =  0  must  be  conjugate  imaginaries  of  the 
roots  of  the  equation  \N—  X  j  =  0,  must  be  all  of  modulus  unity,  and  must 

be  roots  of  the  equation    A  —  X  ]  =  0,  where  A  =  (   ,  ^,  j  .     They  must  there- 

\^     /"^   / 

fore  be  roots  of  unity.  For  the  sake  of  definiteness  we  shall  suppose  p  >  1 
and  that  A  and  r  are  such  that  the  roots  of  |  M  —  \  =0  are  all  different  ; 

this  excludes  the  case  already  considered  when  A  =  (     /[         )  .     Supposing 

\    0  —  7/ 

a  (1,  1)  correspondence  to  exist,  for  which  this  condition  is  satisfied,  if  in 
the  fundamental  equations  (i=l,  ...,p) 

z,c         -,  ,          x,a  ,     Tif  x,a 

vt    SMttl9l    +  ......  +Miipv1>    , 

we  introduce  other  integrals  of  the  first  kind,  say  Ff'",  ...,  F^'a,  where 


*  The  (1,  1)  correspondence  for  the  case  p  =  l  is  considered  in  an  elementary  way  in  §  394. 
The  reader  may  prefer  to  consult  that  Article  before  reading  the  general  investigation. 


650  PERIODICITY    OF   A    (1,    1)    CORRESPONDENCE.  [389 

then  we  can  put  the  fundamental  equations  into  the  form 


for  this  it  is  necessary  that  X;  should  be  a  root  of  the  equation  M  —  \  =  0, 
and  that  the  p  quantities  ajl}  ...,  citp  should  be  determined  from  the 
equations 

Ci,iM1>r+  ......  +  citpMptr  =  \iCitr,          (r=  1,  ...,£>); 

under  the  prescribed  conditions  the  determinant  of  the  matrix  c  will  be 
different  from  zero. 

Hence  as  X^  is  a  root  of  unity,  it  can  be  shewn,  when  p>  1,  that  every 
such  (1,1)  correspondence  is  periodic,  with  a  finite  period  ;  that  is,  if  the  place 
corresponding  to  x  be  zlt  the  place  corresponding  to  the  position  zl,  of  x, 
be  z2,  the  place  corresponding  to  the  position  #2,  of  x,  be  z3,  and  so 
on,  then  after  a  finite  number  of  stages  one  of  the  places  zl}  z2,  z3>... 
coincides  with  x.  In  order  to  prove  this,  suppose  that  all  the  roots  of  the 
equation  |  M  —  X  \  =  0  are  &-th  roots  of  unity  ;  then  denoting  the  place 
x  by  z0  and  the  place  a  by  c0,  the  equations  of  the  correspondence  may 
be  written 


these  give 
and  therefore 

r  7   Zk,Ck         j   Zoic<n    .  r  7   z*>  c*          7   zoip<n         /\ 

Ci^ldv,      -dvl     ]+  ......  +Ci,p[dvp      -dvp     ]  =  0; 

hence  on  the  dissected  Riemann  surface  we  have  equations  of  the  form 

vr*'  *  -  v?'  °  =  \r  +  X/Tr>  !  +  ......  +  \p'rr>  p>  (r  =  l,...,p), 

where  X1(  ...,  Xp'  are  integers.  Thus  either  zk  =  z0  and  ck  =  c0,  which  is  the 
result  we  wish  to  obtain,  or  else  there  is  a  rational  function  expressed  by 

f-fX,a       Ttx>a       o    -/\  /  *i<*  ,  ,  \  /  x>  a\ 

A.a-^.co-2^^^       +  ......  +  VV    >, 

which  is  of  the  second  order,  having  zk,  c0  as  zeros  and  z0,  ck  as  poles;  now 
a  surface  on  which  there  is  a  rational  function  of  the  second  order  is 
necessarily  hyperelliptic  (Chap.  V.  §  55)  —  but,  on  a  hyperelliptic  surface, 
for  which  p>\,  of  the  two  poles  of  such  a  function  either  determines 
the  other,  and  of  the  two  zeros  either  determines  the  other  ;  it  is  not 
possible  to  construct  such  a  function  whereof,  as  here,  one  pole  ck  is  fixed, 
and  the  other  arbitrary  and  variable  (§  52). 

Hence    we   must   have   zk  =  z0,   and    ck  =  c0)    which    proves    the    result 
enunciated. 

There  is  no  need  to  introduce  the  integrals  V  in  order  to  establish  this  result.  It 
is  known  (Cayley,  Coll.  Works,  Vol.  n.  p.  486)  that  if  Xl5  X2,  ...  be  the  roots  of  the  equation 
|j^_A|  =  0,  the  matrix  M  satisfies  the  equation  (M—  Xj)  (M—  X2)  ......  =  0;  when  the  roots 


390]  FORM   OF   THE    FUNDAMENTAL    ALGEBRAIC    EQUATION.  651 

Xj,  X.j,  ...  are  different  &-th  roots  of  unity  it  can  thence  be  inferred  that  the  matrix  M 
.satisfies  the  equation  Mk  =  \  •  then  from  the  successive  equations  dv*1'  c'  =  Mdv*0'  c°, 
dvz*'  et=Mdvfl'Cl,  etc.,  we  can  infer  dvZk'  °k=dvZl>'  c°,  and  hence  as  before  that  zk=z0)  ck=c0. 

A  proof  of  the  periodicity  of  the  (1,  1)  correspondence,  following  different  lines,  and 
not  assuming  that  the  roots  of  the  equation  \M—\\  =  Q  are  different,  is  given  by  Hurwitz, 
Math.  Annal.  xxxn.  (1888),  p.  295,  for  the  cases  when  p>l.  It  will  be  seen  below  that 
the  cases  p  =  0,  p  =  \  possess  characteristics  not  arising  for  higher  values  of  p  (§  394). 

390.  Assuming  the  periodicity  of  the  (1,  1)  correspondence,  we  can 
shew  that  all  Riemann  surfaces  upon  which  a  (1,  1)  correspondence  exists, 
can  be  associated  with  an  algebraic  equation  of  particular  form.  As  before 
let  k  be  the  index  of  the  periodicity,  and  let  w  =  eZnilk;  let  8,  T  be  any 
two  rational  functions  on  the  surface,  and  let  the  values  of  S  at  the 
successive  places  x,  zlt  z.2,  ...,  zh_lt  x  which  arise  by  the  correspondence  be 
denoted  by  8,  Sl}  ...,  $A_1}  S,  and  similarly  for  T  ;  then  the  values  of  the 
functions 


at  the  place  zr  are  respectively 

sr  =  S,.  +  w-]  Sr+1  +  ......  +  o)-t*-i»  Sr+M  =  a>rs,  and  t  ; 

hence  it  can  be  inferred  (cf.  Chap.  I.,  §  4)  that  there  exists  a  rational 
relation  connecting  sk  and  t.  Conversely  S  and  T  can  be  chosen  of  such 
generality  that  any  given  values  of  s  and  t  arise  only  at  one  place  of 
the  original  Riemann  surface.  Thus  the  surface  can  be  associated  with 
an  equation  of  the  form 

(«*,0  =  0, 
wherein  every  power  of  s  which  enters  is  a  multiple  of  k. 

Such  a  surface  is  clearly  capable  of  the  periodic  (1,  1)  transformation 
expressed  by  the  equations 

s'  =  MS,  t'  =  t. 


i* . 


The  following  further  remarkable  results  may  be  mentioned 
(a)     The  index  of  periodicity  k  cannot  be  greater  than  10  (p  -  1). 

(/3)     When  k  >  2p  -  2  the  Riemann  surface  can  be  associated  with  an 
equation  of  the  form 

«*  =  t*i  (t  -  1)*'  (t  -  c)*». 

(7)     When  k  >  4>p  -  4,  the  Riemann  surface  can  be  associated  with  an 
equation  of  the  form 

sk  =  t^(t-l)^. 

Herein  klt  Ar2,  k3  are  positive  integers  less  than  k. 

*  Hurwitz,  Math.  Annal.  xxxn.  (1888),  p.  294. 


652  UPPER    LIMIT   TO    NUMBER    OF    COINCIDENCES.  [391 

391.  We  can  deduce  from  §  389  that  in  the  case  of  a  (1,  1)  correspond 
ence  the  number  of  coincidences  is  not  greater  than  2p  -f  2.  In  the  case  of 
a  hyperelliptic  surface,  when  the  correspondence  is  that  in  which  conjugate 
places  —  of  the  canonical  surface  of  two  sheets  —  are  the  corresponding  pairs, 
the  coincidences  are  clearly  the  branch  places,  and  their  number  is  "2p  4-  2  ; 
for  all  other  (1,  1)  correspondences  on  a  hyperelliptic  surface,  the  number  of 
coincidences  cannot  be  greater  than  4. 

For,  when  the  surface  is  not  hyperelliptic,  let  g  denote  a  rational  function 
which  is  infinite  only  at  one  place  z0  of  the  surface,  to  an  order  p  +  1  ;  and 
let  g'  be  the  value  of  the  same  function  at  the  place  z1}  which  corresponds 
to  z0  ;  then  the  function  g'  —  g  is  of  order  2p  +  2,  being  infinite  to  order 
p  +  1  at  zQ  and  to  order  p  +  1  at  the  place  z^  to  which  z0  corresponds  ;  now 
every  coincidence  of  the  correspondence  is  clearly  a  zero  of  g'  —  g  ;  thus 
the  number  of  coincidences  is  not  greater  than  2p  +  2.  In  the  case  of  a 
hyperelliptic  surface 

2/2  =  \x>  1)20+1  > 

we  may  similarly  consider  the  function  x  —  x,  of  order  4  ;  —  unless  the 
correspondence  be  that  given  by  y  =  —  y,  x'  =  x,  for  which  x  —  x  is  identically 
zero.  We  thus  obtain  the  result  that  the  number  of  coincidences  cannot 
be  greater  than  4,  except  for  the  (1,  1)  correspondence  y'  =  —  y,  x'  =  x. 

It  can  be  shewn  for  the  most  general  possible  (r,  s)  correspondence,  associated  with  the 
equations 


by  equating  the  value  obtained  for  the  following  integral,  taken  round  the  period  loops, 


to  the  value  obtained  for  the  integral  taken  round  the  infinities  of  the  subject  of  integra 
tion,  that  the  number  of  coincidences  is 

C=r+s-(an  + +  OPP+&II  + +/3'pp)- 

Since  au  + +/3V-  ^s  ^ne  sum  of  the  roots  of  the  equation  |A  — X|  =  0,  it  follows  for  a 

(1,  1)  correspondence,  in  which  all  the  2p  roots  of    A  —  X|=0  are  roots  of  unity,  that 

C^-2p  +  2.     For  any  (r,  s)  correspondence  belonging  to  a  matrix  A=f     ^         j,  the  same 

formula  gives  C=r  +  s  +  2py,  as  already  found. 

We  have  remarked  (§  386,  Ex.  iv.)  for  the  case  of  a  (1, 1)  correspondence  associated  with 

a  matrix  A  of  the  form  |      l          ) ,  the  existence  of  a  rational  function  of  order  1  +y.     For 

\    (|   ~yj 

any  such  (1,  1)  correspondence,  if  p  be  >1,  y  must  be  equal  to  +1  in  order  that  the 
number  1  +  1-f  2py  of  coincidences  may  be  ;^>2jo  +  2.  Thus  such  a  correspondence  involves 
the  existence  of  a  rational  function  of  order  2,  and  involves  therefore  that  the  surface  be 
hyperelliptic.  This  is  also  obvious  from  the  fact  that  such  a  correspondence  is  associated 
with  equations  of  the  form 


393]  NUMBER   OF   (1,    1)   CORRESPONDENCES   IS   LIMITED.  653 

conversely,  for  y  =  1,  equations  of  this  form  are  known  to  hold  for  any  hyperelliptic  surface, 
associated  with  the  correspondence  of  the  conjugate  places  of  the  surface.  From  the 
considerations  here  given,  it  follows  for  p>\  that  for  a  (1,  1)  correspondence  the  number 
of  coincidences  can  in  no  case  be  >2/?  +  2. 

392.  In  conclusion  it  is  to  be  remarked  that  on  any  Riemann  surface 
for  which  p  >  1,  there  cannot  be  an  infinite  number  of  (1,  1)  correspondences. 
For  consider  the  places  of  the  Riemann  surface  that  can  be  the  poles  of 
rational  functions  of  order  <(p+l)  which  have  no  other  poles  (§§  28,  31, 
34 — 36,  Chap.  III.).     Denote    these   places   momentarily  as   (/-places.     As 
such  a  (1,  1)  correspondence  is  associated  with  a  linear  transformation  of 
integrals   of  the   first   kind,  which   does  not   affect   the   zeros   of  the  de 
terminant  A,  of  §  31,  it  follows  that  the  place  corresponding  to  a  ^-place 
must  also  be  a  <jr-place.     Now,  when  the  surface  is  not  hyperelliptic,  every 
#-place  cannot  be  a  coincidence  of  the  correspondence;   for  we  have  shewn 
(Chap.  III.,  §  36)  that  then  the  number   of  distinct   (/-places   is   greater 
than  2p  +  2;  and  we  have  shewn  in  this  chapter  (§  391)  that  the  number 
of  coincidences  in  a   (1,  1)   correspondence,  when  p>l,  can   in   no   case 
be  >  2p  +  2.     Therefore,  when    the    surface   is   not   hyperelliptic,   a   (1,  1) 
correspondence  must  give  rise  to  a  permutation  among  the  ^-places;  since 
the  number  of  such  permutations  is  finite,  the  number  of  (1,   1)  corre 
spondences  must  equally  be  finite.      But  the  result  is  equally  true  for  a 
hyperelliptic  surface;  for  we  have  shewn  (§  391)  that  for  such  a  surface  the 
number  of  coincidences  of  a  (1,  1)  correspondence  cannot  be  greater  than  4, 
except  in  the  case  of  a   particular   one   such   correspondence;    since   the 
number  of  distinct  ^-places  is  2p  +  2,  every  (1,  1)  correspondence  other  than 
this  particular  one  must  give  rise  to  a  permutation  of  these  ^-places.     As 
the  number  of  such  permutations  is  finite,   the  number  of  (1,  1)  corre 
spondences  must  equally  be  finite. 

It  is  proved  by  Hurwitz*  that  the  number  of  (1,  1)  correspondences, 
when  p  >  1,  cannot  be  greater  than  84  (p  -  I).  In  case  p  =  3,  a  surface  is 
known  to  exist  having  this  number  of  (1,  1)  correspond  en  cesf. 

393.  The    preceding    proof  §   (§    392)    is    retained    on    account    of   its 
ingenuity.     It  can  however  be  replaced  by  a  more  elementary  proof  j  by 
means  of  the  remark  that  a  (1,  1)  correspondence  upon  a  Riemann  surface 
can  be  represented  by  a  rational,  reversible  transformation  of  the  equation  of 
the  surface  into  itself.      Let  the  equation  of  the  surface  be  f(x,y)  =  Q; 
let  (z,  s)  be  the  place  corresponding  to  (x,  y) ;   then  z,  s  are  each  rational 
functions   of  x   and   y   such   that  f(z,  s)  =  0 ;    conversely   x,   y   are   each 

*  Math.  Annal.  XLI.  (1893),  p.  424. 

+  Klein,  Math.  Annal.  xiv.  (1879),  p.  428;  Modulfunctionen,  t.  i.,  1890,  p.  701. 

§  Hurwitz,  Math.  Annal.  XLI.  (1893),  p.  406. 

£  Weierstrass,  Math.  Werke,  Bd.  11.  (Berlin,  1895),  p.  241. 


654  SELF-TRANSFORMATION   OF  A   RIEMANN   SURFACE.  [393 

rational  functions  of  z,  s.  To  give  a  formal  demonstration  we  may 
proceed  as  follows  ;  supposing  the  number  of  sheets  of  the  Riemann  surface 
to  be  n,  let  z1}  ...,  zn  denote  the  places  corresponding  to  the  n  places 
#1°',  ,..,«£*  for  which  x  =  0,  and  let  zj  ,  ...,z'n  denote  the  n  places  corre 
sponding  to  the  places  d4  ,  ...,  ae^  for  which  x  is  infinite  ;  as  #  is  a  rational 
function  on  the  surface  we  have,  for  suitable  paths  of  integration  (cf.  Chap. 
VIII.  §  154) 

J0>      J«>  JO)      J«>  -  ,. 

v*i'x>   +  ......  +'«J"f   •   =0,  (i  =  l,  ...,_p); 

hence  from  the  equations 

z,  c         ir        a;.  <*    .  n  f          &•  a 

Vi    =  MitlVi    +  ......  +Miipvp   , 

we  have 


there  exists  therefore  (Chap.  VIII.,  §  158)  a  rational  function  having  the 
places  z-i,  ...,  zn  as  zeros,  and  the  places  zj,  .  ..,  zn'  as  poles  ;  regarding  this  as 
a  function  of  z,  s  and  denoting  it  by  (f>  (z,  s),  it  is  clear  therefore  that  x\$  (z,  s) 
is  a  constant,  which  may  be  taken  to  be  1.  Hence  x  =  (j>(z,  s),  etc. 

For  the  theorem  that  for  p>l  the  number  of  (1,  1)  correspondences  is  limited  the 
reader  may  consult,  Schwarz,  Crelle,  LXXXVII.  (1879),  p.  139,  or  Gesamm.  Math.  Abhand., 
Bd.  II.  (Berlin,  1890),  p.  285  ;  Hettner,  Gotting.  Nachr.  (1880),  p.  386  ;  Noether,  Math. 
Annal.,  XX.  (1882),  p.  59  ;  Poincare,  after  Klein,  Acta  Math.,  vn.  (1885)  ;  Klein,  Ueber 
Riemann'  s  Theorie  u.  s.  w.  (Leipzig,  1882),  p.  70  etc.  ;  Noether,  Math.  Annal.,  xxi.  (1883), 
p.  138  ;  Weierstrass,  Math.  Werke,  Bd.  n.  (Berlin,  1895),  p.  241  ;  Hurwitz,  Math.  Annal., 
XLI.  (1893),  p.  406. 

394.  In  regard  to  the  (1,  1)  correspondence  for  the  case  p  =  l,  some  remarks  may  be 
made.  The  case  p  =  0  needs  no  consideration  here  ;  any  (1,1)  correspondence  is  expressible 
by  an  equation  of  the  form 


thus  there  exists  a  triply  infinite  number  of  (1,  1)  correspondences. 

In  case  p  =  l,  if  there  be  a  (1,  1)  correspondence,  whereby  the  variable  place  x 
corresponds  to  #',  and  a,  a!  be  simultaneous  positions  of  x  and  x',  it  is  immediately 
shewn,  if  vF>  a  denote  the  normal  integral  of  the  first  kind,  that  there  exists  an  equation  of 
the  form 

tfV,  a'  =  ptf,  a? 

wherein  /*  is  a  constant  independent  both  of  a  and  x.     From  this  equation,  by  supposing  x 
to  describe  the  period  loops,  we  deduce  eqxiations  of  the  form 


where  a,  a',  /3,  &  are  integers.     By  supposing  x'  to  describe  the  period  loops  we  deduce 
equations  of  the  form 

'),  (ii), 


where  y,  y',  8,  8'  are  integers.     The  expression  of  these  integers  in  terms  of  a,  a',  ft  ft'  is 


394]         ELEMENTARY  TREATMENT  OF  THE  ELLIPTIC  CASE.          655 

known  from  the  general  considerations  of  this  chapter  ;  it  is  however  interesting  to 
consider  the  equations  independently.  From  the  equations  (ii)  we  deduce 

8'  -  ry'  =  n  (y8f  -  y'8),      8  -  ry  =  -  r/x  (yS'  -  y'8)  ; 

if  now  y8'-y'8  =  0,  either  y  and  y  are  zero,  which  is  inconsistent  with  1  =p  (y  +  ry'),  or  else 
T  is  a  rational  fraction  ;  it  is  known  that  in  that  case  the  deficiency  of  the  surface  is  not  1 
but  0  ;  we  may  therefore  exclude  that  case  ;  if  y8'  -  y'8  be  not  zero,  we  have 


hence,  unless  T  be  a  rational  fraction,  we  have 

*'  '  & 

°  -y    _,        y     _ff       -o    _0 

yV-y'6       '       y8'-y'8~    '      y8'-y'8~P'     y8'-y'8~P> 
and  therefore 

l  =  (a/3'-a'/3)(y8'-y'8); 

thus  af?  —  a'P  =  y8'  -y'8  =  +  1  or  -  1  ;  let  t  denote  their  common  value  ;  then  we  deduce 

fc/  f  f  £\t  &  n 

a  =  ea,     y  =  —  a  e,     y  =  pt,     o=  —  pe  ; 
by  these  the  equations  (ii)  lead  to 


that  is,  to  the  equations  (i). 

Further,  from  the  equations  (i)  we  deduce  in  turn 

so  that  /i  is  a  root  of  the  equation 

-/*     ft      =0; 

a       /3'  —  u 

now  if  a  be  zero,  the  first  of  equations  (i)  gives  p  =  a,  and,  therefore,  as  r  cannot  be 
the  rational  fraction  0/(a-00,  the  second  of  equations  (i)  gives  a=p',  0=0  ;  the  equations 

give  /*2=f,  or,  since  /u,  =a,  is  an  integer,  they  require  e=  +1  and  /i=+l  or/i=-l;  the 
equations  corresponding  to  /*  =  + 1  and  p  =  —  I  are 

these  do  belong  to  existing  correspondences — of  the  kind  considered  in  §§  386,  387,  the 
coefficient  y  being  ±\*.  But  they  differ  from  the  (1,1)  correspondences  which  are  possible 
whenp>l,  in  each  containing  an  arbitrary  parameter  ; 

if  next,  a'  be  not  zero,  the  equation  for  T  gives 

2ra'  =  -  (a  -  00  ±  \i(a  +  pj-4f, 
so  that,  as  T  cannot  be  real,  we  must  have 

(«  +  0')2-4f«), 

*  For  instance,  on  a  plane  cubic  curve,  the  former  equation  is  that  in  which  to  a  point  of 
argument  u  we  make  correspond  the  point  of  argument  u  +  constant ;  the  line  joining  these  two 
points  envelopes  a  curve  of  the  sixth  class,  which  in  case  the  difference  of  arguments  be  a 
half-period  becomes  the  Cayleyan,  doubled  ;  while  the  latter  equation  is  that  in  which  we 
make  correspond  the  two  variable  intersections  of  a  variable  straight  line  passing  through  a 
fixed  point  of  the  cubic. 


656  THE    ELLIPTIC   CASE.  [394 

and  this  shews  that,  in  this  case  also,  e  =  l.  Hence  the  equations  are  reduced  to  precisely 
the  same  form  as  those  already  considered  for  the  special  transformation  of  theta  functions 
(§  383) ;  and  the  result  is  that  the  only  special  surfaces,  having  p  =  l,  for  which  there  exists 
a  (1,  1)  correspondence  are  those  which  may  be  associated  with  one  of  the  two  equations 


the  former  has  the  obvious  (1,  1)  correspondence  given  by  x'  =  —A;  y'  =  iy ;  the  latter  has 

the  obvious  correspondence  given  by  x1  =  e  3  x,  /i/=y  ;  the  index  of  periodicity  is  2  in  the 
former  case  and  3  in  the  latter  case. 

Ex.     Consider  the  (1,  2)  correspondence  on  a  surface  for  which  p  =  \  in  a  similar  way. 
For  the  equation 

7/2  =  8^-15^  +  7 

shew  that  a  (1,  2)  correspondence  is  given  (cf.  Ex.  ii.  §  383)  by 

8  (.*•-!)'    *    *    4       (x-\f 


395] 


CHAPTER    XXII. 

DEGENERATE  ABELIAN  INTEGRALS. 

395.  THE  present  chapter  contains  references  to  parts  of  the  existing 
literature  dealing  with  an  interesting  application  of  the  theory  of  trans 
formation  of  theta  functions. 

It  was  remarked  by  Jacobi*  for  the  case  p  =  2,  that  if  the  fundamental 
algebraic  equation  be  of  the  form 

2/2  =  x  (x  -  1)  (x  —  K)  (x  —  \)  (x  —  K\), 

an  hyperelliptic  integral  of  the  first  kind  is  reducible  to  elliptic  integrals  ; 
in  fact,  putting  |  =  x  +  K\/X,  we  immediately  verify  that 

_  (x  ±  V/cX)  dx  _  __  df  _ 

-«X)      </(£+  2  V/t 


396.     Suppose  more  generally  that  for  any  value  of  p  there  exists  an 
integral  of  the  first  kind 

U  =  X^^  4-  ......  -f  \pUp, 

wherein  ul}...,up  denote  the  normal  integrals  of  the  first  kind,  which  is 
reducible  to  the  form 


_ 

R(%)  being  a  cubic  polynomial  in  f,  such  that  £  and  (f)  are  rational 
functions  on  the  original  Riemann  surface;  then  there  exist  p  pairs  of 
equations  of  the  form 


wherein  at-,  &;,  a/,  &/  are  integers  ;  we  may  suppose  H'  to  be  chosen  so  that 
the  *2p  integers 

a1}  ...,  ap,  a/,  ...,  ap' 

have  no  common  factor  and  so  that 

aM  +  a2b2'  +  ......  +  ctpbp  —  a/tj  -  a/62  —  ......  —ap'bp  =  r, 

*  Crelle,  vm.  (1832),  p.  41G. 
B.  42 


658  TRANSCENDENTAL  CONDITIONS  [396 

where  r  is  a  positive  integer;   we  assume  that  r  is  not  zero.      Eliminating 
the  quantities  X1;  ...,  \p,  and  putting  &>  =  H'/Il,  we  have  the  p  equations 


if  therefore  the  matrix  of  integers,  A  =  f   ,  \L,  ]  ,  of  2p  rows  and  columns, 

\(*      ^j  / 

wherein  the  first  column  consists  of  the  integers  aly  ...,  ap'  in  order,  and  the 
(p  +  l)th  column  consists  of  the  integers  bl}  ...,  bpr  in  order,  be  determined 
to  satisfy  the  conditions  for  a  transformation  of  order  r, 

oa'  =  a  a,     J30'  =  ff&,     a/3'  -  a/3  =  r, 

(§  420,  Appendix  II.),  then  it  immediately  follows  from  the  equation,  for 
the  transformed  period  matrix  T',  namely 


that  r'u  =  to,  r'12  =  0,  ...,  r'y,  =  0  ;  to  see  this  it  is  sufficient  to  compare  the 
elements  of  the  first  columns  of  the  two  matrices  /3  +  r/3',  (a  +  rot)r'.  In 
other  words,  when  there  exists  such  a  degenerate  integral  of  the  first  kind  as 
here  supposed,  it  is  possible*,  by  a  transformation  of  order  r,  to  arrive  at 
periods  r  for  which  the  theta  function  ^(w,  T'  \  q)  is  a  product  of  an  elliptic 
theta  function,  in  the  variable  wlt  and  a  theta  function  of  (p—  1)  variables, 
w2,  ...,wp. 

397.     It  can  however  be  shewn  that  in  the  same  case  it  is  possible  by  a 
linear  transformation  to  arrive  at  a  period  matrix  r"  for  which 

r"13=0,  T*14  =  0,  ...,r%  =  0, 

while  r"i2,  =  1/r,  is  a  rational  number.  We  shall  suppose  -f*  two  rows  oc,  x  . 
each  of  p  integers,  to  be  determined  satisfying  the  equations 

ax  —  ax  =  1,     bx  —  b'x  =  0, 

such  that  the  2p  elements  of  rx  —  b,  rx'  —  b'  have  unity  as  their  greatest 
common  factor,  a  denoting  the  row  a1}  ...,  ap,  etc.,  and  suppose  (§  420)  a 
matrix  of  integers,  of  2p  rows  and  columns, 


x,  .. 


»  **    —      /       /     11 
6J      \a,  rx  -b,  ... 


to  be  determined,  satisfying  the  conditions  for  a  linear  transformation, 

^y=ry'ry)        SB'  =8'  8,       j8'  —  j8  =  l, 

wherein  the  first  column  consists  of  the  elements  of  a  and  a',  the  second 
column  consists  of  the  elements  of  rx  —  b  and  rx  —b',  and  the  (jp  +  l)th 

*  This  theorem  is  due  to  Weierstrass,  see  Konigsberger,  Crelle,  LXVII.  (1867),  p.  73  ;  Kowal- 
evski,  Acta  Math.  iv.  (1884),  p.  395.  See  also  Abel,  (Euvres,  t.  i.  (1881),  p.  519. 

t  The  proof  that  this  is  possible  is  given  in  Appendix  II.,  §  419.  It  may  be  necessary,  before 
hand,  to  make  a  linear  transformation  of  the  periods  ft,  ft'. 


398]  FOR   THE    EXISTENCE   OF    A    DEGENERATE   INTEGRAL.  659 

column  consists  of  the  elements  of  as  and  x  ;  the  conditions  for  a  linear  trans 
formation,  so  far  as  they  affect  these  three  columns  only,  are 

a  (rx'  _  &')  _  a'  (rx  -  b)  =  0,  ax  -a'x=l,  (rx  -b)x  -  (rx  -b')x  =  Q, 

and  these  are  satisfied  in  virtue  of  the  equation  ab'  —  a'b  =  r.  Then  the 
equation  for  the  transformed  period  matrix  r",  namely 

(7  +  Ty')  T"  =  8  +  T&, 
leads  to  T"S,  i  =  0,  . . . ,  T"PI  t  =  0  if  only  the  p  equations 

[7<,i  +  (T7  ki]  A,  +  [7,-|8  +  (T7')i,J  T7/a>1  =  Bitl  +  (rS'Xi,  (i  =  1,  ..-,  P), 

which  are  obtained  by  equating  corresponding  elements  of  the  first  columns 
of  the  matrices  S  +  rS',  (7  +  T7')T",  are  satisfied;  these  p  equations  are 
included  in  the  single  equation 

T"J,  i  [a  +  TO,']  +  T\  i[ras-b  +  r  (rx  -  b')]  =  x  +  rx, 

and  are  satisfied*  by  T"V  =  ta/r,  T"2)1  =  l/r ;  for  we  have,  as  the  fundamental 
condition,  the  equation 

a)  (a  +  TO!)  =  b  +  rb'. 

398.     It  follows  therefore  in  case  p=  2  that  the  matrix  r"  has  the  form 

"u,  1M . 

/r,  r"J  ' 

hence  it  immediately  follows  that  beside  the  integral  of  the  first  kind  already 
considered,  which  is  expressible  as  an  elliptic  integral,  there  is  another 
having  the  same  property.  In  virtue  of  the  equations  here  obtained  the  first 
integral  having  this  property  can  be  represented,  after  division  by  fi,  in  the 
form 

U  =  (V  -rr\  XK 

where  u  denotes  the  row  of  2  integrals  uly  u2 ;  consider  now  the  integral 
V  =  [rf  -  a'  -  rr"2>2  (rx  -  b')]  u, 

where  t'  is  a  row  of  two  elements,  these  being  the  constituents  of  the  first 
column  of  the  matrix  8';  the  periods  of  Vat  the  first  set  of  period  loops  are 
given  by  the  row  of  quantities 

rtf  —  a  —  ?'T"2)2  (rx'  —  b'), 


*  See  Kowalevski,  Acta  Math.  iv.  (1884),  p.  400  ;  Picard,  Bulletin  de  la  Soc.  Math,  de  France, 
t.  xi.  (1882—3),  p.  25,  and  Conipt.  Itendtis,  xcn.  xciu.  (1881);  PoincarS,  Bulletin  de  la  Soc.  Math, 
de  France,  t.  xn.  (1883—4),  p.  124  ;  Poincare,  American  Journal,  vol.  vin.  (1886),  p.  289. 

42—2 


660  CONNEXION   WITH   THEORY   OF   COMPLEX   MULTIPLICATION.  [398 

and  are  linear  functions  of  the  two  quantities  1,  rr"2i2;  the  periods  of  Fat 
the  second  set  of  period  loops  are  given  by 

[r  (rt'  -  a')l  -  rr"2,2  [T  (rx'  -  V)]it  (»  =  1,  2)  ; 

now  the  equation  (7  +  TJ)  r"  =  8  +  r8'  gives 

(7  +  T7)f,i  r\2  +  (y  +  ry\,  r"2,2  =  (8  +  rS\2,  (i  =  1,  2), 

and  hence  we  have 

T*I,S  [a  +  ra]  +  r"2>2  [rx-b  +  r  (rx  -  b')]  =  t  +  rt', 

where  t  is  the  row  formed  by  the  constituents  of  the  first  column  of  the 
matrix  B;  therefore,  as  T//1)2=l/r,  the  periods  of  V  at  the  second  set  of 
period  loops  are  expressible  in  the  form 

-  (rt  -  a)i  +  rr\t  2  (rx  -  b){  ,  (i  =  1  ,  2), 

and  these  are  also  linear  functions  of  the  two  quantities  1,  rr"2j2.  Hence  it 
may  be  inferred  that  the  integral  V  is  reducible  to  an  elliptic  integral. 

399.  It  has  been  shewn  in  the  last  chapter  that  for  special  values  of  the 
periods  T  there  exist  transformations  of  the  theta  functions  into  theta  func 
tions  for  which  the  transformed  periods  are  equal  to  the  original  periods.  It 
can  be  shewn*  that  for  the  special  case  now  under  consideration  such  a 
transformation  holds.  Suppose  that  a  theta  function  S-,  with  period  r,  is 
transformed,  as  described  above,  into  a  theta  function  <£,  with  period  T,  for 
which  r'li2=  0  =  ...  =  T'I>P,  by  a  transformation  associated  with  the  matrix 

A  =  (  ,  ni  }  5  suppose  further  that  there  exists,  associated  with  a  matrix 
H  —  (  „  ,  ,  )  ,  a  transformation  whereby  the  theta  function  <f>  is  transformed 

\x  nJ 

into  another  theta  function  with  the  same  period  T'  ;  then  it  is  easy  to  prove 
that  there  exists  a  corresponding  transformation  of  the  theta  function  ^ 
whereby  it  becomes  changed  into  a  theta  function  with  the  same  period  T, 
namely  the  transformation  is  that  associated  with  the  matrix 


,f  g'J      U/3'AxVA-a       « 
to  prove  this  it  is  only  necessary  to  shew  that  the  equations 

(X  +  r'A/)  r'  =  fj,  +  r'/jf,     (a  +  rot) T'  =  {3  +  r/3' 
give  the  equation 


Wiltheiss,  Math.  Annal.  xxvi.  (1886),  p.  127. 


401]     ALGEBRAIC  CONDITIONS  FOR  A  DEGENERATE  INTEGRAL.         661 

Hence  it  follows  that  in  order  to  determine  a  transformation  of  the  function 
^  which  leaves  the  period  r  unaltered,  it  is  sufficient  to  determine  a  trans 
formation  of  the  function  <f>  which  leaves  the  period  r  unaltered  ;  this 
determination  is  facilitated  by  the  special  values  of  T\,Z,  ...,  T\,P\  and  in 
fact  we  immediately  verify  that  the  equation  (A,  +  T'\')  T'  =  //-  +  T'JA  is  satisfied 
by  taking  X'  =  p  =  0  and  by  taking  each  of  X  and  p'  to  be  the  matrix  in 
which  every  element  is  zero  except  the  elements  in  the  diagonal,  each  of 
these  elements  being  1  except  the  first,  which  is  —  1. 

400.  Thus  for  the  case  p  =  2,  supposing  r  =  2,  the  original  function  ^  is 
transformed  into  a  theta  function  with  unaltered  period  T,  by  means  of  the 
transformation  of  order  4  associated  with  the  matrix, 


where  m  denotes  the  matrix  (  j  ;  the  matrix  V  is  equal  to  2A"1,  and  it 

is  easy  to  see  that  this  transformation  of  order  4  is  equivalent  to  a  multipli 
cation,  with  multiplier  2,  together  with  a  linear  transformation  associated 
with  the  matrix 


We  have  therefore  the  result  ;  when,  in  case  p  —  2,  there  exists  a  transforma 
tion  of  the  second  order  whereby  the  periods  r  are  changed  into  periods  T'  for 
which  T'IF  2  =  0,  then  there  exists  a  linear  transformation  whereby  the  periods 
T  are  changed  into  the  same  periods  r,  or  what  we  have  called  in  the  last 
chapter  a  complex  multiplication. 

401.  The  transcendental  results  thus  obtained  enable  us  to  specify  the 
algebraic  conditions  for  the  existence  of  an  integral  of  the  first  kind  which  is 
reducible  to  an  elliptic  integral. 

Thus  for  instance  when  p  =  2,  to  determine  all  the  cases  in  which  an 
integral  of  the  first  kind  can  be  reduced  to  an  elliptic  integral  by  means  of  a 

transformation  of  the  second  order,  A  =  (,  Q,  }  ,  it  is  sufficient  to  consider 

\a   p  ) 

the  conditions  that  the  transformed  even  theta  function  ^\w\  T'  ^L      ]) 

may  vanish  for  zero  values  of  w  ;  for  when  T',i2  =  0  this  function  breaks  up  into 
the  product  of  two  odd  elliptic  theta  functions.  By  means  of  the  formulae* 
for  transformation  of  the  second  order,  it  can  be  shewn*f-  that  this  condition 
leads  to  the  equation 


*  Chap.  XX.  §  364. 

t  Konigsberger,  Crelle,  LXVII.  (1867),  p.  77. 


662  ALGEBRAIC    CONDITIONS.  [401 

and  by  means  of  the  relations  expressing  the  constants  of  the  fundamental 
algebraic  equation  in  terms  of  the  zero  values  of  the  even  theta  functions*  it 
can  be  shewn  that  this  is  equivalent  to  the  condition  that  the  fundamental 
algebraic  equation  may  be  taken  to  be  of  the  form 

2/2  =  x  (x  —  1)  (x  —  K)  (x  —  \)(x  —  K\), 

so  that  the  case  obtained  by  Jacobi  is  the  only  one  possible  for  transformations 
of  the  second  order. 

In  the  same  case  of  p  =  2,  r  =  2,  the  same  result  follows  more  easily  from 
the  existence,  deduced  above,  of  a  complex  multiplication  belonging  to  a 
transformation  of  the  first  order.  For  it  follows  from  this  fact  that  the 
algebraic  equation  can  be  taken  in  a  form  in  which  it  can  be  transformed 
into  itself  by  a  transformation  in  which  the  independent  variable  is  trans 
formed  by  an  equation  of  the  form 


_ 

~ 


and  this  leadsf  to  the  form,  for  the  fundamental  algebraical  equation, 

S2  =  (02  _  ft2)  ^a  _  fc)  ^  _  ca^ 

which  is  immediately  identified  with  the  form  above  by  putting 

X  =  \/KX(Z  + 

the  quantities  a,  b,  c  being  respectively 


Similarly  for  p  =  3,  when  the  surface  is  not  hyperelliptic,  it  can  be  shewn  j 
from  the  relations  connecting  the  theta  functions  when  a  theta  function  is  the 
product  of  an  elliptic  theta  function  and  a  theta  function  of  two  variables, 
that  the  only  cases  in  which  an  integral  of  the  first  kind  can  be  reduced  to 
an  elliptic  integral  are  those  in  which  the  fundamental  algebraic  equation 
can  be  taken  to  be  of  the  form 

Jx(Ax+By)  +  \/y(Cx  +  Dy)  +  Vl  +  Fas  +  Gy  =  0. 

The  Riemann  surface  associated  with  this  equation  possesses  a  (1,  1)  corre 
spondence  given  by  the  equations 


*  Cf.  Ex.  v.  p.  341.  By  means  of  the  substitution  x  =  cl  +  (a1-c1)l-,  the  branch  places  can  be 
taken  at  £  =  0,  1,  K,  X,  /x,  wherein,  if  cx,  a1(  c2,  a2,  c  be  real  and  in  ascending  order,  0,  1,  K,  X,  ft 
are  in  ascending  order  of  magnitude.  For  complete  formulae,  when  the  theta  functions  are 
regarded  as  primary,  and  the  algebraic  equation  as  derived,  see  Eosenhain,  Mem.  p.  divers 
Savants,  xi.  (1851),  p.  416  ff. 

t  Wiltheiss,  Math.  Annal.  xxvi.  (1886),  p.  134. 

£  Kowalevski,  Acta  Math.  iv.  (1884),  p.  403. 


4-03]  REFERENCES.  663 

402.  But  the  problem  of  determining  the  algebraic  equations  for  which  an  associated 
integral  of  the  first  kind  reduces  to  an  elliptic  integral  may  be  considered  algebraically,  by 
beginning  with  an  elliptic  integral  and   transforming  it  into  an  Abelian  integral.     The 
reader  may   consult   Richelot,   Crelle,  xvi.   (1837);   Malet,   Crelle,  LXXVI.  (1873),  p.  97; 
Brioschi,  Compt.  Rendus,  LXXXV.  (1877),  p.  708;  Goursat,  Bulletin  de  la  Soc.  Math,  de 
France,  t.  xni.  (1885),  p.  143,  and  Compt.  Rendus,  c.  (1885),  p.  622  ;  Burnside,  Proc.  Lond. 
Math.  Soc.  vol.  xxm.  (1892),  p.  173. 

403.  The  paper  of  Konigsberger  already  referred  to  (Crelle,  LXVII.)  deals  with  the  case 
of  a  transformation  of  the  second  order,  for  p  =  2.     For  the  case  of  a  transformation  of  the 
third  order,  when  p  =  2,  consult,   beside  the  papers   of  Goursat   (loc.    cit.    §    402),   also 
Hermite,  Ann.  de  la  Soc.  Scient.  de  Bnixelles,  1876,  and  Burkhardt,  Math.  Annal.  xxxvi. 
(1890),  p.  410.     For  the  case  p  =  2,  and  a  transformation  of  the  fourth  order,  see  Bolza, 
Ueber  die  Reduction  hyperelliptischer  Integrale  u.  s.  w.,  Getting.   Dissertation    (Berlin, 
Schade,  1885),  or  Sitzungsber.  der  Naturforsch.  Ges.  zu  Freiburg  (1885).     The  paper  of 
Kowalevski  (Ada  Math,  iv.)  deals  with  the  case  of  a  transformation  of  the  second  order  for 
p  =  3.      See  further  the  references  given  in  this  chapter,  and  Poincare,  Compt.  Rendus, 
t.  xcix.  (1884),  p.  853  ;  Biermann,  Sitzungsber.  der  Wiener  Akad.  Bd.  LXXXVII.  (ii.  Abth.) 
(1883),  p.  983. 


[404 


APPENDIX   I. 

ON  ALGEBRAIC  CURVES  IN  SPACE. 

404.     GIVEN  an  algebraic  curve  ((7)  in  space,  let  a  point  0  be  found,  not  on  the  curve, 
such  that  the  number  of  chords  of  the  curve  that  pass  through  0  is  finite  ;  let  the  curve 
be  projected  from  0  on  to  any  arbitrary  plane,  into  the  plane  curve  (/),  and  referred  to 
homogeneous  coordinates  £,  r],  T  in  that  plane,  whose  triangle  of  reference  has  such  a 
position  that  the  curve  does  not  pass  through  the  angular  point  TJ,  and  has  no  multiple 
points  on  the  line  r=0;  let  the  curve  (C)  be  referred  to  homogeneous  coordinates  £,  77,  f,  T 
of  which  the  vertex  f  of  the  tetrahedron  of  reference  is  at  0.     Putting  X  =  £/T,  y  =  r)/r, 
Z  =  C/T,  it  is  sufficient  to  think  of  x,  y,  z  as  Cartesian  coordinates,  the  point  0  being  at 
infinity.     Thus  the  plane  curve  (/)  is  such  that  y  is  not  infinite  for  any  finite  value  of  x, 
and  its  equation  is  of  the  form  f(y,  x)=ym  +  A1ym~1  +  ......  +Am=Q,  where  A^..,,Am 

are  integral  polynomials  in  x  ;  the  curve  (C)  is  then  of  order  ra;  we  define  its  deficiency 
to  be  the  deficiency  of  (/);  to  any  point  (x,  y)  of  (/)  corresponds  in  general  only  one 
point  (x,  y,  z)  of  (C),  and,  on  the  curve  (C),  z  is  not  infinite  for  any  finite  values  of  x,  y. 


Now  let  /'  (y)  =  9/(y,  x)fiy,  let  <£  be  an  integral  polynomial  in  x  and  y,  so  chosen 
that  at  every  finite  point  of  (/)  at  which  f'(y)  =  0,  say  at  x=a,  y  =  b,  the  ratio 
(x  -  a)  (fr/f  (y)  vanishes  to  the  first  order  at  least  ;  let  a  =  n  (x-  a)  contain  a  simple  factor 
corresponding  to  every  finite  value  of  x  for  which  /'(y)  =  0;  let  y±,  ...,ym  be  the  values 
of  y  which,  on  the  curve  (/),  belong  to  a  general  value  of  x,  so  that  to  each  pair  (x,  y>) 
there  belongs,  on  the  curve  (C),  only  one  value  of  z;  considering  the  summation 

%  (c-yQ  ......  (c-ym)r  ^  1 

i=i         c-Vi  L/'  (#)>="*' 

where  c  is  an  arbitrary  quantity,  we  immediately  prove,  as  in  §  89,  Chap.  VI.,  that  it 
has  a  value  of  the  form 

a  (cm~l  ttx  +  cm~2  U2  +  ......  +  wj, 

where  «1,...,«m  are  integral  polynomials  in  x\  putting  yi  for  c,  after  division  by  a,  we 
therefore  infer  that  z  can  be  represented  in  the  form 


where  0,  ^  are  integral  polynomials  in  x  and  y,  whereof  </>  is  arbitrary,  save  for  the 
conditions  for  the  fractions  (x  -  a]  <£//'  (y).  This  is  Cayley's  monoidal  expression  of  a 
curve  in  space  with  the  adjunction  of  the  theorem,  described  by  Cay  ley  as  the  capital 
theorem  of  Halphen,  relating  to  the  arbitrariness  of  0  (Cayley,  Collect.  Works,  Vol.  v.  1892, 
p.  614). 


404]  ALGEBRAIC   CURVES   IN    SPACE.  665 

It  appears  therefore  that  a  curve  in  space  may  be  regarded  as  arising  as  an 
interpretation  of  the  relations  connecting  three  rational  functions  on  a  Riemann  surface ; 
and,  within  a  finite  neighbourhood  of  any  point  of  the  curve  in  space,  the  coordinates 
of  the  points  of  the  curve  may  be  given  by  series  of  integral  powers  of  a  single  quantity  t, 
this  being  the  quantity  we  have  called  the  infinitesimal  for  a  Riemann  surface;  to 
represent  the  whole  curve  only  a  finite  number  of  different  infinitesimals  is  necessary. 
More  generally  the  representation  by  means  of  automorphic  functions  holds  equally  well 
for  curves  in  space.  And  the  theory  of  Abelian  integrals  can  be  developed  for  a  curve 
in  space  precisely  as  for  a  plane  curve,  or  can  be  deduced  from  the  latter  case;  the 
identity  of  the  deficiency  for  the  curve  in  space  and  the  plane  curve  may  be  regarded  as 
a  corollary.  Also  we  can  deduce  the  theorem  that,  of  the  intersections  with  a  curve  in 
space  of  a  variable  surface,  not  all  can  be  arbitrarily  assigned,  the  number  of  those  whose 
positions  are  determined  by  the  others  being,  for  a  surface  of  sufficiently  high  order,  equal 
to  the  deficiency  of  the  curve. 

Ex.  If  through  p  - 1  of  the  generators  of  a  quadric  surface,  of  the  same  system,  a 
surface  of  order  p  +  l  be  drawn,  the  remaining  curve  of  intersection  is  representable  by 
two  equations  of  the  form 

y   =  W   1  /2P  +  2  >       ZU1 =  M2 ' 

where  (x,  l)2P  +  2  is  an  integral  polynomial  in  x  of  order  2/?  +  2,  and  wn  w2  are  respectively 
linear  and  quadric  polynomials  in  x  and  y. 

For  the  development  of  the  theory  consult,  especially,  Noether,  Abh.  der  Akad.  zit 
Berlin  vom  Jahre  1882,  pp.  1  to  120  ;  Halphen,  Journ.  £cole  Polyt.,  Cah.  LII.  (1882), 
pp.  1—200;  Valentiner,  Acta  Math.,  t.  n.  (1883),  pp.  136—230.  See  also,  Schubert, 
Math.  Annal.  xxvi.  (1885);  Castelnuovo,  Rendiconti  delta  R.  Accad.  dei  Lincei,  1889; 
Hilbert,  Math.  Annal.,  xxxvr.  (1890). 


[405 


APPENDIX   II. 
ON  MATRICES*. 

405.  A  SET  of  n  quantities 

(#j ,  . . . ,  Xn) 

is  often  denoted  by  a  single  letter  a,  which  is  then  called  a  row  letter,  or  a  column  letter. 
By  the  sum  (or  difference)  of  two  such  rows,  of  the  same  number  of  elements,  is  then 
meant  the  row  whose  elements  are  the  sums  (or  differences)  of  the  corresponding  elements 
of  the  constituent  rows.  If  m  be  a  single  quantity,  the  row  letter  mx  denotes  the  row 
whose  elements  are  mx^  ...,  mxn.  If  x,  y  be  rows,  each  of  n  quantities,  the  symbol  xy 
denotes  the  quantity  xlyl  -f- +  xnyn. 

406.  The  set  of  n  equations  denoted  by 

#<  =  0i,i!i  + +  ai,p£j»  (i=l, ,n) 

where  n  may  be  greater  or  less  than  p,  can  be  represented  in  the  form  a;=a£,  where  a 
denotes  a  rectangular  block  of  np  quantities,  consisting  of  n  rows  each  of  p  quantities, 
the  r-th  quantity  of  the  i-ih  row  being  ai>r.  Such  a  block  of  quantities  is  called  a 
matrix  ',  we  call  ait  r  the  (i,  r)th  element  of  the  matrix.  The  sum  (or  difference)  of  two 
matrices,  of  the  same  number  of  rows  and  columns,  is  the  matrix  formed  by  adding  (or 
subtracting)  the  corresponding  elements  of  the  component  matrices.  Two  matrices  are 
equal  only  when  all  their  elements  are  equal ;  a  matrix  vanishes  only  when  all  its 
elements  are  zero.  If  £x ,  . . ,  £p  be  expressible  by  m  quantities  X1,...)  Xm  by  the  equations 

f.  =  &r,i^l  + +1>r,mXm*  (r=l,  2> ,P\ 

so  that  £  =  bX,  where  b  is  a  matrix  of  p  rows  and  m  columns,  then  we  have 

•^  =  ct,i^i  + +ci>mXm,  (i=l, ,  n), 

or  x=cX,  where 

/i=l, ,  n\ 

c;,s=«i,  101,8  + +ai,pbp>s,  I  I, 

\°  —  i) >  m/ 

*  The  literature  of  the  theory  of  matrices,  or,  under  a  slightly  different  aspect,  the  theory  of 
bilinear  forms,  is  very  wide.  The  following  references  may  be  given  :  Cayley,  Phil.  Trans.  1858, 
or  Collected  Works,  vol.  n.  (1889),  p.  475  ;  Cayley,  Crelle,  L.  (1855) ;  Hermite,  Crelle,  XLVII. 
(1854) ;  Christoffel,  Crelle,  LXIII.  (1864)  and  LXVIII.  (1868) ;  Kronecker,  Crelle,  LXVUI.  (1868)  or 
Gesam.  Werke,  Bd.  i.  (1895),  p.  143 ;  Schlafli,  Crelle,  LXV.  (1866) ;  Hermite,  Crelle,  LXXVIII. 
(1874) ;  Kosanes,  Crelle,  LXXX.  (1875) ;  Bachmann,  Crelle,  LXXVI.  (1873) ;  Kronecker,  Berl. 
Monatsber.,  1874;  Stickelberger,  Crelle,  LXXXVI.  (1879);  Frobenius,  Crelle,  LXXXIV.  (1878), 
LXXXVI.  (1879),  LXXXVIII.  (1880) ;  H.  J.  S.  Smith,  Phil.  Trans.,  CLI.  (1861),  also,  Proc.  Lond.  Math. 
Soc.,  1873,  pp.  236,  241 ;  Laguerre,  J.  d.  Vec.  Poly.,t.  xxv.,  cah.  XLII.  (1867),  p.  215  ;  Stickelberger, 
Progr.  poly.  Schule,  Zurich,  1877 ;  Weierstrass,  Berl.  Monats.  1858,  1868 ;  Brioschi,  Liouville, 
xix.  (1854) ;  Jordan,  Compt.  Rendus,  1871,  p.  787,  and  Liouville,  1874,  p.  35  ;  Darboux,  Liouville, 
1874,  p.  347. 


408]  INTRODUCTORY    ACCOUNT   OF    MATRICES.  667 

cit  g  being  the  (i,  .<)th  element  of  a  matrix  of  n  rows  and  m  columns  ;  it  arises  from  the 
equations  x=a£,  £  =  &Jf,  whereof  the  result  may  be  written  x=abX  ;  hence  we  may 
formulate  the  rule  :  A  matrix  a  may  be  multiplied  into  another  matrix  b  provided  the 
number  of  columns  of  a  be  the  same  as  the  number  of  rows  of  b  ;  the  (i,  s)th  element  of  the 
resulting  matrix  is  the  result  of  multiplying,  in  accordance  with  the  rule  given  above,  the 
\-th  row  of  a  by  the  &-th  column  of  b.  Thus,  for  multiplication,  matrices  are  not  generally 
commutative,  but,  as  is  easy  to  see,  they  are  associative. 

The  matrix  whose  (i,  «)th  element  is  cg>i,  where  cSii  is  the  (s,  ?')th  element  of  any 
matrix  c  of  n  rows  and  m  columns,  is  called  the  transposed  matrix  of  c,  and  may  be 
denoted  by  c  ;  it  has  m  rows  and  n  columns,  and,  briefly,  is  obtained  by  interchanging  the 
rows  and  columns  of  c.  The  matrix  which  is  the  transposed  of  a  product  of  matrices  is 
obtained  by  taking  the  factor  matrices  in  the  reverse  order,  each  transposed  ;  for  example, 
if  a,  6,  c  be  matrices, 

abc=cba. 

407.  The  matrices  which  most  commonly  occur  are  square  matrices,  having  an  equal 
number  of  rows  and  columns.  With  such  a  matrix  is  associated  a  determinant,  whose 
elements  are  the  elements  of  the  matrix.  When  the  determinant  of  a  matrix,  a,  of  p  rows 
and  columns,  does  not  vanish,  the  p  linear  equations  expressed  by  x  =  a%  enable  us  to 
represent  the  quantities  £t,  ...,  £p  in  terms  of  a,\,  ...,  xv  ;  the  result  is  written  £  =  a~lx,  and 
a"1  is  called  the  inverse  matrix  of  a  ;  the  (i,  r)th  element  of  a~l  is  the  minor  of  ar<  f  in 
the  determinant  of  the  matrix  a,  divided  by  this  determinant  itself.  The  inverse  of  a 
product  of  square  matrices  is  obtained  by  taking  the  inverses  of  the  factor  matrices  in 
reverse  order  ;  for  example,  if  a,  b,  c  be  square  matrices,  of  the  same  number  of  rows  and 
columns,  for  each  of  which  the  determinant  is  not  zero,  we  have 


The  inverse  of  the  transposed  of  a  matrix  is  the  transposed  of  its  inverse  ;  thus 


The  determinant  of  a  matrix  a  being  represented  by  |  a  \  ,  we  clearly  have  |  ah  \  =  \  a  \  \b\. 

408.  Finally,  the  following  results  are  of  frequent  application  in  this  volume  :  (i)  If  a 
be  a  matrix  of  n  rows  and  p  columns,  and  £  a  row  of  p  quantities,  the  symbol  a£  denotes 
a  row  of  ?i  quantities  ;  if  TJ  be  a  row  of  n  quantities,  the  product  of  these  two  rows,  or 
(^X7?)*  is  denoted  by  agij.  When  n=p  this  must  be  distinguished  from  the  matrix 
which  would  be  denoted  by  a  .  fr  —  this  latter  never  occurs.  We  have  then 


and  this  is  called  a  bilinear  form  ;  we  also  clearly  have  the  noticeable  equation 


(ii)  if  b  be  a  matrix  of  n  rows  and  q  columns,  the  product  of  the  two  rows  «£,  brj,  wherein 
is  now  a  row  of  q  quantities,  is  given  by  either  (ba)  £17  or  (ab)  qg,  so  that  we  have 


The  result  of  multiplying  any  square  matrix,  of  p  rows  and  columns,  by  the  matrix  Et 
of  p  rows  and  columns,  wherein  all  the  elements  are  zero  except  the  diagonal  elements, 
which  are  each  unity,  is  to  leave  the  multiplied  matrix  unaltered.  For  this  reason  the 
matrix  E  is  often  denoted  simply  by  1,  and  called  the  matrix  unity  of  p  rows  and 
columns. 


668 


SYSTEMS   OF    UNITIES   FORMED    WITH    MATRICES. 


[409 


409.  Ex.  i.  If  a  bilinear  form  axy,  wherein  x,  y  are  rows  of  p  quantities,  and  a  is  a 
square  matrix  of  p  rows  and  columns,  be  transformed  into  itself  by  the  linear  substitution 
x=  R£,  y  =  *S'»7,  where  R,  S  are  matrices  of  p  rows  and  columns,  then  aR£.  iSr)  =  a^rj  ;  hence 

SaR  =  a. 

Ex.  ii.  If  h  be  an  arbitrary  matrix  of  p  rows  and  columns,  such  that  the  determinants 
of  the  matrices  a  +  h  do  not  vanish,  and  the  determinant  of  the  matrix  a  do  not  vanish, 

prove  that 

(a+h}a~l  (a-h)=a-ha~1  h  =  (a  —  h)a~1  (a+h)  ; 

hence  shew  that  if 

R  =  a~1(a-h)(a  +  h')-1a,     S=a  (a-h)~l  (a  +  h)a~\ 

the  substitutions  x  =  R%,  y  —  Sr]  transform  axy  into  a^rj. 

For  a  substitution  in  which  R  =  S  see  Cayley,  Collected  Works,  vol.  n.  p.  505.  Cf.  also 
Taber,  Amer.  Journ.,  vol.  xvi.  (1894)  and  Proc.  Lond.  Math.  Soc.,  vol.  xxvi.  (1895). 

Ex.  iii.     The  matrices,  of  two  rows  and  columns, 


P     (l     °\  7 

Mo   I/I       " 

give  E2  =  jE,  J2=  —  E  ;  and  the  determinant  of  the  matrix 


vanishes,  for  real  values  of  x,  y,  only  when  x  —  0,  y  =  0. 
Ex.  iv.     The  matrices,  of  four  rows  and  columns, 

/I  0  0  0\  /     0  1  0 

e  =  l 


° 


0       010 
0       001 
-1       000 
0-100' 


(oo  o  r 
00-10 
01  00 
-10  00' 


00107  \       000   -II 

10  0  0  V  \     0  0  1       0 

give  j*=jf=j3*=-e,  jJ3=  -J3j2=ji,  J3Ji=-JiJ3=J2, 

Hence  these  matrices  obey  the  laws  of  the  fundamental  unities  of  the  quaternion 
analysis.     Further  the  determinant  of  the  matrix 


which  is  equal  to  (x^+^+x^+a;^,  vanishes,  for  real  values  of  x,  x^  x2,  x3,  only  when 
each  of  a?,  tclt  #2,  xz  is  zero.     (Frobenius,  Crelle,  LXXXIV.  (1878),  p.  62.) 

410.     In  the  course  of  this  volume  we  are  often  concerned  with  matrices  of  2p  rows 
and  2p  columns.     Such  a  matrix  may  be  represented  in  the  form 


/*  = 


wherein  a,  b,  c,  d  are  square  matrices  with  p  rows  and  columns ;  if  //  be  another  such 
matrix  given  by 

b' 


411]  REDUCTION   OF   GENERAL   ABELIAN   MATRIX.  669 

the  (i,  r)th  element  of  the  product  /*'/*,  when  i  and  r  are  both  less  than  p  + 1  is 

a'ft  j  <Z1)  r  -f- +  Q>  i ,  p  dp,  r  4"  b'i,  \  C\,  r  + -f-  ^'i,  p  £/>,  r  > 

and  this  is  the  sum  of  the  (i,  r)ih  elements  of  the  matrices  a'a,  b'c  ;  similarly  when  i  and  r 
are  not  both  less  than  p  + 1  ;  hence  we  may  write 

fa'  6'\  fa  6\  _  fa! a  +  b'c ,  a'b  +  6'cA 
\c'  d'J  \c  d)  ~\c'a+d'c,  c'b  +  d'd)' 

the  law  of  formation  for  the  product  matrix  being  the  same  as  if  a,  b,  c,  d,  a',  b',  c',  d'  were 
single  quantities. 

Ex.     Denoting  the  matrices  ( n  1  ) ,  ( ,       A  ]  respectively  by  1  and  j,  the  matrices  of 


0  - 


, 


Ex.  iv.  can  be  denoted  by 

/I  0\  f-jO\  (     0  IN  /     0 

e=(oi)>  *~(  oy>  *K-io)'  *-(-,- 


411.  We  proceed  now  to  prove  the  proposition*  assumed  in  §  333,  Chap.  XVIII. 
Retaining  the  definitions  of  the  matrices  Ak,  B,  C,  D  there  given,  and  denoting 
Ak~l,  B~l,  C~l,  D'1  respectively  by  ak,  b,  c,  d,  we  find 


and 


=  Ak,  so  that  Ak2  =  l, 


b  =  (      01         ),    c  =  (  1       1         ),    d=(  1       01       ) 


1       0 

1       0 

1     10 

1       0 

1       0 

1       0 

1       0 

1       0 

1       0 

-1       0 

0       1 

0       1 

0       1 

0       1 

0       1 

0       1 

0       1 

0       1 

0       1 

0       1 

0       1 

so  that  b,  c,  d  differ  respectively  from  B,  C,  D  only  in  the  change  of  the  sign  of  the 
elements  which  are  not  in  the  diagonal.  It  is  easy  moreover  to  verify  such  facts  as  the 
following 


which  are  equivalent  respectively  with 

64=1,  (cb)3=l,  a2d=da2,  bakbak  =  akbakb, 

but  such  results  are  immediately  obvious  from  the  interpretations  of  the  matrices  ak,  b,  c,  d 
which  are  now  to  be  given. 

Let  A  denote  any  matrix  of  2p  rows  and  columns,  and  let  the  four  products 

A'';  .      -V'.     AC,     _V/ 

*  For  a  shorter  proof  of  an  equivalent  result  the  reader  may  consult  C.  Jordan,  Traite  des 
Substitutions  (Paris,  1870),  p.  174.  The  theorem  was  first  given  by  Kronecker,  "  Ueber  bilineare 
Formen,"  Monatsber.  Berl.  Akad.  1866,  Crelle,  LXVIII.  or  in  Werke  (Leipzig,  1895),  Bd.  i.  p.  160  ; 
the  proof  here  given  follows  the  lines  there  indicated. 


670  REDUCTION   OF   GENERAL  [411 

be  formed  ;  the  resulting  matrices  will  differ  from  A  in  respects  which  are  specified  in  the 
following  statements  : 

(i)  ak  interchanges  the  first  and  Mh  columns  (of  A),  and,  at  the  same  time,  the 
(p  +  l)th  and  (p  +  k)th  columns  (l<  k<  p  +  l).  For  the  sake  of  uniformity  we  introduce 
also  al5  =1. 

(ii)  b  interchanges  the  first  and  (^>  +  l)th  columns,  at  the  same  time  changing  the 
signs  of  the  elements  of  the  new  first  column. 

(iii)     c  adds  the  first  column  to  the  (jt)  +  l)th. 

(iv)  d  adds  the  first  and  second  columns  respectively  to  the  (p  +  2)ih  and 
the  Qo  +  l)th. 

Hence  we  have  these  results  :  if  the  matrices  denoted  by  the  following  symbols  be 
placed  at  the  right  side  of  any  matrix  A,  of  2p  rows  and  columns,  so  that  the  matrix 
A  acts  upon  them,  the  results  mentioned  will  accrue  :  — 

Ik=akb2ak,  changes  the  signs  of  the  k-th  and  (p  +  k)th  columns  (of  A), 

t}c  =  akbalc,  interchanges  the  k-th  and  (p  +  k}th  columns  (of  A),  giving  the  new  k-th 

column  an  opposite  sign  to  that  it  had  before  its  change  of  place, 
t'k  =  akb5ak,  interchanges   the   k-th   and   (p  +  k)th   columns,  giving  the   new  (p  +  k)th 

column  a  changed  sign. 

mk=akb2cb*ak,  adds  the  k-th  column  to  the  (p  +  k)th. 

m'ic=akb3cbcb3ak=aicb'2c~1b2ak,  subtracts  the  k-th  column  from  the  (p  +  k)th. 
nk  =  akb2cbcak  =  akbc~1b3ak,  adds  the  (p  +  k}th  column  to  the  k-th. 
n'k=akb3cbak,  subtracts  the  (p  +  k)th  column  from  the  k-th. 
gr>a=ara2aaa2b3dba2asa2ar,  subtracts  the  s-th  column  from  the  r-th,  and,  at  the  same 

time,  adds  the  (p  +  r}th  column  to  the  (p  +  s)th. 
g'r>  s=ara2aga2&Q?&3a2aga2a,.,  adds  the  s-th  column  to  the  r-th,  and,  at  the  same  time, 

subtracts  the  (p  +  r)th  from  the  (p  +  s)th  column. 

fr,s  —  ts9r,/at  adds  the  (p  +  r)th  and  (p  +  s)th  columns  respectively  to  the  s-th  and 
r-th  columns. 


f'r,a  —  tig'r,/»i  subtracts  the  (^  +  ?-)th  and  (p  +  s)th  columns  respectively  from  the  s-th 
and  r-th  columns. 

To  this  list  we  add  the  matrix  ak,  whose  effect  has  been  described,  and  the  matrix  b'2, 
which  changes  the  sign  both  of  the  first  and  of  the  (p  +  l)th  columns;  then  it  is  to  be 
shewn  that  a  product,  P,  of  positive  integral  powers  of  these  matrices,  can  be  chosen  such 
that,  if  A  be  any  Abelian  matrix  of  integers,  given  by 

where  aj8=/3a,  a'£'  =  /3'a',  a|3'-£a'  =  l, 

the  product  AP  is  the  matrix  unity  —  of  which  every  element  is  zero  except  those  in  the 
diagonal,  each  of  which  is  1.  Hence  it  will  follow  that  fj.  =  P~1  ;  namely  that  every  such 
Abelian  matrix  can  be  written  as  a  product  of  positive  integral  powers  of  the  matrices 
Ak,  B,  C,  D.  Up  to  a  certain  point  of  the  proof  we  shall  suppose  the  matrix  A  to  be 
that  for  a  transformation  of  any  order,  r. 

In  the  matrices  at,  ar,  aa,  each  of  k,  r,  s  is  to  be  <jo  +  l;  and  in  general  each  of 
k,  r,  s  is  >1  ;  but  for  the  sake  of  uniformity  it  is  convenient,  as  already  stated,  to 
introduce  a  matrix  ax  =  l  ;  then  each  of  k,  r,  s  may  have  any  positive  value  less  than  p  +  l. 


412] 


ABELIAN   MATRIX. 


671 


412.  Of  the  matrix  A  we  consider  first  the  first  row,  and  of  this  row  we  begin  with 
the  jo-th  and  2p-th  elements,  a,jp,  0lip ;  if  the  numerically  greater  of  these  elements  be 
not  a  positive  integer,  use  the  matrix  lp  to  make  it  positive*— form,  that  is,  the  product 
Alp.  Then,  let  y  be  the  greater,  and  8  the  less  of  these  two  elements ;  if  8  is  positive, 
use  the  matrix  m'p  or  the  matrix  n'p,  as  many  times  as  possible,  to  subtract  from  y  the 
greatest  possible  multiplef  of  8  (i.e.  if  v  be  the  matrix  upon  which  we  are  operating,  =A 
or  =&lp,  form  one  of  the  products  v(m'p)r,  v  (n'p)8) ;  if  8  is  negative,  use  mp  or  np  to  add 
to  y  the  greatest  possible  multiple  of  8  ;  so  that,  in  either  case,  the  remainder,  y', 
from  y,  is  numerically  less  than  8  and  positive.  Now,  by  the  matrix  lpt  take  the  element 
8  to  be  positivej  ;  then  again,  by  application  of  mp  or  np  or  m'p  or  n'p  replace  8  by  a 
positive  quantity  numerically  less  than  y'.  Let  this  process  alternately  acting  on  the 
remainder  from  y  and  8,  be  continued  until  either  y  or  8  is  replaced  by  zero.  Then  use 
the  matrix  tp  or  l!v  to  put  this  zero  element  at  the  2p-th  place  of  the  first  row  of  the 
matrix,  A',  which,  after  all  these  changes,  replaces  A. 

Let  a  similar  process  of  alternate  reduction  and  transposition  be  applied  to  A',  until 
the  (1,  2/>-l)th  element  of  the  resulting  matrix  is  zero.  And  so  on.  Eventually  we 
arrive,  in  continuing  the  operation,  at  a  matrix  instead  of  A,  in  which  there  is  a  zero  in 
each  of  the  places  formerly  occupied  by  /31(1, ,  0lt  p. 

Now  apply  the  processes  given  by  b2,  lp,  gltp,  gp>l,  and  eventually  ap,  if  necessary,  to 
reduce  the  (1,  p)th  element  to  zero.  Then  the  processes  b2,  lp,1,  glt  p_1,  gp_ltl,  ap_1,  as 
far  as  necessary,  to  reduce  the  (1,  p-l)th  element  to  zero;  and  so  on,  till  the  places, 
which  in  the  original  matrix  were  occupied  by  a1>2,  ...,  alip,  are  all  filled  by  zeros. 

Consider  now  the  second  row  of  the  modified  matrix.  Beginning  with  the  (2,  p)th  and 
(2,  2/?)th  elements,  use  the  specified  processes  to  replace  the  latter  by  a  zero.  Next 
replace,  similarly,  the  (2,  2p-l)th  element  by  a  zero;  and  so  on,  finally  replacing  the 
(2,  jo  +  2)th  element  by  a  zero.  The  necessary  processes  will  not  affect  the  fact  that  all 
the  elements  in  the  first  row,  except  the  (1,  l)th  element,  are  zero.  Next  reduce  the 
elements  occupying  the  (2, p)th,  ...,  (2,  3)th  places  to  zero. 

Proceeding  thus  we  eventually  have  (i)  the  (r,  s+p)th  element  zero,  for  every  r<p  and 
every  s<p,  in  which  s>r,  (ii)  the  (r,  s)th  element  zero,  for  every  r<p  and  every  s<p,  in 
which  s>r.  In  other  words  the  matrix  has  a  form  which  may  be  represented,  taking  p  =  4, 
by  the  matrix  p, 

p  =  (  an    0      0       0       0       0       0      0       ); 


«21 

«22     ° 

0         021 

0 

0 

0 

«31 

Q32     a33 

0        031 

032 

0 

0 

«41 

a42     a43 

a44     041 

042 

043 

0 

«'ll 

"12  «'i3 

«14   #11 

#12 

#13 

#14 

«'« 

a'42  a'43 

a/44    0'41 

0*42 

0'43 

0« 

since  now  the  original  matrix  is  an  Abelian  matrix,  and  each  of  the  matrices  ak   b  c  d  is 
an  Abelian  matrix,  it  follows  (Chap.  XVIII.,  §  324)  that  a0=0d  ;  if  the  original  matrix  be 

*  The  changes  of  sign  of  the  other  elements  of  the  same  column  which  enter  therewith  do  not 
concern  us. 

t  The  simultaneous  subtractions,  effected  by  the  matrix  m'p,  of  the  other  elements  of  the 
column,  do  not  concern  us.  Similar  remarks  apply  to  following  cases. 

t  It  is  not  absolutely  necessary  to  use  the  matrix  /„  in  this  or  in  the  former  case ;  but  it  con- 
duces  to  clearness. 


672  REDUCTION   OF   GENERAL  [412 

for  greater  generality  supposed  primarily  to  be  associated  with  a  transformation  of  order  r, 
the  value  r=l  being  introduced  later,  the  determinant  of  the  matrix  is  ±rf  (§  324,  Ex.  i.) 
and  is  not  zero  ;  hence  comparing  in  turn  the  1st,  2nd,  ...,  rows  of  the  matrices  a£  and  £d 
we  deduce  that  in  the  matrix  p  the  elements  /821,  /331,  /332,  ...  of  the  matrix  /3  which  are  on 
the  left  side  of  the  diagonal  are  also  zero  ;  thus,  in  p,  every  element  of  the  matrix  £  is  zero. 
Apply  now  to  the  matrix  p  the  relation 

a/3'-/3d'  =  r, 

which  in  this  case  reduces  to  aft  =  r.  Then  it  is  immediately  found  that  the  elements  of 
the  matrix  ft  which  are  on  the  left  side  of  the  diagonal  are  also  zero — and  also  that 

an  #11  = =  appftpp=r. 

The  resulting  form  of  the  matrix  p  may  then  be  shortly  represented  by 


If  now  to  the  matrix  a-  we  apply  the  processes  given  by  the  matrices  glt  2  or  g1^  2  and  £2, 
we  may  suppose  a21  numerically  less  than  a^,  and  a22  positive  ;  if  then  we  apply  the 
processes  given  by  the  matrices  glt  3  or  g'l>  s  and  13,  and  the  processes  given  by  the  matrices 
#2, 3  or  #'2,  s  and  ^3?  we  may  suppose  a31,  a32  numerically  less  than  a33,  and  may  suppose  a33 
to  be  positive.  Proceeding  thus  we  may  eventually  suppose  all  the  elements  of  any  row  of 
the  matrix  a  which  are  to  the  left  of  its  diagonal  to  be  less  than  the  diagonal  elements  of 
that  row— and  may  suppose  that  all  the  elements  of  the  diagonal  of  the  matrix  a  are 
positive  ;  this  involves  that  the  diagonal  elements  of  ft  are  positive,  and  in  particular 
when  r  is  a  prime  number  involves  that  these  elements  are  each  1  or  r. 

Further  we  may  reduce  the  elements  of  the  matrix  a  which  are  in  the  diagonal  of 
a',  and  those  which  are  to  the  left  of  this  diagonal,  by  means  of  the  diagonal  elements  of 
the  matrix  ft.  We  begin  with  the  elements  of  the  last  row  of  a  ;  by  means  of  the 
processes  given  by  the  matrices  np  or  rip  we  may  suppose  a'pp  to  be  numerically  less  than 
#PP  5  by  means  of  the  processes  given  by  the  matrices  fp,p-l  or  f'p,p-i  we  may  suppose 
°'P,P-I  to  be  numerically  less  than  ftp,p;  in  general  by  means  of  the  processes  given  by 
fp,s  or  f'p,s  we  may  suppose  a'p>g  to  be  numerically  less  than  ftp,p.  Similarly  by  the 
processes  given  by  »p_1  or  n'p_1  we  may  suppose  a'p_1>p_1  numerically  less  than  ftp-llp-i, 
and  by  the  processes  fp _ lt s  or/'p_1)g,  where  s<p-l,  we  may  suppose  a'p_ljg  numerically 
less  than  ftp^lip_1.  The  general  result  is  that  in  every  row  of  the  matrix  a'  we  may 
suppose  the  diagonal  element,  and  the  elements  to  the  left  of  the  diagonal,  to  be  all 
numerically  less  than  the  diagonal  element  of  the  same  row  of  the  matrix  ft. 

413.  If  then  we  take  the  case  when  r  =  l  we  have  the  result  that  it  is  possible  to  form 
a  product  Q  of  the  p  +  2  matrices  ak,  b,  c,  d,  such  that  the  product  AQ  has  a  form  which 
may  be  represented,  taking  p  =  3,  by 

A0  =  (  100000), 
01      0      00      0 
00      1      00      0 
0  a'12  a'13  1  ft12  ftl3 
0  0      a'23  0  1       #23 
00      0      00      1 

wherein  all  the  elements  of  each  of  the  matrices  a  and  ft  to  the  left  of  the  diagonals  are 
zero,  and  all  the  elements  of  the  matrix  a  both  in  the  diagonal,  and  to  the  left  of  the 


or  ~ 
I  TTNIVERSJ1 


415] 


ABELIAN    MATRIX. 


673 


diagonal,  are  zero.  Applying  then  the  condition  a/3'  =  l,  we  find  that  the  elements  of  the 
matrix  /3'  to  the  right  of  its  diagonal  are  also  zero,  so  that  /3'  =  a=  1.  Then  finally,  applying 
the  condition  a  ft' =  ft  a,  equivalent  to  a'  =  a',  we  have  a'  =  0.  Thus  the  reduced  matrix  is 
the  matrix  unity  of  2p  rows  and  columns,  and  A,  =O-1,  is  expressed  as  a  product  of 
positive  integral  powers  of  the  p+Z  matrices  Ak,  B,  C,  D,  as  desired.  Since  the  determinant 
of  each  of  the  matrices  Ak,  B,  C,  D  is  +1,  the  determinant  of  the  linear  matrix  A  is  also 
+  1. 

414.  In  the  particular  case  p  =  \  the  only  matrices  of  the  p  +  2  matrices  Ak,  B,  C,  D 
which  are  not  nugatory  are  the  two  matrices  B  and  C ;  we  denote  these  here  by  U  and  V 
and  put  further 

u=U~l  —  (  \,   v=V~l  =  (        ),   vl  =  uvu3vu3,  w  =  uvu3,  w 

then  we  immediately  verify  the  facts  denoted  by  the  following  table 


M 

& 

UA 

V 

*t 

10 

»i 

(-*£) 

C-fe-9) 

(«?,  -£) 

(l,i?+£) 

Cfef-D 

fc-%.t) 

(5  +  7,  >?) 

of  which,  for  example,  the  first  entry  means  that  if  A  =  (  a,  ^,  )  be  any  matrix  of  2  rows 

\«  P/ 

and  columns,  and  we  form  the  product  Aw,  then  the  columns  £,  9  of  the  matrix  A  are 
interchanged,  and  at  the  same  time  the  sign  of  the  new  first  column  is  changed  ;  we  have 
in  fact 

«  /3W    01X/-/3   « 


hence  it  is  immediately  shewn,  as  in  the  more  general  case,  that  every  matrix  A  =  (  a,     ,}  , 

\a  PY 

for  which  the  integers  a,  /3,  a',  /3'  satisfy  the  relation  a£'-a'p"  =  l,  can  be  expressed  as  a 
product  of  positive  integral  powers  of  the  two  matrices 


415.  Combining  the  final  result  for  the  decomposition  of  a  linear  Abelian  matrix  with 
the  results  obtained  for  any  Abelian  matrix  of  order  r  we  arrive  at  the  following  statement, 
whereof  the  parts  other  than  the  one  which  has  been  formally  proved  may  be  deduced  from 

~,  )  be  any  Abelian  matrix  of  order  r  ; 
/ 


that  one,  or  established  independently  :  let  A  = 


then  it  is  possible  to  find  a  linear  matrix  Q  expressible  as  a  product  of  positive  integral 
powers  of  the  (jo  +  2)  matrices  Ak,  B,  C,  D,  which  will  enable  us  to  write  A  =  A;Q,  where  At 
is  an  Abelian  matrix  of  order  r  having  any  one,  arbitrarily  chosen,  of  the  four  forms  repre- 
sentable  by 


A 
A'= 


fc 


and  it  is  also  possible  to  choose  the  linear  matrix  Q  to  put  A  into  the  form  A  =  QAt,  where 
A<  is  also  any  one,  arbitrarily  chosen,  of  these  same  four  forms.  It  follows  that  the  deter 
minant  of  the  matrix  A  is  +r".  In  virtue  of  the  equations  a«/3'«  =  r(t  =  l,  ...,p~),  which 
hold  for  any  one  of  the  matrices  A1}  A2,  A3,  A4,  and  the  inequalities  which  may  also  be 
supposed  to  hold  among  the  other  elements,  as  exemplified,  §  412,  for  the  case  of  A^  it  is  easy 
to  find  the  number  of  different  existing  reduced  matrices  of  any  one  of  these  forms.  For 
instance  when  p  =  2,  the  number  when  r  is  a  prime  number  is  l+r  +  r^  +  r5 ;  for  p  =  3,  and  r 

B.  43 


674  LEMMAS   IN   REGARD   TO   GENERAL  [415 


a  prime  number,  it  is  1  +r  +  r*  +  2r3  +  ri+r5  +  r6  ;  for  details  the  reader  may  consult  Hermite, 
Compt.  Rendus,  t.  XL.  (1855),  p.  253,  Wiltheiss,  Crelle,  xcvi.  (1884),  pp.  21,  22,  and  the 
book  of  Krause,  Die  Transformation  der  Hyperelliptischen  Functionen  (Leipzig,  1886), 
which  deal  with  the  case  p  =  2  ;  for  the  case£>  =  3,  see  Weber,  Annali  di  Mat.  Ser.  2",  t.  ix. 

(1878),  p.  139,  where  also  the  reduction  to  the  form  A  =  Q  (r     \  Q',  in  which  Q,  Q'  are 

linear  matrices,  is  considered.  Of.  also  Gauss,  Disq.  Arith.,  §  213  ;  Eisenstein,  Crelle,  xxviu. 
(1844),  p.  327;  Hermite,  Crelle,  XL.,  p.  264,  XLI.  (1851),  p.  192;  Smith,  Phil.  Trans.  CLI. 
(1861),  Arts.  13,  14. 

416.     Considering  (cf.  §  372)  any  reduction,  of  the  form 

A 


where  (  p,  °j  is  a  linear  matrix,  we  prove  that  however  this  reduction  be  effected,  (i)  the 

determinant  of  the  matrix  B'  is  the  same,  save  for  sign,  (ii)  if  p  be  a  row  of  p  positive 
integers    each    less  than   r  (including    zero),   the    rows  determined   by  the    condition, 

-  -B'/i  —  integral,  are  the  same.     For  any  other  reduction  of  this  kind,  say  A=Q'A'0,  must 

be  such  that 

,_p    <r\  /      q'-q\  _p    q\      A  B 

~ 


where  (  %  ^  J  is  a  linear  matrix  ;  the  condition  that  the  matrix  a'  of  the  matrix  A'0  should 

vanish,  namely  p'A  =  0,  requires  (since  |4|  1^1=7*  and  therefore  \A\,  the  determinant  of 
A,  is  not  zero)  that  p'  =  0  ;  thus  the  reduction  A  =  Q'A'0  can  be  written 
(a    p\  =  /pq',    -pq  +  <rp\       fpA  ,  pB  +  qB'\ 
\ft.-ftj       \p'q',    -p'q  +  v'p)  '   \0    ,       q'B'     )' 

Now  pq1  =  1  ;  therefore  \q'\=±l  ;  thus  \q'B'\=  ±\B'\,  which  proves  the  first  result.    Also, 

if  fj.  be  a  row  of  integers  such  that  -  B'p.  is  a  row  of  integers,  =m  say,  then  -  q'B'p,  =q'm, 
is  also  a  row  of  integers  ;  while  if  -q'B'p  be  a  row  of  integers,  =n  say,  then  -p 


which  is  equal  to  -B'p,  is  equal  to  pn,  and  is  also  a  row  of  integers  ;  since  q'B'  is  the 

matrix  which,  for  the  reduction  A  =  Q'A'0,  occupies  the  same  place  as  that  occupied,  for  the 
reduction  A  =  QA0,  by  the  matrix  B',  the  second  result  is  also  proved. 

417.  Considering  any  rectangular  matrix  whose  constituents  are  integers,  if  all  the 
determinants  of  (£  +  1)  rows  and  columns  formed  from  this  matrix  are  zero,  but  not  all 
determinants  of  I  rows  and  columns,  the  matrix  is  said  to  be  of  rank  I.    The  following 
theorem  is  often  of  use,  and  is  referred  to  §  397,  Chap.  XXII.  ;  In  order  that  a  system  of 
simultaneous  not-homogeneous  linear  equations,  with  integer  coefficients,  should  be  capable 
of  being  satisfied  by  integer  values  of  the  variables,  it  is  necessary  and  sufficient  that  the 
rank  I  of,  and  the  greatest  common  divisor  of  all  determinants  of  order  I  which  can  be 
formed  from,  the  matrix  of  the  coefficients  of  the  variables  in  these  equations,  should  be 
unaltered  when  to  this  matrix  is  added  the  column  formed  by  the  constant  terms  in  these 
equations.     For  the  proof  the  reader  may  be  referred  to  H.  J.  S.  Smith,  Phil.  Trans.  CLI. 
(1861),  Art.  11,  and  to  Frobenius,  Crelle,  LXXXVI.  (1879),  pp.  171—2. 

418.  Consider  a  matrix  of  n+l  columns  and  n+1  or  more  rows,  whose  constituents 
are  integers,  of  which  the  general  row  is  denoted  by 

^f  "i  ......  ^'t'j  'tj  ^i  5 


419]  MATRICES   OF   INTEGERS.  675 

let  A  be  the  greatest  common  divisor  of  the  determinants  formed  from  this  matrix  with 
n  +  1  rows  and  columns;  let  A'  be  the  greatest  common  divisor  of  the  determinants 
formed  from  this  matrix  with  n  rows  and  columns  ;  then,  since  every  determinant  of  the 
(n  +  l)th  order  may  be  written  as  a  linear  aggregate  of  determinants  of  the  n-th  order, 
the  quotient  A/  A'  is  integral,  =  M,  say.  Then  the  n  +  l  or  more  simultaneous  linear 
congruences 

Ui  =  aix+biy+  ......  +&ie+lit  +  eju=Q    (mod.  M) 


have  just  A  incongruent  sets  of  solutions,  and  have  a  solution  whose  constituents  have  unity  as 
their  highest  common  divisor.  Frobenius,  Crelle,  LXXXVI.  (1879),  p.  193. 

Also,  if  in  the  m  linear  forms  (m<  =  or  >n  +  l) 

Ui=aix+biy  +  ......  +kiz  +  lit  +  eiut  (i=l,  ...,m), 

the  greatest  common  divisor  of  the  m(n  +  l)  coefficients  be  unity,  it  is  possible  to  determine 
integer  values  of  x,y,  ...,t,  u,  such  that  the  m  forms  have  unity  as  their  greatest  common 
divisor;  in  particular,  when  n=l,  if  the  2m  numbers  at,  bt  have  unity  as  their  greatest 
common  divisor,  and  the  fyn(m-l)  determinants  aibj-ajbi  be  not  all  zero,  it  is  possible  to 
find  an  integer  x  so  that  the  m  forms  atx+bi  have  unity  as  their  greatest  common  divisor. 
Frobenius,  loo.  cit.,  p.  156. 

419.  The  theorem  of  §  418  includes  the  theorem  of  §  357,  p.  589  ;  it  also  includes  the 
simple  result  stated  §  383,  p.  637,  note.  It  also  justifies  the  assumption  made  in  §  397, 
that  the  periods  Q,  Q'  may  be  taken  so  that  the  simultaneous  equations  aotf  -a'x=\, 
bxf-b'x=Q  can  be  solved  in  integers  in  such  a  way  that  the  2p  elements  rx-b,  rod  -b' 
have  unity  as  their  greatest  common  divisor;  assuming  that  r  is  not  zero  so  that  the 
p  (2p-  1)  determinants  a^j-afc,  ai6/-a/6i,  a^'-a-b-  are  not  all  zero,  and  that  Q'  has 
been  taken  so  that  the  2p  integers  av,  ...,  ap,  a/,  ...,  ap'  have  no  common  divisor  other 
than  unity,  the  necessary  and  sufficient  condition  for  the  solution  of  the  equations 
ax'  -  a'x=\,  bx1  -  b'x=Q  is  (§  417)  that  the  greatest  common  divisor,  say  M,  of  the  p  (2p  -  1) 
binary  determinants  spoken  of  should  divide  each  of  the  2p  integers  b1}  ...,bp'\  if  this 
condition  is  not  already  satisfied  we  may  proceed  as  follows  :  find  two  coprime  integers 
(§  418)  which  satisfy  the  2p  congruences 


i  =0,  \bi+nai  =  0    (mod.  M),  (*=1, 

and  thence  two  integers  p,  a-  such  that  Ao--/*p  =  l  ;   put  Q,±  =\Q.'  +  p.Q,  Q1  = 


i  =  bi\+aifji,  Ai  —  bip  +  aia;  Bi=bl\  +  ain,  .4  /  =  6^  +  0/0-;  then 


and  the  greatest  common  divisor  of  the  p(2p-l}  binary  determinants  AiBj-AjBi, 
AiBj  -Aj'Bi,  A^Bj'-  A-Bi,  which  is  equal  to  M,  divides  the  2jo  integers  £lt  ...,  Bp'; 
thus  M  is  the  greatest  common  divisor  of  these  2p  integers;  next  put  Q2=MQl,  Q^Q/, 
bi  =  Bi/Af,  \>i=BijM,  &i  =  Ai,  aj'=Ji';  then  the  greatest  common  divisor  of  the  p(2p-  1) 
binary  determinants  a^-  —  a,-bi,  etc.,  is  unity,  and  this  is  also  the  greatest  common  divisor 
of  the  2p  integers  bt,  ...,  bp'.  Now  let  (x,  x1}  be  any  solution  of  the  equations  &x'-a'x=l, 
b^-b'^=0,  so  that  (rx  —  b,  rx"  -\j]  is  a  solution  of  the  equations  a£'  —  a'£  =  0,  b£'-b'£=0; 
let  (£»  I')  be  an  independent  solution  of  these  latter  equations  (Smith,  Phil.  Trans.,  CLI. 
(1861),  Art.  4)  so  that  the  p(2p-l)  binary  determinants  #i&-#>&,  etc.,  are  not  all  zero, 
so  chosen  that  the  2p  elements  £,-,  &'  have  unity  as  their  highest  common  divisor;  then  if 
h  be  any  integer,  the  2p  elements  #<+!!&,  a?/  +  h^'  form  a  solution  of  the  equations 
ajcf-&'x=\,  bo/-b'ar=0;  let  h  be  chosen  so  that  the  2p  elements  rxt  -  b<  +  hr£,-  , 
7vr/-b/  +  hr£i'  have  no  common  factor  greater  than  unity  (§  418).  Putting  A"=.r 


676  COMPLETION    OF    DEFECTIVE    ABELIAN   MATRICES.  [420 

2T'=a/+h|',  the  first  column  of  the  matrix  in  §  397  will  consist  of  the  elements  of  (a,  a'), 
the  (p  +  l)th  column  will  consist  of  the  elements  of  (b,  b'),  the  second  column  will 
consist  of  the  elements  of  rJT-b,  rJT'-b';  and  since  these  latter  have  unity  as  their 
greatest  common  factor,  it  is  possible  to  construct  the  (^  +  2)th  and  all  other  columns 
of  this  matrix  (§  420). 

420.  A  theorem  is  assumed  in  §  396,  which  has  an  interest  of  its  own— If  of  an 
Abelian  matrix  of  order  r  there  be  given  the  constituents  of  the  first  r  columns,  and  also  the 
constituents  of  the  (p  +  l)th,  ...,  (p  +  r}th  columns  (r<p\  it  is  always  possible  to  determine 
the  remaining  2(p-r)  columns.  For  a  general  enunciation  the  reader  may  refer  to 
Frobenius,  Crette,  LXXXIX.  (1880),  p.  40.  We  explain  the  method  here  by  a  particular  case  ; 
suppose  that  of  an  Abelian  matrix  of  order  r,  for  p  =  3,  there  be  given  the  first  an 
columns  ;  denote  the  matrix  by 


(  a  x   t 

y?  t' 


b  y   u   ); 
b'  y"  u'  I 


the  elements  of  the  given  columns  will  satisfy  the  relation  ab'-a'b=r ;  it  is  required  to 
determine  in  order  the  second,  the  fifth,  the  third  and  the  sixth  columns ;  the  relations 
arising  from  the  equations 

aa'  —  a'a  =  0,     ftft1  —  ft' ft  =  0,     ap  —  a' ft  =  T 

so  far  as  they  affect  these  columns  respectively,  are  as  follows  : 

ax'-a'x=Q\    .  ay>-a'y  =  Q\  at'-a't  =  Q\  au'-a'u  =  ( 

bx'—b'x  —  O]  by'  —  b'y=0\-  (ii),         bt' —  b't  =  0\     .....          bu' —  b'u  =  ( 

I  r   (111)1  i    /•  \ 

xy'-yfy  =  r]  xt-x't  =  Q\  xu'-afu  =  QY  (iv); 

yt  —  i/t  =  0j  yu'  —  y'u=Q\ 

.  . 

.  .  tu  -  tu  =  r> 

now  let  (x,  x1)  be  a  solution  of  equations  (i)  in  which  the  2p  constituents  have  no  common 
factor  other  than  unity  ;  determine  2  rows  of  p  elements  £,  £'  such  that  xg  —  ofg  =  l,  and 
denote  ag  -  a'£  by  A  and  bg  -  6'|  by  B  ;  then  it  is  immediately  verified  that  the  values 

y  =  r£-(Ab-Ba],    T/ =  rg  -  (AV  -  Ba"), 

satisfy  equations  (ii) ;  next  let  (t,  t)  be  a  solution  of  equations  (iii)  in  which  the  2p 
constituents  have  no  common  factor  other  than  unity  ;  determine  2  rows  of  p  elements, 
u,  v,  such  that  tv  —  t'v  =  l,  and  denote  av'-a'v,  bv'-b'v,  xv'-x'v,  yv'-y'v  respectively  by 
A,  B,  X,  T;  then  it  is  immediately  verified  that  the  values 

u=rv-(Ab-Ba}- (Xy -  Yx\    u1  =  rv' -(Ab'~ Ba') -(Xy'-  IV) 
satisfy  the  equations  (iv). 


INDEX   OF   AUTHORS   QUOTED.      THE   NUMBERS   REFER 

TO   THE   PAGES. 


Abel  90,   173,   205,  206,   207  ff.,   221,   225  ff., 

231,  243,  246,  377,  397,  657 
Appell  200,  392 

Bacharach  141 

Bachmann  666 

Baur  57,  112 

Benoist  153,  156,  222,  647 

Bertini  137 

Biermann  663 

Bobek  647 

Bolza  177,  294,  296,  315,  329,  342,  436,  663 

Borchardt  340,  342,  468 

Bouquet  90 

Braunmiihl  486,  521 

Brill  12,  29,  134,  137,  145,  149,  436,  647 

Brioschi  296,  311,  342,  448,  516,  526,  663,  666 

Briot  90 

Broch  221 

Burkhardt  43,  429,  436,  555,  623,  663 

Burwide  345,  373,  663 

Cantor  239 

Casorati  579 

Caspary  474,  486,  525 

Castelnuovo  647,  665 

Cauchy  600 

Cayley  12,  137,  141,  145,  165,  168,  193,  222, 

230,   283,    296,   340,   342,   374,   387,  459, 

540,  646,  647,  650,  664,  666,  668 
Chasles  137,  647 
Christo/el  666 
Clebsch    131,    142,    153,    156,    165,    168,    183, 

222,   241,   244,   288,   295,   392,   423,   448, 

544,  545,  556,  578,  623,  647 

Darboux  666 
Dedekind  57 
de  Jonquieres  137 


Dersch  647 
Dini  239 
Dirichlet  246,  600 

Eisemtein  246,  674 
Epstein  342 
Euler  159 

Fagnano  638 

Forsyth  2,  3,  7,  9,  10,  13,  14,  15,  16,  21,  24, 
25,  29,  39,  90,  114,  122,  123,  144,  150, 
198,  212,  233,  296,  327,  373,  395,  421, 
439,  441,  442,  445,  459,  531,  577,  578 

Frahm  383 

Fricke  639,  648 

Frobenius  342,  387,  447,  474,  486,  491,  500, 
516,  517,  521,  522,  525,  586,  588,  589, 
598,  628,  629,  630,  632,  633,  666,  668, 
674,  676 

Frost  389 

Fuchs  206,  566 

Gauss  559,  600,  674 

Geiser  383 

Gopel  246,  338,  339 

Gordan   131,    142,    168,    183,    241,   244,    255, 

288,   295,  392,   423,  448,    544,   545,   556, 

578,  623 
Goursat  663 
Grassman  137 
Greenhill  639 
Giinther  174,  189,  200 

Halphen   124,   165,   364,   370,  421,  473,   474, 

639,  665 
Hamburger  2 
Hancock  296,  326 
Harkness  2,   10,   14,   15,   16,  21,  24,   25,    79, 

101,  124,  239,  342 


678 


INDEX    OF   AUTHORS   QUOTED. 


Harnack  222 

Hensel  57,  64,  78,  118 

Hermite   238,   246,   448,   452,    538,   577,  600, 

615,  632,  639,  663,  666.  674 
Hettner  177,  654 
Hilbert  665 

Humbert  222,  255,  340,  486 
Hunoitz  41,  392,  639,  648,  651,  653,  654 

Jacobi    165,  206,  221,  230,  235,  237,  246,  360, 

577,  600,  639,  657 

Jordan  248,  392,  549,  623,  639,  666,  669 
Joubert  639 
Jiirgensen  221 

Kiepert  638,  639 

Klein    9,   25,    156,   159,   169,   177,   342,   343, 

360,   373,   378,   383,   392,   429,  430,  431, 

433,   436,   438,   439,   544,   639,   648,  653, 

654 

Kohn  387 
Konigsberger  337,   342,    448,   459,    477,    529, 

570,  600,  607,  615,  628,  658,  661,  663 
Kowalevski  658,  659,  662,  663 
Krause  296,  342,  468,  486,  600,  623,  674 
Krazer  477,  486,  555,  600,  627 
Kronecker    56,   79,   124,   445,   577,   600,    629, 

631,  639,  666,  669 
Kummer  340 

Lagrange  230 
Laguerre  632,  666 
Lindemann  153,  156,  222,  647 
Liiroth  239 

Malet  663 
Mathews  165 
Minding  221 
Hittag-Leffler  202 

Morley  2,  10,  14,  15,  16,  21,  24,  25,  79,  101, 
124,  239,  342 

Netto  20,  90 

Neumann  14,  17,  169,  296,  531 

Noether  12,  29,  32,  124,  131,  134,  137,  142, 
145,  149,  156,  165,  168,  180,  272,  292, 
295,  390,  392,  430,  486,  522,  544,  566, 
654,  665 

Picard  14,  165,  594,  659 
Pick  360,  430,  639 
Plucker  124,  165 

Poincare  239,  372,  373,  439,  486,  594,  654, 
659,  663 


Pringsheim  445 

Prym  2,   296,   342,    392,  477,   486,   511,  566, 
600,  627 

Richelot  221,  230,  529,  600,  663 

Riemann  1,  2,  6,  9,  13,  45,  47,  77,  113,  115, 

246,  248,  255,  296,  343,  397,  409,  628 
Ritter  360,  373,  392,  429,  439,  442 
Roch  29 
Rosanes  666 
Rosenhain  221,  222,  246,  311,  459,  600,  607, 

628,  662 

Salmon  5,  6,  7,   11,   39,   117,    124,   136,   144, 

159,  165,  267,  383,  389 
Schepp  239 
Sclilafli  666 
Schottky    32,    101,   283,    296,   340,    343,   345-, 

360,   371,   372,   373,   387,   448,   461,  469, 

486,  544,  628 
Schubert  665 
Schwarz  14,  654 
Scott  473 

Smith  12,  600,  639,  666,  674,  675 
Sohnke  639 

Stahl  288,  301,  392,  430,  486,  502 
Stickelberger  666 
Stolz  2 
Sylvester  136 

Taber  668 

Thomae  288,  296,  318,  533,  556,  600 

Thompson  436 

Toeplitz  383 

Valentin  101 

Valentiner  124,  165,  665 

Voss  137 

Weber  8,  56,  270,  272,  373,  387,  392,  430, 
460,  486,  533,  538,  559,  600,  615,  620, 

629,  639,  674 

Weierstrass  32,  93,  99,  101,  177,  195,  197, 
205,  231,  239,  242,  246,  301,  311,  317, 
326,  339,  443,  474,  486,  525,  570,  571, 
572,  573,  577,  579,  594,  628,  653,  654, 
658,  666 

White  165 

Wiltheiss  342,  600,  629,  660,  662,  674 

Wirtinger  340,  486,  578,  628 


TABLE   OF   SOME   FUNCTIONAL   SYMBOLS. 

Riemann's  normal  elementary  integrals 

of  first  kind,  generally,  v*'a,  ...  ,  v*'  a,  p.  15.     For  periods,  p.  16, 

of  second  kind,  T*'  a  ;  periods  of,  fy,  ...  ,  ftp,  or  Qa  (z),  ...  ,  Op  (z),  pp.  15,  21, 

of  third  kind,  II*'",  p.  15. 

Integral,  rational,  functions,  git  or  gt  (x,  y),  or  </;  (y,  x),  pp.  55,  61. 
0-polynomials,  special  functions,  numerators  of  differential  coefficients  of  integrals  of  the  first 

kind,  01}  ...,  #„_!,  p.  61.     Also  01(  ...,  0P,  p.  146. 


Elementary  integral  of  third  kind,  P£«,  p.  68.     (Canonical  integral),  Q*Ba,  p.  185.     (Canonical 

integral),  jR*'c",  p.  ]94. 
Integrals  of  second  kind,  associated  with  given  system  of  integrals  of  first  kind,  L*'a,  p.  193; 

periods  of,  196.    Also  #*•  ",  p.  182,  and  F*  °,  p.  291,  are  used  for  integrals  of  second  kind. 

*(*,  a?   2,  CL  ...,  cp),  pp.  77,   171,   177.      This  is  called  Weierstrass's  fundamental  rational 

function. 

$(x,a;  z,  c),  pp.  174,  175,  178,  200. 
E(x,  z),  pp.  171,  178  (Prime  function). 
E  (x,  z),  pp.  176,  178,  205  (Prime  function). 
Matrices,  see  Appendix  n.,  p.  666. 


;  <?,<?')  ore(M,r    QQ\  or  Q  (  u   \%\  or  0(«;  Q,  Q>) 
\  "  /  \       i  V  / 


(«;  Q,  Q')  or  3 

o 


),  p.  287. 

j\rt 

Pi,  i  (u)  =  -  ^—5^.  Io8  M«).  P-  292.    See  also  p.  516. 

Wi(x)  (Differential  coefficient  of  integral  of  first  kind),  p.  169.     Also  u-  (r)   p  192 

„,-,_,,  p.  192.     ?,.,-,  p.  288. 

W(x,  z;  clt  ...,  <:„),  p.  174. 

™  (f.  7).  P-  360  (Prime  function).    But  for  w  (x,  z),  see  pp.  430  428 

\  (fc  |t),  p.  367. 

|  Q  |,    Q,R  |,  Qj).P.48f, 

*  (u,  a  ;  J),  p.  509. 

0  (u),  a  Jacobian  function,  p.  579,  ff. 

^r(w;  K,  K'  +  fj.),  ^r(ir;  A',  K'  +  /JL),  p.  601. 


SUBJECT  INDEX  TO   THE   PAGES  OF  THIS   VOLUME. 


Abelian  functions,  236,  600,  see  Inversion ;  in 
tegrals,  see  Integrals;  matrix,  669. 

Abel's  theorem,  207,  ff.;  statement  of,  210, 
214 ;  proof  of,  213 ;  number  of  inde 
pendent  equations  given  by,  222  ff. ; 
for  radical  functions,  377 ;  for  factorial 
functions,  397 ;  for  curves  in  space, 
231;  Abel's  proof  of,  219,  220;  con 
verse  of,  222. 

Abel's  differential  equations,  225,  ff. 

Addition  equation  for  hyperelliptic  theta  func 
tions,  deduced  algebraically,  331,  ff. ; 
for  theta  functions  in  general,  457 — 
461,  472,  476,  481,  513,  521. 

Adjoint  polynomial  (or  curve),  definition  of, 
121 ;  number  of  terms  in,  128 ;  ex 
pression  of  rational  function  by,  127  ; 
see  Integrals,  Sets,  Lots. 

Argument  and  parameter,  interchange  of,  16, 
185,  187,  189,  191,  194,  206. 

Associated :  Forms  associated  with  fundamental 
integral  functions,  62 ;  integrals  of 
second  kind  associated  with  integrals 
of  the  first  kind,  193,  195,  198,  532 ; 
associated  system  of  factorial  func 
tions,  397 

Automorphic  functions,  simple  case  of,  352,  ff.; 
connection  with  factorial  functions, 
439,  ff. 

Azygetic  characteristics,  487,  497  ;  transforma 
tion  of,  542,  547  ;  see  Characteristics. 

Bacharach's  modification  of  Cayley's  theorem 
for  plane  curves,  141. 

Biquadratic,  see  Gopel. 

Birational  transformation  of  a  Eiemann  sur 
face  :  does  not  affect  the  theory,  3,  7 ; 
number  of  invariants  in,  9,  144,  148, 
150 ;  of  plane  curves,  11 ;  by  0-poly- 
nomials,  142 — 152  ;  for  hyperelliptic 
surface,  152,  85;  when  p  —  l,  or  0, 


153  ;   of  surface  into  itself,  653.     See 

Invariants,  and  Curves. 

Bitangents  of  a  plane  curve,  381—390;  644, 646. 
Branch  places,  see  Places. 

Canonical  equation  for  a  Kiemann  surface,  83, 
91, 103,  143, 145,  152;  curve  discussed 
by  Klein,  159 ;  integral  of  the  third 
kind,  168,  185,  189,  194,  195. 

Cayley's  theorem  for  plane  curves,  141. 

Characteristics:  of  a  theta  function,  number 
of  odd  and  even,  251;  expression  of 
any  half-integer  characteristic  by 
means  of  a  fundamental  system,  301, 
487,  500,  502;  Weirstrass's  number 
notation  for,  570,  337,  303  ;  tables  of 
half -integer  characteristics  for  p  =  2, 
p  =  3,  303,  305;  syzygetic,  azygetic, 
487;  period  characteristics  and  theta 
characteristics,  543,  564;  of  radical 
functions,  380,  564 ;  Gopel  groups 
and  systems  of,  489,  490,  494,  ff.  ; 
general  theory  of,  486,  ff . ;  transform 
ation  of,  536,  542,  547,  564,  568. 

Coincidences  of  a  correspondence,  645. 

Column  and  row.     See  Matrices. 

Column  of  periods,  571. 

Complex  multiplication  of  theta  functions, 
629,  ff.,  639,  660. 

Composition  of  transformations  of  theta  func 
tions,  551. 

Condition  of  dimensions,  49. 

Confonnal  representation,  343,  356,  372. 

Congruence,  meanings  of  sign  of,  236,  256,  261, 
264,  487. 

Constants,  invariant  in  rational  transformation, 
9,  88,  144,  148,  150 ;  in  linear  trans 
formation  of  theta  functions,  555 — 
559;  in  any  transformation  of  theta 
functions,  620,  622. 

Contact  curves,  see  Curves,  and  Radical. 


SUBJECT    INDEX   TO   THE    PAGES   OF   THIS   VOLUME. 


681 


Convergence  of  an  automorphic  series,  350; 
of  transformed  theta  function,  538. 

Coresidual  sets  of  places  on  a  Riemann  surface, 
135,  ff.,  213;  are  equivalent  sets,  136; 
enter  in  statement  of  Abel's  theorem, 
210. 

Correspondence  of  Riemann  surfaces,  3,  ff., 
81,  639,  642,  647,  648,  649,  654,  662. 

Covariant,  see  Invariant. 

Cubic  surface  associated  with  a  plane  quartic 
curve,  382,  389. 

Curves :  as  alternative  interpretation  of  fun 
damental  algebraic  equation,  11 ;  in 
flexions  of  a  plane  quartic  in  con 
nection  with  the  gap  theorem,  36 ; 
generalisation,  40 ;  inflexions  and 
bitangents  in  connection  with  theory 
of  correspondence,  644, 646 ;  bitaugents 
of  a  plane  quartic  curve,  384 ;  adjoint 
curves,  121,  129  ;  coresidual  and 
equivalent  sets  upon,  134 — 136  ;  trans 
formation  of,  see  Birational,  In 
variants,  and  Constants ;  correspon 
dence  of,  see  Correspondence ;  special 
sets  upon,  146,  ff.;  contact  curves, 
381 ;  general  form  of  Pliicker's  equa 
tions  for,  124 ;  Weierstrass's  canon 
ical  equation  for,  93,  103 ;  Cayley's 
theorem  for,  141 ;  curves  in  space,  157, 
160,  ff.,  166,  664;  Abel's  theorem  for, 
231. 

Cusps,  11,  114. 

Deficiency  of  a  Riemann  surface,  7,  55,  60. 
Denning  relation  for  theta  functions,  443. 
Definition  equation  of  theta  functions  of  general 

order,  448. 

Degenerate  Abelian  integrals,  657. 
Dependence  of  the  poles  of  a  rational  function, 

27. 
Differential  equations  of   inversion    problem, 

'225,  ff. ;    of  theta  functions,  see  Ad 
denda  (p.  xx). 
Differentials  of  integrals  of  first  kind,  25,  62, 

67,  127,  169. 
Dimension  of  an  integral  function,  48,  ff.,  55 ; 

condition  of  dimensions,  49. 
Discriminant  of  a  fundamental  set  of  integral 

functions,  74,  101,  124. 
Dissection  of  the  Riemann  surface,  26,   529, 

253,  257,  569,  297,  550,  560. 
Double  points  of  a  Riemann  surface  (or  curve), 

1,  2,  3,  11,  114;  tangents  of  a  plane 

curve,  644,  646. 


Elementary  integrals,  see  Integrals. 

Equivalence,  meanings  of  sign  of,  236,  256, 
261,  264,  487. 

Equivalent  sets  of  places  on  a  Riemann  sur 
face,  134,  ff.,  136,  213. 

Essential  factor  of  the  discriminant,  60,  74,  124. 

Existence  theorems,  algebraically  deducible, 
78 ;  references,  14. 

Expression  of  any  rational  function,  77,  176, 
212 ;  of  fundamental  integral  func 
tions,  105,  ff. ;  of  half-integer  charac 
teristic  by  means  of  a  fundamental 
system,  301,  487,  500,  502. 

Factorial  functions,  392,  ff.;  definition  of,  396; 
which  are  everywhere  finite,  399;  ex 
pressed  by  factorial  integrals,  403 ; 
expressed  by  fundamental  factorial 
function,  413;  with  fewest  poles,  406; 
used  to  express  theta  functions,  423, 
426 ;  connection  with  automorphic 
functions,  439,  ff. 

Factorial  integrals,  398  ;  which  are  everywhere 
finite,  399  ;  fundamental,  having  only 
poles,  408 ;  simplified  form  of  that 
integral,  411  ;  expression  of  factorial 
function  by  means  of  that  integral, 
412. 

Function,  automorphic,  352,  ff.,  439,  ff.;  fac 
torial,  see  Factorial ;  integral,  see 
Rational,  and  Transcendental ;  ^  func 
tion,  292,  324,  333,  516  ;  prime,  172, 
177,  205,  also  360,  363,  428 ;  radical, 
374,  390,  565 ;  rational,  see  Rational ; 
Theta,  see  Theta  functions,  and 
Transformation  ;  I  function,  287,  292, 
320  ;  see  Fundamental  rational. 

Fundamental  algebraical  equation,  10,  113. 

Fundamental  rational  function,  Weierstrass's, 
171,  175,  177,  178,  ff.,  182. 

Fundamental  set  for  the  expression  of  rational 
integral  functions,  48,  ff.,  55,  56,  57, 
105,  ff. 

Fundamental  system  of  theta  characteristics, 
301,  487,  500,  502. 

Gap  theorem,  32,  34,  93,  174. 

Geometrical  investigations,  113;  see  Curves. 

Go'pel   biquadratic   relation,  338 — 340  ;    465 — 

468  ;  see  Addenda  (p.  xx). 
Gopel  group  and  system,  see  Characteristics. 
Grade,  of  a  polynomial,  120. 
Group,  Gopel,  see  Characteristics. 


B. 


44 


682 


SUBJECT   INDEX   TO   THE   PAGES   OF  THIS   VOLUME. 


Hensel's  determination  of  fundamental  integral 
functions,  105,  ff. 

Homogeneous  variables,  118,  441. 

Homographic  behaviour  of  differentials  of  in 
tegrals  of  first  kind,  26. 

Hyperelliptic  surfaces,  80,  ff.,  152,  153,  373; 
see  Theta  functions  and  Transforma 
tion. 

Independence  of  the  poles  of  a  rational  func 
tion,  27;  of  the  22p  theta  functions 
with  half-integer  characteristics,  446, 
447 ;  See  Linearly. 

Index  of  a  place  on  a  Riemann  surface,  122, 
123,  124;  at  the  infinite  place  of 
Weierstrass's  canonical  surface,  129. 

Infinitesimal  on  a  Riemann  surface,  1,  2,  3. 

Infinitesimal  periods,  238,  573. 

Infinities  of  rational  function,  27,  ff.;  see 
Residue. 

Infinity,  the  places  at  infinity  on  a  Riemann 
surface,  algebraic  treatment  of,  118. 

Inflexions  of  a  plane  curve,  36,  40,  646. 

Integrals,  degenerate,  657;  factorial,  see  Fac 
torial;  Riemann's,  normal  elementary, 
15 ;  all  derivable  from  integral  of  third 
kind,  22 ;  algebraic  expression  of,  65, 
ff.,  127,  131,  163,  185,  189,  194; 
hyperelliptic,  195  ;  formulae  connect 
ing  with  logarithmic  differential  coeffi 
cients  of  theta  functions,  289, 290,320. 

Integral  functions,  see  Rational  and  Transcen 
dental. 

Interchange  of  argument  and  parameter,  16, 
185,  187,  189,  191,  194,  206;  of  period 
loops,  see  Transformation. 

Invariants  in  birational  transformation:  the 
number  p,  7;  the  3p-3  moduli,  9, 
144,  148,  150;  the  ratios  of  ^-poly 
nomials,  26,  153 ;  the  contact  <f>- 
polynomials,  281,  427;  the  0-places, 
38,  653;  for  transformation  of  the 
dependent  variable,  74,  124. 

Inversion  theorem,  Jacobi's,  235,  ff.,  270; 
solution  of,  239,  242,  244,  275;  by 
radical  functions,  390;  in  the  hyper 
elliptic  case,  317,  324. 

Jacobi's  inversion  theorem,  see  Inversion. 

Jacobian  functions,  their  periods,  are  generali 
sation  of  theta  functions,  579 — 588; 
their  expression  by  theta  functions, 
588 — 594 ;  there  exists  a  homogeneous 
polynomial  relation  connecting  any 


p  +  2    Jacobian    functions    of    same 
periods  and  parameter,  594. 

Klein,  prime  form,  360,  427,  430,  433. 

Laurent's  theorem,  for  p  variables,  444. 

Left  side  of  period  loop,  529. 

Linearly  independent  ^-products  of  order  /u, 
154;  columns  of  periods,  575;  theta 
functions,  446,  447;  Jacobian  func 
tions,  594. 

Linear  transformation,  see  Transformation. 

Loops,  period  loops  on  a  Riemann  surface,  21, 
529. 

Lots,  of  sets  of  places  on  an  algebraic  curve, 
or  Riemann  surface,  135. 

Matrices,  248,  283,  580,  666,  669. 
Mittag-Leffier's  theorem  for  uniform  function 

on  a  Riemann  surface,  202. 
Moduli,  of  the  algebraic  equation,  are  3p  -  3  in 

number,   9,    144,    148,    150;    for   the 

hyperelliptic  equation,  88. 
Moduli  of  periodicity,  see  Periods. 
Multiplication,   complex,    of  theta   functions, 

629,    ff. ;    by   an    integer,    for    theta 

functions,  527. 

Multiply-periodic,  236 ;  see  Inversion. 
Noether's  (Kraus's)  0-curve  in  space,  156,  157. 
Normal  equation  for  a  Riemann  surface,  83, 

91,  103,  143,  145,  152. 
Normal  integrals  (Riemann's)  see  Integrals. 
Number  of  independent  products  of  /j.  0-poly- 

nomials,  154;  of  odd  and  even  theta 

functions,  251 ;  of  theta  functions  of 

general  order,  452,  463;   of  Jacobian 

functions,  594. 

Order  of  small  quantity  on  a  Riemann  surface,  2; 
of  a  theta  function,  448. 

#>  Function,  292,  324,  333,  516. 

Parameter,  interchange  of  argument  and  para 
meter,  see  Interchange. 

Parameters,  in  the  algebraic  equation,  see 
Constants. 

Period  loop,  see  Loops. 

Period  characteristics,  see  Characteristics. 

Periodicity  of  a  (1,  1)  correspondence,  650. 

Periods  of  Riemann's  integrals,  16,  21 ;  Rie 
mann's  and  Weierstrass's  relations  for 
the  periods  of  integrals  of  the  first 
kind,  and  of  associated  integrals  of 
the  second  kind,  197,  285,  581,  587  ; 


SUBJECT   INDEX  TO   THE   PAGES   OF  THIS   VOLUME. 


683 


rule  for  half-periods  on  a  hyperelliptic 
surface,  297  ;  for  integrals  of  second 
kind,  323  ;  of  factorial  integrals,  404 ; 
linear  transformation  of  periods,  532  ; 
general  transformation,  536,  538 ; 
general  theory  of  systems  of  periods, 
571,  ff.,  579,  ft". ;  of  degenerate  inte 
grals,  657. 

Picard's  theorem  (Weierstrass's),  G58. 

Places,  of  a  lliemann  surface,  1,  2,  3  ;  branch 
places,  7,  9,  46,  74,  122,  297,  569; 
where  a  rational  fiinction  is  infinite, 
to  order  less  than  p  +  l,  38,  41,  90, 
653; 

the  places  mlt  ...,  m}> ,  255 ;  their  geo 
metrical  interpretation,  265,  2G6 ;  after 
linear  transformation,  562 ;  deter 
mination  of,  for  a  Riemann  surface 
with  assigned  period  loops,  567  ;  for  a 
hyperelliptic  surface,  297,  563. 

Plucker's  equations,  generalised  form  of,  123, 
124  ;  for  curves  in  space,  166. 

Poles,  see  Infinities. 

Polynomial,  grade  of,  120 ;  algebraic  treat 
ment  of,  120;  adjoint,  121,  128; 
0-polynomials,  141 ;  transformation 
of  fundamental  equation  by  ^-polyno 
mials,  142, 154  ;  expression  of  rational 
functions,  and  algebraic  integrals  by 
means  of  adjoint  polynomials,  156 ; 
see  Curves. 

Positive  direction  of  period  loop,  529. 

Primary  and  associated  systems  of  factorial 
functions,  397. 

Prime  function  (or  form),  see  Function. 

Product  expression  of  uniform  transcendental 
function  with  single  essential  singu 
larity,  205. 

Quartic.     Double  tangents    of    plane   quartic 

curve,  381—390,  647. 
Quotients   of  theta   functions,   310,  311,  390, 

426,  516. 

Radical  function,  see  Function. 

Rational  function,  of  order  1,  only  exists  when 
p  =  0,  8 ;  is  an  uniform  function  on  the 
Riemann  surface  whose  only  infinities 
are  poles,  27  ;  infinities  of,  Riemann  - 
Iloch  theorem,  Weierstrass's  gap  theo 
rem,  27,  ff. ;  special,  25,  137  ;  of  order 
p,  38,  137;  integral  function,  47,  ff., 
55,  91,  ff. ;  of  the  second  order,  80,  ff. ; 
fundamental  integral  rational  func 


tions,  algebraic  determination  of,  105, 
ff. ;  algebraic  expression  of,  by  adjoint 
polynomials,  125,  ff.,  156 ;  Weier 
strass's  fundamental,  171,  175,  177, 
178,  ff.,  182  ;  expressed  by  Riemann's 
integrals,  24, 212  ;  expressed  by  Weier 
strass's  function,  176. 

Reciprocal  sets  of  zeros  of  adjoint  polynomials, 
134. 

Residual  sets  of  places,  135. 

Residue,  fundamental  residue  theorem,  232, 
189,  20. 

Reversible  transformation,  see  Birational. 

Riemann-Roch  theorem,  44,  133 ;  for  factorial 
functions,  405. 

Riemann  and  Weierstrass's  period  relations, 
197,  285,  581,  587. 

Right  side  of  period  loop,  529. 

Row  and  column,  see  Matrices 

Schottky- Klein  prime  form  and  function,  360, 

427,  430,  433. 

Sequence,  theorem  of,  114,  161,  165. 
Sequent  sets  of  places,  135. 
Sets  of  places  on  a  Riemann  surface  or  algebraic 

curve,  135.     See  Special. 
Sign  of  equivalence  and  congruence,  236,  256, 

261,  264,  487. 
Special  correspondences  on  a  Riemann  surface, 

648. 

Special  rational  functions,  25,  62,  137. 
Special  sets  of  zeros  of  adjoint  polynomials, 

134,  147. 
Special   transformation   of   a   theta   function, 

629,  ff. ,  639,  660. 
Strength  of  assigned  zeros,  as  determinators  of 

a  polynomial,  133. 
Supplementary    transformations    of    a    theta 

function,  552. 

System,  Gopel,  see  Characteristics. 
Syzygetic  characteristics,  487,  542. 

Tables  of  Characteristics,  303,  305. 

Tangents,  double,  of  a  plane  curve,  by  the 
principle  of  correspondence,  644,  646. 

Theta  functions : 

Riemann's  theta  functions,  246,  ff.  ;  con 
vergence  of,  247;  determination  of, 
from  periodicity,  444 ;  period  proper 
ties  of,  249;  number  of  odd  and  even, 
251,  446;  zeros  of,  252,  255,  258,  567; 
identical  vanishing  of,  258,  271,  276, 
303;  hyperelliptic,  296,  ff. ;  algebraic 
expression  of  quotients  of,  310,  311, 


684 


SUBJECT   INDEX   TO  THE   PAGES   OF   THIS   VOLUME. 


390,  426 ;  addition  theorem  for  hyper- 
elliptic,  332,  337;  algebraic  expression 
for  hyperelliptic,  435;  algebraic  ex 
pression  of  first  logarithmic  derivatives 
of,  288,  290,  320;  algebraic  expression 
of  second  logarithmic  derivatives  of, 
293,  324,  329,  333 ;  solution  of  inver 
sion  problem  by  means  of,  275,  324, 
390,  426,  ff . ;  Kiemann's  functions  not 
the  most  general,  248,  628. 

General  theta  function  of  first  order,  283, 
444;  period  relations,  285,  197,  581, 
587;  second  logarithmic  derivatives 
of,  516;  addition  theorems  for,  457, 
472,  481,  513,  521 ;  Gopel  relation  for, 
in  case  p  =  2,  see  Gopel;  expression 
of  Jacobian  functions  by  means  of, 
594. 

Theta  functions  of  second  and  higher  order, 
448 ;  expression  of,  number  of  linearly 
independent,  452,  463;  of  order  2,  of 
special  kind,  509,  510;  every  p  +  2 
theta  functions  of  same  order,  periods, 
and  characteristic,  connected  by  a 
homogeneous  polynomial  relation,  453. 

Transformation  of  theta  functions,  see 
Transformation ;  characteristics  of 
theta  functions,  see  Characteristics ; 
complex  multiplication  of  theta  func 
tions,  629,  ff.,  639,  660;  theta  func 
tions  expressed  by  factorial  functions 
and  simpler  theta  functions,  426; 
particular  cases,  430,  ff . ;  hyperelliptic 
case,  433. 

Transcendental  uniform  function,  200 ;  Mittag- 
Leffler's  theorem  for,  202;  expressed 
in  prime  factors,  205;  application  of 
Laurent's  theorem  when  the  function 
is  integral,  444. 


Transformation 

of  the  algebraic  equation  (or  Kiemann 
surface),  3,  143,  145,  151,  152,  654, 
655 ;  see  Birational ; 

of  theta  functions,  535;  linear  trans 
formation,  539;  constants  in,  554 — 
559;  for  hyperelliptic  case,  568;  of 
second  order,  603,  617;  for  any  odd 
order,  general  theorem,  614;  con 
stants  in,  620,  622;  when  coefficients 
not  integers,  625 ;  supplementary 
transformations,  552 ;  composition  of, 
551;  special  transformations,  629, 
630,  660; 

of  periods,  528,  534,  539,  551,  553,  555, 
559,  568; 

of  characteristics,  see  Characteristics. 

Uniform,  see  Rational,  and  Transcendental. 

Vanishing  of  theta  function,  253,  258,  271  ff., 

276,  303. 
Variables,  homogeneous,  118,  429,  441  _ 

\ — / 

Weierstrass's  gap   theorem,  32,  34,   93,  174; 

special  places  which  are  the  poles  of 
rational  functions  of  order  less  than 
p  +  l,  34,  ff . ;  canonical  surface  (or 
equation),  90,  ff.,  93;  fundamental 
rational  function,  171,  175,  177,  178, 
182,  189;  period  relations,  197,  ff., 
285,  581,  587;  rule  for  characteristics 
of  hyperelliptic  theta  functions,  569  ; 
theorem  for  degenerate  integrals,  658. 

Zeros,  generalised  zeros  of  a  polynomial,  121 ; 

zeros    of    Eiemann    theta    function, 

252. 
Zeta  function,  287,  292,  320. 


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